View/edit a dataset - magnetochronology/all

This page allows you to view all the information for a dataset, or subdataset, i.e. for a set of events and the intervals that they define, including the definitions of the basal events and the data used to set their age. The intervals table can show two levels of intervals, such as zones and sub-zones, or stages and sub-stages. The events table shows all the events in the dataset, including for example taxon events not used as markers of the base of intevals. page. On this page codes such as TAsZ (Tethyan Ammonite subZone) which are added to interval and/or event names to make them unique are shown. To see the data as it appears on TSC, and without those codes use the column view page

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Dataset selected - magnetochronology

Columns in the dataset
intervals - coloured: Polarity chrons,
intervals: Chron Label , Series Label,
events: Geomagnetic Excursions during Quaternary Period,

Dataset metadata

Name: id:4 sort: 300 Dataset type: Data types:
TSC_source_notes:
compilation_notes:
Cenozoic notes &
compilation notes
Cretaceous notes &
compilation notes
Jurassic notes &
compilation notes
Triassic notes &
compilation notes
Permo-Carboniferous notes &
compilation notes
Devonian notes &
compilation notes
Silurian-Ordovician notes &
compilation notes
Cambrian notes &
compilation notes
refs to add:
Linked refs:Cande & Kent 1995;Hansma et al. 2015;Hounslow & Balabanov 2018;Hounslow & Muttoni 2010;Hounslow 2020;Husson et al. 2011;Kent et al. 2018;Ogg 2020;Steiner 2006;Thibault et al. 2012;Zhang et al. 2020;
Interval Colour:
Event Colour:
Added abbreviations:
interval types:Main interval type:
prefix(es):

Missing references:Chanell et al. 2020; Li 2016; Yan Chen 2020; sorry, these are not in the bibliography yet insert new entry

subintvtype:subchron

chrons and subchrons in the magnetochronology dataset

age range: -->500
intervaldurationinterval notessub-intervaldurationnotesbasal event base agepupwithin_intvoffsetoffset fromevent notescompilation notesstage
C1n0.7728C1n (Brunhes) 0.7728Matuyama Reversed incudes all of C1r & C2, and contains 4 brief normals - Jaramillo, Cobb Mountain, Olduvai & Fenibase C1n0.773000.0000Chron C1n (= Brunhes Normal) base is in the upper (younger) part of Oxygen isotopic stage 19; with astrochronology age of 773 +/- 1 ka (Channell et al., 2010; reviewed by Singer, 2014). Base of Middle Pleistocene (= base of Ionian Stage) = base of Brunhes Chron.Chibanian
C1r.1r (Matuyama) 0.2170Matuyama Reversed incudes all of C1r & C2, and contains 4 brief normals - Jaramillo, Cobb Mountain, Olduvai & Fenibase C1r.1r0.99000990 +/-4 ka; and base of MIS 27 (Channell et al., 2020)Calabrian
C1r.1n (Jaramillo) 0.0800Jaramillo Normal is a brief normal within the Matuyama Reversedbase C1r.1n1.07000Chron C1r.1n (= Jarmallo Normal) top coincides with Oxygen isotope stage 27, and base is in stage 31. 1070 +/-3 ka (MIS 31; and dated lavas in Tahiti; Channell et al., 2020)Calabrian
C1r.2r (Matuyama continued) 0.1100base C1r.2r1.18000End of the Cobb Mountain excursion in ODP/IODP records is approximately 1178 ka (reviewed in Channell et al., 2020)Calabrian
C1r.2n (Cobb Mountain) 0.0350Cobb Mountain cryptochron is a brief normal within the Matuyama Reversedbase C1r.2n1.21500Excursion named after Alder Creek rhyolite at Cobb Mountain (California) is near MIS36/37 boundary with onset in ODP/IODP cores at 1215 ka. Set sa polarity chron C1r.2r (="C1r.2r-1n" of Cande-Kent nomenclature). Marine cyclostratigraphy indicates a 30 kyr duration. Ar-Ar dating of base and top are summarized in Singer (2014) and Channell et al. (2020)Calabrian
C1r0.9970C1r.3r (Matuyama continued) 0.5550base C11.77000In MIS 63. Astrochronology at ODP Site 677 (1.77 Ma) is consistent with that of Italan land sections (1.79 Ma) (Channell et al., 2020)Calabrian
C2n0.1550C2n (Olduvai) 0.1550Olduvai Normal is a brief normal within the Matuyama Reversedbase C2n1.92500Chron C2n (= Olduvai Normal). "Near LAD of Discoaster brouweri and MIS 71/72 transition.""Site U1308 result implies an age for the base Olduvai, on the LR04 timescale, of 1925 ka"" (review by Channell et al., 2020, of difficulties dating the onset)". Ar-Ar dating agrees with astronomical-cycles (e.g., Channell, 2002).Gelasian
C2r.1r (Matuyama continued) 0.1910base C2r.1r2.116000.0000Gelasian
C2r.1n (Feni) 0.0240Feni Normal is a brief normal within the Matuyama Reversedbase C2r.1n2.140000.0000C2r.1n was formerly named Reunion; but the type location was discovered to be a brief excursion before the main Normal; therefore Singer (2014) recommended Feni be used after the documented extent and age-control at Feni Drift ODP Site 981 in North Atlantic (Channell et al., 2003). Reunion "upper" excursion suggested from Reunion island volcanics in Indian Ocean, is now best documented at Feni Drift ODP Site 981as spanning ca. 2.140 to 2.116 Ma (25 kyr)Gelasian
C2r0.6700C2r.2r (Matuyama continued) 0.4550base C22.595000.0000Gelasian
C2An.1n (Gauss) 0.4370Gauss Normal spans all of C2An, and contains two brief reversed-polarity intervals -- Kaena (2An.1r) and Mammoth (2An.2r)base C2An.1n3.032000.0000Chron C2r/C2An boundary (= Matuyama Reversed/Gauss Normal boundary) coincides with Oxygen isotope stage 103-104 boundary. "Gauss Normal Chron" (C2An) contains two reversed intervals -- Kaena (2An.1r) and Mammoth (2An.2r). Polarity chron C2An.1n -- Top (= top of Gauss) is 2.581 Ma in Cande-Kent’95 (used here), vs. 2.60 in Hilgen ’91. This 2.581 Ma age (Gauss/Matuyama boundary) was by Langereis, van Hoof & Hilgen (1994, Nature 369: 615).Piacenzian
C2An.1r (Kaena) 0.0840Kaena Reversed is a brief reversed interval with the Gauss Normalbase C2An.1r3.11600Chron C2An.1r (Kaena Reversed) top coincides with Oxygen isotope stage G21-G22 boundary; and base with K3-KM2 boundary.Piacenzian
C2An.2n (Gauss continued) 0.0910base C2An.2n3.20700Piacenzian
C2An.2r (Mammoth) 0.1230Mammoth Reversed is a brief reversed interval with the Gauss Normalbase C2An.2r3.33000 Chron C2An.2r (Mammoth Reversed) top coincides with Oxygen isotope stage KM6; and base with stage MG1.Piacenzian
C2An1.0010C2An.3n (Gauss continued) 0.2660base C2An.3n3.59600Base of Piacenzian is base of Chron C2An.3nPiacenzian
C2Ar0.5910C2Ar (Gilbert) 0.5910Gilbert Reversed Chron" spans Chrons C2Ar throug C3r and contains 4 brief normal intrvals - Cochiti, Nunivak, Sidufjall & Thverabase C2A4.18700Gilbert Reversed Chron" spans Chrons C2Ar throug C3r. Chron C2An/C2Ar boundary (= Gauss Normal/Gilbert Reversed boundary) coincides with Oxygen isotope stage MG6-Gi1 boundary.Zanclean
C3n.1n (Cochiti) 0.1130Cochiti Normal [in Gilbert Reversed, which spans C2Ar through C3r)base C3n.1n4.30000 Chron C3n.1n (Cochiti Normal) top coincides with Oxygen isotope stage Co1-Co2 boundary; and base with stage CN1.Zanclean
C3n.1r (Gilbert continued) 0.1930base C3n.1r4.49300Zanclean
C3n.2n (Nunivak) 0.1380Nunivak Normalbase C3n.2n4.63100 Chron C3n.2n (Nunivak Normal) top coincides with Oxygen isotope stage N1-N2 boundary; and base with stage N7-N8 boundary.Zanclean
C3n.2r (Gilbert continued) 0.1680base C3n.2r4.79900Zanclean
C3n.3n (Sidufjall) 0.0970Sidufjall Normalbase C3n.3n4.89600 Chron C3n.3n (Sidufjall Normal) top coincides with Oxygen isotope stage Si1-Si2 boundary; and base with stage Si6.Zanclean
C3n.3r (Gilbert continued) 0.1010base C3n.3r4.99700Zanclean
C3n1.0480C3n.4n (Thvera) 0.2380Thvera Normalbase C3n.4n5.23500Chron C3n.4n (Thvera Normal) top coincides with Oxygen isotope stage T1; and base with stage TG2.Zanclean
C3r0.7880C3r ((Gilbert continued) 0.7880Base of polarity chron C3r is an alternate definiton for base of Pliocenebase C36.02300Messinian
C3An.1n 0.2490Polarity chrons C3A through C5Bn have been scaled to fit astronomically calibrated Miocene/Pliocene boundary (5.32 Ma).base C3An.1n6.27200Messinian
C3An.1r 0.1140base C3An.1r6.38600Messinian
C3An0.7040C3An.2n 0.3410base C3An.2n6.72700Messinian
C3Br.1r 0.0480Base of Messinian is in lowermost Chron C3Br.1rbase C3Br.1r7.26200Messinian
C3Br.1n 0.0430base C3Br.1n7.30500Tortonian
C3Br.2r 0.1510base C3Br.2r7.45600Tortonian
C3Br.2n 0.0430base C3Br.2n7.49900Tortonian
C3Br0.3230C3Br.3r 0.0380base C3B7.53700Tortonian
C4n.1n 0.1130base C4n.1n7.65000Tortonian
C4n.1r 0.0510base C4n.1r7.70100Tortonian
C4n0.5880C4n.2n 0.4240base C4n.2n8.12500Tortonian
C4r.1r 0.1320base C4r.1r8.25700Tortonian
C4r.1n 0.0430base C4r.1n8.30000Tortonian
C4r0.6460C4r.2r 0.4710base C48.771000.0000Tortonian
C4Ar.1r 0.2060base C4Ar.1r9.31100Tortonian
C4Ar.1n 0.1150base C4Ar.1n9.42600Tortonian
C4Ar.2r 0.2210base C4Ar.2r9.64700Tortonian
C4Ar.2n 0.0740base C4Ar.2n9.72100Tortonian
C4Ar0.6810C4Ar.3r 0.0650base C4A9.78600Tortonian
C5n.1n 0.1510base C5n.1n9.93700Tortonian
C5n.1r 0.0470base C5n.1r9.98400Tortonian
C5n1.2700C5n.2n 1.0720base C5n.2n11.05600Tortonian
C5r.1r 0.0900base C5r.1r11.14600Tortonian
C5r.1n 0.0420base C5r.1n11.18800Tortonian
C5r.2r 0.4040base C5r.2r11.59200Tortonian
C5r.2n 0.0650base C5r.2n11.65700Base of Tortonian = base of Chron C5r.2nTortonian
C5r0.9930C5r.3r 0.3920base C512.04900Tortonian
C5An.1n 0.1250base C5An.1n12.17400Serravallian
C5An.1r 0.0980base C5An.1r12.27200Serravallian
C5An0.4250C5An.2n 0.2020base C5An.2n12.47400Serravallian
C5Ar.1r 0.2610base C5Ar.1r12.73500Serravallian
C5Ar.1n 0.0350base C5Ar.1n12.77000Serravallian
C5Ar.2r 0.0590base C5Ar.2r12.82900Serravallian
C5Ar.2n 0.0580base C5Ar.2n12.88700Serravallian
C5Ar0.5580C5Ar.3r 0.1450Ref "19" refers to Lourens et al. (GTS2004) interpolating ages of magnetic chrons using a smoothed spreading model from 13.0 Ma to base of Miocene (23.0 Ma)base C5A13.03200Serravallian
C5Bn.1n 0.0950base C5Bn.1n14.87000Langhian
C5Bn.1r 0.1700base C5Bn.1r15.04000Langhian
C5Bn0.4110C5Bn.2n 0.1460base C5Bn.2n15.18600Langhian
C5Cn.1n 0.2670base C5Cn.1n16.26100Burdigalian
C5Cn.1r 0.0900base C5Cn.1r16.35100Burdigalian
C5Cn.2n 0.0830base C5Cn.2n16.43400Burdigalian
C5Cn.2r 0.0980base C5Cn.2r16.53200Burdigalian
C5Cn0.6430C5Cn.3n 0.1050base C5Cn.3n16.63700Burdigalian
C5Dr.1r 0.1680base C5Dr.1r17.63400Burdigalian
C5Dr.1n 0.0420C5Dr.1n is a Crptochron within C5Drbase C5Dr.1n17.67600Burdigalian
C5Dr0.5410C5Dr.2r 0.3310base C5D18.00700Burdigalian
C6An.1n 0.2030base C6An.1n20.18200Burdigalian
C6An.1r 0.2660base C6An.1r20.44800Burdigalian
C6An0.7860C6An.2n 0.3170base C6An.2n20.76500Burdigalian
C6AAr.1r 0.2370base C6AAr.1r21.44100Aquitanian
C6AAr.1n 0.0780base C6AAr.1n21.51900Aquitanian
C6AAr.2r 0.1720base C6AAr.2r21.69100Aquitanian
C6AAr.2n 0.0310base C6AAr.2n21.72200Aquitanian
C6AAr0.6020C6AAr.3r 0.0840base C6AA21.80600Aquitanian
C6Bn.1n 0.1790base C6Bn.1n21.98500Aquitanian
C6Bn.1r 0.0570base C6Bn.1r22.04200Aquitanian
C6Bn0.5360C6Bn.2n 0.3000base C6Bn.2n22.342000.0000Aquitanian
C6Cn.1n 0.1710base C6Cn.1n22.79200Aquitanian
C6Cn.1r 0.1810base C6Cn.1r22.97300Aquitanian
C6Cn.2n 0.0670base C6Cn.2n23.04000Oligocene/Miocene boundary = base of C6Cn.2n = 23.8 Ma = age calibration point of Cande and Kent (1992)Aquitanian
C6Cn.2r 0.1720base C6Cn.2r23.21200Chattian
C6Cn0.6970C6Cn.3n 0.1060base C6Cn.3n23.31800Aquitanian
C7n.1n 0.0360base C7n.1n24.06100Chattian
C7n.1r 0.0630base C7n.1r24.12400Chattian
C7n0.4340C7n.2n 0.3350base C7n.2n24.45900Chattian
C8n.1n 0.1650base C8n.1n25.26400Chattian
C8n.1r 0.0400base C8n.1r25.30400Chattian
C8n0.8880C8n.2n 0.6830base C8n.2n25.98700Chattian
C10n.1n 0.2280base C10n.1n28.08700Rupelian
C10n.1r 0.0540base C10n.1r28.14100Rupelian
C10n0.4190C10n.2n 0.1370base C10n.2n28.27800Rupelian
C11n.1n 0.2940base C11n.1n29.47700Rupelian
C11n.1r 0.0500base C11n.1r29.52700Rupelian
C11n0.7870C11n.2n 0.4430base C11n.2n29.97000Rupelian
C16n.1n 0.1380base C16n.1n35.71800Priabonian
C16n.1r 0.0560base C16n.1r35.77400Priabonian
C16n0.7710C16n.2n 0.5770base C16n.2n36.35100Priabonian
C17n.1n 0.8120base C17n.1n37.38500Base of Priabonian (working version in GTS2012) was assigned here as base of Chron C17n.1nPriabonian
C17n.1r 0.1450base C17n.1r37.53000Priabonian
C17n.2n 0.2510base C17n.2n37.78100Priabonian
C17n.2r 0.0770base C17n.2r37.85800Bartonian
C17n1.5080C17n.3n 0.2230base C17n.3n38.08100Priabonian
C18n.1n 1.1840base C18n.1n39.58200Bartonian
C18n.1r 0.0840base C18n.1r39.66600Bartonian
C18n1.6750C18n.2n 0.4070base C18n.2n40.07300Bartonian
C23n.1n 0.2290base C23n.1n50.99600Ypresian
C23n.1r 0.0510base C23n.1r51.04700Ypresian
C23n0.9570C23n.2n 0.6770base C23n.2n51.72400Ypresian
C24n.1n 0.3900base C24n.1n52.93000Ypresian
C24n.1r 0.0900base C24n.1r53.02000Ypresian
C24n.2n 0.1000base C24n.2n53.12000Ypresian
C24n.2r 0.1300base C24n.2r53.25000Ypresian
C24n1.3600C24n.3n 0.6500base C24n.3n53.90000Ypresian
M20n.1n 0.3268base M20n.1n144.29480.7M20nTithonian
M20n.1r 0.0561base M20n.1r144.35090.65M20nTithonian
M20n1.0785M20n.2n 0.6956base M20n145.04650.38M20Tithonian
M22n.1n 1.2916base M22n.1n148.30060.13M22n0.0000Tithonian
M22n.1r 0.0431base M22n.1r148.34370.1M22nTithonian
M22n.2n 0.0460base M22n.2n148.38970.07M22n0.0000Tithonian
M22n.2r 0.0414base M22n.2r148.43110.04M22n0.0000Tithonian
M22n1.4846M22n.3n 0.0625base M22n148.49360.29M22Tithonian
M23r.1r 0.3076base M23r.1r150.13530.7M23rKimmeridgian
M23r1.0253M23r.1n 0.0287base M23r150.85300M23Kimmeridgian
M24r.1r 0.5150base M24r.1r151.63270.33M24rKimmeridgian
M24r0.7733M24r.1n 0.0286base M24r151.89100M24Kimmeridgian
M25An.1n 0.1318base M25An.1n153.57380.69M25AnKimmeridgian
M25An.1r 0.0686base M25An.1r153.64240.52M25AnKimmeridgian
M25An.2n 0.0803base M25An.2n153.72270.33M25AnKimmeridgian
M25An0.4184M25An.2r 0.1034base M25An153.86040.27M25AKimmeridgian
M26n.1n 0.1441base M26n.1n154.16010.74M26nKimmeridgian
M26n.1r 0.0685base M26n.1r154.22860.61M26nKimmeridgian
M26n.2n 0.0301base M26n.2n154.25870.56M26nKimmeridgian
M26n.2r 0.0608base M26n.2r154.31950.45M26nKimmeridgian
M26n.3n 0.1145base M26n.3n154.43400.24M26nKimmeridgian
M26n.3r 0.1069base M26n.3r154.54090.04M26nKimmeridgian
M26n0.5479M26n.4n 0.0230base M26n154.56390.28M26Kimmeridgian
M28n.1n 0.3390base M28n.1n155.46700M28n.1nOxfordian
M28n.1r 0.1700base M28n.1r155.63700M28n.1rOxfordian
M28n.2n 0.1130base M28n.2n155.75000M28n.2nOxfordian
M28n.2r 0.2660base M28n.2r156.01600M28n.2rOxfordian
M28n.3n 0.2790base M28n.3n156.29500M28n.3nOxfordian
M28n1.3630M28n.3r 0.1040base M28n156.49100M28nOxfordian
M33n.1n 0.2320base M33n.1n158.98400M33n.1nOxfordian
M33n.1r 0.1570base M33n.1r159.14100M33n.1rOxfordian
M33n.2n 0.0930base M33n.2n159.23400M33n.2nOxfordian
M33n.2r 0.0820base M33n.2r159.31600M33n.2rOxfordian
M33n.3n 0.0810base M33n.3n159.39700M33n.3nOxfordian
M33n.3r 0.1340base M33n.3r159.53100M33n.3rOxfordian
M33n1.0330M33n.4n 0.2540base M33n159.78500M33nOxfordian
M34n.1n 0.0950base M34n.1n160.12300M34n.1nOxfordian
M34n0.6670M34n.1r 0.4630base M34n160.69500M34nOxfordian
M36n.1n 0.3090base M36n.1n161.40500M36n.1nOxfordian
M36n0.5650M36n.1r 0.1720base M36n161.66100M36nOxfordian
M37n.1n 0.2970base M37n.1n162.10900M37n.1nCallovian
M37n0.5740M37n.1r 0.1410base M37n162.38600M37nCallovian
M38n.1n 0.1310base M38n.1n162.67300M38n.1nCallovian
M38n.1r 0.0820base M38n.1r162.75500M38n.1rCallovian
M38n.2n 0.1230base M38n.2n162.87800M38n.2nCallovian
M38n.2r 0.1030base M38n.2r162.98100M38n.2rCallovian
M38n.3n 0.1000base M38n.3n163.08100M38n.3nCallovian
M38n.3r 0.1380base M38n.3r163.21900M38n.3rCallovian
M38n.4n 0.2810base M38n.4n163.50000M38n.4nCallovian
M38n1.2220M38n.4r 0.1570base M38n163.76400M38nCallovian
M39n.1n 0.1160base M39n.1n164.09600M39n.1nCallovian
M39n.1r 0.3670base M39n.1r164.46300M39n.1rCallovian
M39n.2n 0.5500base M39n.2n165.01300M39n.2nCallovian
M39n.2r 0.1900base M39n.2r165.20300M39n.2rCallovian
M39n.3n 0.0860base M39n.3n165.28900M39n.3nCallovian
M39n.3r 0.1990base M39n.3r165.48800M39n.3rBathonian
M39n.4n 0.1000base M39n.4n165.58800M39n.4nBathonian
M39n.4r 0.1310base M39n.4r165.71900M39n.4rBathonian
M39n.5n 0.0780base M39n.5n165.79700M39n.5nBathonian
M39n2.0340M39n.5r 0.1120base M39n166.01400M39nCallovian
M40n.1n 0.0610base M40n.1n166.18000M40n.1nBathonian
M40n.1r 0.1560base M40n.1r166.33600M40n.1rBathonian
M40n.2n 0.1440base M40n.2n166.48000M40n.2nBathonian
M40n0.5280M40n.2r 0.1110base M40n166.64700M40nBathonian
M41n.1n 0.0740base M41n.1n167.17800M41n.1nBathonian
M41n.1r 0.0600base M41n.1r167.23800M41n.1rBathonian
M41n.2n 0.0460base M41n.2n167.28400M41n.2nBathonian
M41n0.4200M41n.2r 0.0470base M41n167.52400M41nBathonian
M42n.1n 0.1700base M42n.1n168.16900M42n.1nBathonian
M42n.1r 0.3800base M42n.1r168.54900M42n.1rBajocian
M42n.2n 0.1180base M42n.2n168.66700M42n.2nBajocian
M42n.2r 0.0990base M42n.2r168.76600M42n.2rBajocian
M42n.3n 0.1620base M42n.3n168.92800M42n.3nBajocian
M42n1.2750M42n.3r 0.0370base M42n169.27400M42nBajocian
mid-Aal R1.1270base mid-Aal R172.66000.05Ludwigia murchisonae TAZpart of a confused interval, needs checkingAalenian
E22n.2n 0.2300base E22n.2n203.030000.0000Rhaetian
E22n.1r 0.0100base E22n.1r203.040000.0000Rhaetian
E22n0.6100E22n.1n 0.3700base E22n.1n203.410000.0000Rhaetian
E21r.3r 0.3200base E21r.3r203.730000.0000Rhaetian
E21r.2n 0.0200base E21r.2n203.750000.0000Rhaetian
E21r.2r 0.1300base E21r.2r203.880000.0000Rhaetian
E21r.1n 0.0500base E21r.1n203.930000.0000Rhaetian
E21r0.7100E21r.1r 0.1900base E21r.1r204.120000.0000Rhaetian
E20r.1n 0.0400base E20r.1n206.070000.0000Norian
E20r0.2100E20r.1r 0.1700base E20r.1r206.240000.0000Norian
E15r.1n 0.0400base E15r.1n212.400000.0000Norian
E15r0.2400E15r.1r 0.2000base E15r.1r212.600000.0000Norian
E13n.2n 0.9200base E13n.2n217.890000.0000Norian
E13n.1r 0.0400base E13n.1r217.930000.0000Norian
E13n1.4900E13n.1n 0.5300base E13n.1n218.460000.0000Norian
MK5n.1r 0.5040E5rbase MK5n.1r230.00900.57Tuvalian0.0000Base of Germanic Carnian "MK5n.1r" is ca. 57% up in Tuvalian (Wendy Zhang summary figure, 2020). Fits Spino-N1/UT11n.1r -- Base = 0.18 of Tuvalian 3 (A. spinosus Zone) in Hounslow-Muttoni 2010 synthesis based on relative durations at Pizzo Mondello. Shortened from Concise GTS of 0.99 of T. subbullatus Zone Carnian
MK5n.1n.2n 1.7640E2n-5n?base MK5n..1n.2n231.77300.29Tuvalian0.0000Base of Germanic Carnian "MK5n.1n.2n" is 29% up in Tuvalian (Wendy Zhang summary figure, 2020). MUCH LONGER than former Spino-N1/UT11n.1n -- Base = 0.10 of A. spinosus Zone to bring equal to base of Newark E4n in this "long Rhaetian" correlation version. Shortened from Concise GTS where Base of Gallet composite is probably Channell SB.2n.1n short normal = 0.85 of T. subbullatus Zone. They assign as E5n, but this really compacts their section. NOTE: Hounslow-Muttoni put this entirely into A. spinosus Zone (plus uppermost UT10r) => adjusted to be 0.1 up in A. sphasus zone (and all ones above are shifted/compacted accordingly). Carnian
MK5n.1n.1r 0.0630E2r?base MK5n.1n.1r231.83600.28Tuvalian0.0000Base of Germanic Carnian "MK5n.1n.1r" (very brief) is 28% up in Tuvalian (Wendy Zhang summary figure, 2020). MUCH SHORTER than former Subb-R/UT10r -- Chanell SB.2r base = about 70% up in former P. carpathica zone (merged with next higher zone here due to changes in definition). They assign as E4r, but this really compacts their section. Carnian
MK5n3.1500MK5n.1n.1n 0.8190pre-Ebase MK5n.1n.1n232.65500.15Tuvalian0.0000Base of Germanic Carnian "MK5n.1n.1n" is 15% up in Tuvalian (Wendy Zhang summary figure, 2020). = similar to base of Subb-N/UT10n -- Channel SB.2n base = about 20% up in former P. carpathica zone (merged with next higher zone here due to changes in definition) (hence about base of T. subbullatus ammonite zone). They assign as E4n, but this really compacts their section. Carnian
WY1n.2n 0.1755Duration of interpreted WY1n = UT2n is 3 100-kyr cycles in lower Zhuganpobase WY1n.2n235.74550.35WY1n0.0000Trachy-N/UT2n (upper) Base = 35% up in UT2n [=WY1n] Carnian
WY1n.r1 0.0270base WY1n.r1235.77250.25WY1n0.0000Trachy-N/UT2n (very brief R) Base = 25% up in UT2n (Hounslow-Muttoni) [=WY1n] Carnian
WY1n0.2700Duration of interpreted WY1n = UT2n is 3 100-kyr cycles in lower ZhuganpoWYn.1n 0.06750.269283333base WYn.1n235.84000.8Trachyceras aon TAZ0.0000Trachy-N/UT2n -- Base = 0.8 of Trachy. aon s.z. (was 0.7; but moved up to fit Zhuganpo cycle-mag) Carnian
WY1n.2n 0.1755Duration of interpreted WY1n = UT2n is 3 100-kyr cycles in lower Zhuganpobase WY1n.2n235.74550.35WY1n0.0000Trachy-N/UT2n (upper) Base = 35% up in UT2n [=WY1n] Carnian
WY1n.r1 0.0270base WY1n.r1235.77250.25WY1n0.0000Trachy-N/UT2n (very brief R) Base = 25% up in UT2n (Hounslow-Muttoni) [=WY1n] Carnian
WYn0.2700WYn.1n 0.06750.269283333base WYn.1n235.84000.8Trachyceras aon TAZ0.0000Trachy-N/UT2n -- Base = 0.8 of Trachy. aon s.z. (was 0.7; but moved up to fit Zhuganpo cycle-mag) Carnian
SC4r.3r 0.0440base SC4r.3r239.09400.92SC4r0.0000ca. 92% up in SC4r Ladinian
SC4r.2n 0.0385base SC4r.2n239.13250.85SC4r0.0000ca. 85% up in SC4r Ladinian
SC4r.2r 0.0990base SC4r.2r239.23150.67SC4r0.0000ca. 67% up in SC4r Ladinian
SC4r.1n 0.0385base SC4r.1n239.27000.6SC4r0.0000ca. 60% up in SC4r Ladinian
SC4r0.5500SC4r1rr 0.3300base SC4r1rr239.600000.0000Numerical age from Maron et al. (2018) Ladinian
SC3n.3n 0.0910base SC3n.3n240.59100.87SC3n0.0000Ca.87% up in SC3n. Gred-N2.n1/MT10n -- was Base = 0.68 of Euprotrachy. gredleri s.z. Ladinian
SC3n.2r 0.0490base SC3n.2r240.64000.8SC3n0.0000Ca.80% up in SC3n. Gred-R1/MT9r -- was Base = 0.50 of Euprotrachy. gredleri s.z. Ladinian
SC3n.2n 0.1800base SC3n.2n240.82000-0.0300base SC3n.1rBase is 0.03 above SC3n.1r Ladinian
SC3n.1r 0.0300base SC3n.1r240.85000.5SC3n0.0000Brief (0.03) R begins 50% up in SC3n of Maron et al. (2019). Gred-R1/MT9n.1r -- was Base = 0.10 of Euprotrachy. gredleri s.z. Assumed to be the brief R in Hounslow-Muttoni (2010) -- would need to tract down sets that I used. Ladinian
SC3n0.7000SC3n.1n 0.3500base SC3n.1n241.200000.0000Numerical age from Maron et al. (2019). Margar-N/MT9n.1n -- This long-Normal-polarity zone extends from upper (0.7) Eoprotrachy. curionii Zone through entire Protrachy. margaritosum to lowermost Euprotrachy. gredleri (see continuation in "secondary" column). Top in "Primary" column shown as top of Protrachy. margaritosum s.z. for "splice" purposes. Ladinian
MT3r.3r 0.1721base MT3r.3r244.98340.5MT3r0.0000Aeg-2r/CG11r -- Base = base of Bithynian in Hounslow-Muttoni (2010) composite diagram. Drawn as 50% up in complex MT3r in Hounslow-Muttoni (2010) composite diagram (used here)Anisian
MT3r.2n 0.0516base MT3r.2n245.03500.35MT3r0.0000Drawn as 35% up in complex MT3r in Hounslow-Muttoni (2010) composite diagram (used here)Anisian
MT3r.2r 0.0517base MT3r.2r245.08670.2MT3r0.0000Drawn as 20% up in complex MT3r in Hounslow-Muttoni (2010) composite diagram (used here)Anisian
MT3r0.3442MT3r.1n 0.0344base MT3r.1r245.15550.9E16 ChL0.0000Aeg-2r/CG11r -- Base MT3r is about 90% up in E16 at Guandao (Mingsong Li, revised preliminary; used here). Was drawn in Houslow-Muttoni as about 90% up in Aegean; and was tentatively CG11r of Szurlies (in uppermost Rot Fm, or about middle of his Germanic cycle s7.7 (or 7.11 using Menning’s 2013 scale which indicated a gap of 3 cycles below the one-cycle "R" at 7.11) -- which would be about 0.5 myr lower; however that study didn’t extend high enough, and cyclicity may not always be 100kyr?) GTS04 -- Base = 0.75 of Paracrochordiceras Zone, which projected to nearly same level after adjusting base-Anisian age!Anisian
MT3n.2n 0.4017base MT3n.2n245.55720.72MT3n0.0000Aeg-1n/CG11n/MT3n -- ca. 72% up in main MT3n in Hounslow-Muttoni (2010) diagramAnisian
MT3n1.4345MT3n.1r 0.1004base MT3n.1n246.59000s7.3 DeL0.0000Aeg-1n/CG11n/MT3n -- Set to base of CG11n of Szurlies’07 (lowermost Rot, put 2 cycles up as base of Germanic cycle s7.3 to be consistent with Guandao cycle-mag and Wantou mag-UPb age model (YanChen’19 EPSL) relative to base-Ch. timorensis. However, it is drawn in Houslow-Muttoni as about 25% up in Aegean. A better scaling might require shifting "MT1n-MT1n" to be in Spathian (which may just be a problem relating base-Rot to GSSP in Romania)Anisian
CG9n.3n 0.4800base CG9n.3n247.60000.9s5.10 DeL0.0000CG9n.3n base at ca. 90% up in s5.10 (Szurlies’07; fig. 7)Olenekian
CG9n.2r 0.0400base CG9n.2r247.64000.5s5.10 DeL0.0000Brief CG9n.2r subchron base at at middle of s5.10 (Szurlies’07, Fig. 7)Olenekian
CG9n.2n 0.3250base CG9n.2n247.96500.25s5.7 DeL0.0000CG9n.2n base ca. 25% up in s5.7 (Szurlies’07; Fig.7)Olenekian
CG9n.1r 0.0600base CG9n.1r248.02500.65s5.6 DeL0.0000CG9n.1r subchron base ca. 65% up in s5.6 (Szurlies’07; Fig.7)Olenekian
CG9n1.0050CG9n.1n 0.1000base CG9n.1n248.12500.65s5.5 DeL0.0000CB9n base ca. 65% up in s5.5 (Szurlies’07; Fig.7) (was base of s5.8 in Szurliles’04)Olenekian
NB sub-intervals will not be downloaded, either select them as the main interval, or cut and paste from the table above.

Events in the magnetochronology dataset

idEventtypecategorystageageplacementTSC notescompilation_notesabv termstage
5913base C2r.2n’intv baseHolocene-Holocene
5914base C2r.3rintv baseHolocene-Holocene
5904base C1nintv baseChibanian0.7730preset age: Chron C1n (= Brunhes Normal) base is in the upper (younger) part of Oxygen isotopic stage 19; with astrochronology age of 773 +/- 1 ka (Channell et al., 2010; reviewed by Singer, 2014). Base of Middle Pleistocene (= base of Ionian Stage) = base of Brunhes Chron.Chibanian
5905base C1r.1rintv baseCalabrian0.9900preset age: 990 +/-4 ka; and base of MIS 27 (Channell et al., 2020)Calabrian
5906base C1r.1nintv baseCalabrian1.0700preset age: Chron C1r.1n (= Jarmallo Normal) top coincides with Oxygen isotope stage 27, and base is in stage 31. 1070 +/-3 ka (MIS 31; and dated lavas in Tahiti; Channell et al., 2020)Calabrian
5907base C1r.2rintv baseCalabrian1.1800preset age: End of the Cobb Mountain excursion in ODP/IODP records is approximately 1178 ka (reviewed in Channell et al., 2020)Calabrian
5908base C1r.2nintv baseCalabrian1.2150preset age: Excursion named after Alder Creek rhyolite at Cobb Mountain (California) is near MIS36/37 boundary with onset in ODP/IODP cores at 1215 ka. Set sa polarity chron C1r.2r (="C1r.2r-1n" of Cande-Kent nomenclature). Marine cyclostratigraphy indicates a 30 kyr duration. Ar-Ar dating of base and top are summarized in Singer (2014) and Channell et al. (2020)Calabrian
5909base C1intv baseCalabrian1.7700preset age: In MIS 63. Astrochronology at ODP Site 677 (1.77 Ma) is consistent with that of Italan land sections (1.79 Ma) (Channell et al., 2020)Calabrian
5910base C2nintv baseGelasian1.9250preset age: Chron C2n (= Olduvai Normal). "Near LAD of Discoaster brouweri and MIS 71/72 transition.""Site U1308 result implies an age for the base Olduvai, on the LR04 timescale, of 1925 ka"" (review by Channell et al., 2020, of difficulties dating the onset)". Ar-Ar dating agrees with astronomical-cycles (e.g., Channell, 2002).Gelasian
8183base C2r.1rintv baseGelasian2.1160preset age: Gelasian
5912base C2r.1nintv baseGelasian2.1400preset age: C2r.1n was formerly named Reunion; but the type location was discovered to be a brief excursion before the main Normal; therefore Singer (2014) recommended Feni be used after the documented extent and age-control at Feni Drift ODP Site 981 in North Atlantic (Channell et al., 2003). Reunion "upper" excursion suggested from Reunion island volcanics in Indian Ocean, is now best documented at Feni Drift ODP Site 981as spanning ca. 2.140 to 2.116 Ma (25 kyr)Gelasian
5911base C2intv basePiacenzian2.5950preset age: Piacenzian
5915base C2r.2rintv basePiacenzian2.5950preset age: Base of Pleistocene is just above the base of Matuyama Chron (reversed-polarity chron C2r) (= top of Gauss; normal-polarity C2An.1n). MIS 104 at 2595 ka; and an Ar/Ar date from Kenya of 2606 +/-6 ka. (Channell et al., 2020). Was 2.581 Ma in Cande-Kent’95 vs. 2.60 in Hilgen ’91 vs. recalculated Ar-Ar 2.61 Ma (Singer, 2014; used here).Piacenzian
5916base C2An.1nintv basePiacenzian3.0320preset age: Chron C2r/C2An boundary (= Matuyama Reversed/Gauss Normal boundary) coincides with Oxygen isotope stage 103-104 boundary. "Gauss Normal Chron" (C2An) contains two reversed intervals -- Kaena (2An.1r) and Mammoth (2An.2r). Polarity chron C2An.1n -- Top (= top of Gauss) is 2.581 Ma in Cande-Kent’95 (used here), vs. 2.60 in Hilgen ’91. This 2.581 Ma age (Gauss/Matuyama boundary) was by Langereis, van Hoof & Hilgen (1994, Nature 369: 615).Piacenzian
5917base C2An.1rintv basePiacenzian3.1160preset age: Chron C2An.1r (Kaena Reversed) top coincides with Oxygen isotope stage G21-G22 boundary; and base with K3-KM2 boundary.Piacenzian
5918base C2An.2nintv basePiacenzian3.2070preset age: Piacenzian
5919base C2An.2rintv basePiacenzian3.3300preset age: Chron C2An.2r (Mammoth Reversed) top coincides with Oxygen isotope stage KM6; and base with stage MG1.Piacenzian
5920base C2An.3nintv basePiacenzian3.5960preset age: Base of Piacenzian is base of Chron C2An.3nPiacenzian
5921base C2Aintv baseZanclean4.1870preset age: Gilbert Reversed Chron" spans Chrons C2Ar throug C3r. Chron C2An/C2Ar boundary (= Gauss Normal/Gilbert Reversed boundary) coincides with Oxygen isotope stage MG6-Gi1 boundary.Zanclean
5922base C3n.1nintv baseZanclean4.3000preset age: Chron C3n.1n (Cochiti Normal) top coincides with Oxygen isotope stage Co1-Co2 boundary; and base with stage CN1.Zanclean
5923base C3n.1rintv baseZanclean4.4930preset age: Zanclean
5924base C3n.2nintv baseZanclean4.6310preset age: Chron C3n.2n (Nunivak Normal) top coincides with Oxygen isotope stage N1-N2 boundary; and base with stage N7-N8 boundary.Zanclean
5925base C3n.2rintv baseZanclean4.7990preset age: Zanclean
5926base C3n.3nintv baseZanclean4.8960preset age: Chron C3n.3n (Sidufjall Normal) top coincides with Oxygen isotope stage Si1-Si2 boundary; and base with stage Si6.Zanclean
5927base C3n.3rintv baseZanclean4.9970preset age: Zanclean
5928base C3n.4nintv baseZanclean5.2350preset age: Chron C3n.4n (Thvera Normal) top coincides with Oxygen isotope stage T1; and base with stage TG2.Zanclean
5929base C3intv baseMessinian6.0230preset age: Messinian
5930base C3An.1nintv baseMessinian6.2720preset age: Messinian
5931base C3An.1rintv baseMessinian6.3860preset age: Messinian
5932base C3An.2nintv baseMessinian6.7270preset age: Messinian
5933base C3Aintv baseMessinian7.1040preset age: Messinian
5934base C3Bnintv baseMessinian7.2140preset age: Messinian
5935base C3Br.1rintv baseTortonian7.2620preset age: Tortonian
5936base C3Br.1nintv baseTortonian7.3050preset age: Tortonian
5937base C3Br.2rintv baseTortonian7.4560preset age: Tortonian
5938base C3Br.2nintv baseTortonian7.4990preset age: Tortonian
5939base C3Bintv baseTortonian7.5370preset age: Tortonian
5940base C4n.1nintv baseTortonian7.6500preset age: Tortonian
5941base C4n.1rintv baseTortonian7.7010preset age: Tortonian
5942base C4n.2nintv baseTortonian8.1250preset age: Tortonian
5943base C4r.1rintv baseTortonian8.2570preset age: Tortonian
5944base C4r.1nintv baseTortonian8.3000preset age: Tortonian
8513top C4r.2r-1intv topTortonian8.6610preset age: cryptochron within C4r.2rTortonian
8512base C4r.2r-1intv baseTortonian8.6990preset age: Tortonian
5946base C4intv baseTortonian8.7710preset age: Tortonian
5947base C4Anintv baseTortonian9.1050preset age: Tortonian
5948base C4Ar.1rintv baseTortonian9.3110preset age: Tortonian
5949base C4Ar.1nintv baseTortonian9.4260preset age: Tortonian
5950base C4Ar.2rintv baseTortonian9.6470preset age: Tortonian
5951base C4Ar.2nintv baseTortonian9.7210preset age: Tortonian
5952base C4Aintv baseTortonian9.7860preset age: Tortonian
5953base C5n.1nintv baseTortonian9.9370preset age: Tortonian
5954base C5n.1rintv baseTortonian9.9840preset age: Tortonian
5955base C5n.2nintv baseTortonian11.0560preset age: Tortonian
5956base C5r.1rintv baseTortonian11.1460preset age: Tortonian
5957base C5r.1nintv baseTortonian11.1880preset age: Tortonian
8514top C5r.2r-1intv topTortonian11.2670preset age: top of cryptochron within C5r.2rTortonian
5959base C5r.2r-1intv baseTortonian11.2980preset age: base of cryptochron within C5r.2rTortonian
5958base C5r.2rintv baseTortonian11.5920preset age: Tortonian
5960base C5r.2nintv baseSerravallian11.6570preset age: Base of Tortonian = base of Chron C5r.2nSerravallian
5961base C5intv baseSerravallian12.0490preset age: Serravallian
5962base C5An.1nintv baseSerravallian12.1740preset age: Serravallian
5963base C5An.1rintv baseSerravallian12.2720preset age: Serravallian
5964base C5An.2nintv baseSerravallian12.4740preset age: Serravallian
5965base C5Ar.1rintv baseSerravallian12.7350preset age: Serravallian
5966base C5Ar.1nintv baseSerravallian12.7700preset age: Serravallian
5967base C5Ar.2rintv baseSerravallian12.8290preset age: Serravallian
5968base C5Ar.2nintv baseSerravallian12.8870preset age: Serravallian
5969base C5Aintv baseSerravallian13.0320preset age: Serravallian
5970base C5AAnintv baseSerravallian13.1830preset age: Serravallian
5971base C5AAintv baseSerravallian13.3630preset age: Serravallian
5972base C5ABnintv baseSerravallian13.6080preset age: Serravallian
5973base C5ABintv baseSerravallian13.7390preset age: Serravallian
5974base C5ACintv baseLanghian14.0700preset age: Base of Serravalian = upper Chron C5ACnLanghian
5975base C5ACrintv baseLanghian14.1630preset age: Langhian
5976base C5ADnintv baseLanghian14.6090preset age: Langhian
5977base C5ADintv baseLanghian14.7750preset age: Langhian
5978base C5Bn.1nintv baseLanghian14.8700preset age: Langhian
5979base C5Bn.1rintv baseLanghian15.0400preset age: Langhian
5980base C5Bn.2nintv baseLanghian15.1860preset age: Langhian
5981base C5Bintv baseLanghian15.9940preset age: Base of Langhian = base of Chron C5Br. ABOVE = GTS04 (which was a partial spline also?). BELOW = GTS2012 Spline; keeping Base of Langhian as fixed age = base of C5Br. Langhian
5982base C5Cn.1nintv baseBurdigalian16.2610preset age: Burdigalian
5983base C5Cn.1rintv baseBurdigalian16.3510preset age: Burdigalian
5984base C5Cn.2nintv baseBurdigalian16.4340preset age: Burdigalian
5985base C5Cn.2rintv baseBurdigalian16.5320preset age: Burdigalian
5986base C5Cn.3nintv baseBurdigalian16.6370preset age: Burdigalian
5987base C5Cintv baseBurdigalian17.1540preset age: Burdigalian
5988base C5Dnintv baseBurdigalian17.4660preset age: Burdigalian
5989base C5Dr.1rintv baseBurdigalian17.6340preset age: Burdigalian
5990base C5Dr.1nintv baseBurdigalian17.6760preset age: Burdigalian
5991base C5Dintv baseBurdigalian18.0070preset age: Burdigalian
5992base C5Enintv baseBurdigalian18.4970preset age: Burdigalian
5993base C5Eintv baseBurdigalian18.6360preset age: Burdigalian
5994base C6nintv baseBurdigalian19.5350preset age: Burdigalian
5995base C6intv baseBurdigalian19.9790preset age: Burdigalian
5996base C6An.1nintv baseBurdigalian20.1820preset age: Burdigalian
5997base C6An.1rintv baseBurdigalian20.4480preset age: Burdigalian
5998base C6An.2nintv baseAquitanian20.7650preset age: Aquitanian
5999base C6Aintv baseAquitanian21.1300preset age: Aquitanian
6000base C6AAnintv baseAquitanian21.2040preset age: Aquitanian
6001base C6AAr.1rintv baseAquitanian21.4410preset age: Aquitanian
6002base C6AAr.1nintv baseAquitanian21.5190preset age: Aquitanian
6003base C6AAr.2rintv baseAquitanian21.6910preset age: Aquitanian
6004base C6AAr.2nintv baseAquitanian21.7220preset age: Aquitanian
6005base C6AAr.3rintv baseAquitanian21.8060preset age: Aquitanian
6008base C6AAintv baseAquitanian21.8060preset age: Aquitanian
6006base C6Bn.1nintv baseAquitanian21.9850preset age: Aquitanian
6007base C6Bn.1rintv baseAquitanian22.0420preset age: Aquitanian
8326base C6Bn.2nintv baseAquitanian22.3420preset age: Aquitanian
6009base C6Bintv baseAquitanian22.6210preset age: Aquitanian
6010base C6Cn.1nintv baseAquitanian22.7920preset age: Aquitanian
6011base C6Cn.1rintv baseAquitanian22.9730preset age: Aquitanian
6012base C6Cn.2nintv baseAquitanian23.0400preset age: Oligocene/Miocene boundary = base of C6Cn.2n = 23.8 Ma = age calibration point of Cande and Kent (1992)Aquitanian
6013base C6Cn.2rintv baseChattian23.2120preset age: Chattian
6014base C6Cn.3nintv baseChattian23.3180preset age: Chattian
6015base C6Cintv baseChattian24.0250preset age: Chattian
6016base C7n.1nintv baseChattian24.0610preset age: Chattian
6017base C7n.1rintv baseChattian24.1240preset age: Chattian
6018base C7n.2nintv baseChattian24.4590preset age: Chattian
6019base C7intv baseChattian24.6540preset age: Chattian
6020base C7Anintv baseChattian24.7660preset age: Chattian
6021base C7Aintv baseChattian25.0990preset age: Chattian
6022base C8n.1nintv baseChattian25.2640preset age: Chattian
6023base C8n.1rintv baseChattian25.3040preset age: Chattian
6024base C8n.2nintv baseChattian25.9870preset age: Chattian
6025base C8intv baseChattian26.4200preset age: Chattian
6026base C9nintv baseRupelian27.4390preset age: Rupelian
6027base C9intv baseRupelian27.8590preset age: Base of Chattian (working version) was base of Chron C9r - Oi-2a isotope excursion and global lowstandRupelian
6028base C10n.1nintv baseRupelian28.0870preset age: Rupelian
6029base C10n.1rintv baseRupelian28.1410preset age: Rupelian
6030base C10n.2nintv baseRupelian28.2780preset age: Rupelian
6031base C10intv baseRupelian29.1830preset age: Rupelian
6032base C11n.1nintv baseRupelian29.4770preset age: Rupelian
6033base C11n.1rintv baseRupelian29.5270preset age: Rupelian
6034base C11n.2nintv baseRupelian29.9700preset age: Rupelian
6035base C11intv baseRupelian30.5910preset age: Rupelian
6036base C12nintv baseRupelian30.9770preset age: Rupelian
6037base C12intv baseRupelian33.2140preset age: Rupelian
6038base C13nintv baseRupelian33.7260preset age: Rupelian
6039base C13intv basePriabonian35.1020preset age: Priabonian
6040base C15nintv basePriabonian35.3360preset age: Priabonian
6041base C15intv basePriabonian35.5800preset age: Priabonian
6042base C16n.1nintv basePriabonian35.7180preset age: Priabonian
6043base C16n.1rintv basePriabonian35.7740preset age: Priabonian
6044base C16n.2nintv basePriabonian36.3510preset age: Priabonian
6045base C16intv basePriabonian36.5730preset age: Priabonian
6046base C17n.1nintv basePriabonian37.3850preset age: Base of Priabonian (working version in GTS2012) was assigned here as base of Chron C17n.1nPriabonian
6047base C17n.1rintv basePriabonian37.5300preset age: Priabonian
6048base C17n.2nintv baseBartonian37.7810preset age: Bartonian
6049base C17n.2rintv baseBartonian37.8580preset age: Bartonian
6050base C17n.3nintv baseBartonian38.0810preset age: Bartonian
6051base C17intv baseBartonian38.3980preset age: Bartonian
6052base C18n.1nintv baseBartonian39.5820preset age: Bartonian
6053base C18n.1rintv baseBartonian39.6660preset age: Bartonian
6054base C18n.2nintv baseBartonian40.0730preset age: Bartonian
6055base C18intv baseBartonian41.0300preset age: Bartonian
6056base C19nintv baseLutetian41.1800preset age: Lutetian
6057base C19intv baseLutetian42.1960preset age: Lutetian
6058base C20nintv baseLutetian43.4500preset age: Lutetian
6059base C20intv baseLutetian46.2350preset age: Lutetian
6060base C21nintv baseLutetian47.7600preset age: Upper part of polarity chron C21n (C21n.67) = 46.8 Ma = calibration point of Cande and Kent (1992)Lutetian
6061base C21intv baseYpresian48.8780preset age: Base of Lutetian is at Chron C21r.4Ypresian
6062base C22nintv baseYpresian49.6660preset age: Ypresian
6063base C22intv baseYpresian50.7670preset age: Ypresian
6064base C23n.1nintv baseYpresian50.9960preset age: Ypresian
6065base C23n.1rintv baseYpresian51.0470preset age: Ypresian
6066base C23n.2nintv baseYpresian51.7240preset age: Ypresian
6067base C23intv baseYpresian52.5400preset age: Ypresian
6068base C24n.1nintv baseYpresian52.9300preset age: Ypresian
6069base C24n.1rintv baseYpresian53.0200preset age: Ypresian
6070base C24n.2nintv baseYpresian53.1200preset age: Ypresian
6071base C24n.2rintv baseYpresian53.2500preset age: Ypresian
6072base C24n.3nintv baseYpresian53.9000preset age: Ypresian
6073base C24intv baseThanetian57.1010preset age: Thanetian
6074base C25nintv baseThanetian57.6560preset age: Thanetian
6075base C25intv baseThanetian58.9590preset age: Thanetian
6076base C26nintv baseThanetian59.2370preset age: Thanetian
6077base C26intv baseDanian62.2780preset age: Danian
6078base C27nintv baseDanian62.5300preset age: Danian
6079base C27intv baseDanian63.5370preset age: Danian
6080base C28nintv baseDanian64.6450preset age: Danian
6081base C28intv baseDanian64.8620preset age: Danian
2993base C29nintv baseDanian65.7000preset age: Danian
2994base C29intv baseMaastrichtian66.38000.3400 Ma offset from base DanianBase of C29r is 0.406 Myr below K/P (Thibault et al., 2012); or 0.34 (Battenberg et al., 2012; used here and in GTS2020). Mesozoic/Cenozoic boundary event is approx. Chron C29r.4 (300 kyr up in total C29r span of ca. 710 kyr, according to cycles; Husson et al., 2011; Tibault et al., submitted); however, Batenberg et al., 2012 imply base is 66.31; for use in GTS2020 (Andy Gale's table) => 0.61 durationMaastrichtian
2995base C30nintv baseMaastrichtian68.1780-Maastrichtian
2996base C30intv baseMaastrichtian68.3510-Maastrichtian
2997base C31nintv baseMaastrichtian69.2710-Maastrichtian
2998base C31intv baseMaastrichtian71.4510-Maastrichtian
2999base C32n.1nintv baseMaastrichtian71.6910-Maastrichtian
3000base C32n.1rintv baseMaastrichtian71.8510-Maastrichtian
3001base C32n.2nintv baseCampanian73.6510-Campanian
3002base C32r.1rintv baseCampanian73.9510-Campanian
3003base C32r.1nintv baseCampanian74.0510-Campanian
3004base C32intv baseCampanian74.2010-Campanian
3005base C33nintv baseCampanian79.9000preset age: Base of C33n constrained by Ar/Ar ages to be slightly younger than 80.08 myr ? 0.61 (2-sigma); and following Hicks’95, it is extrapolated as 79.9 myr. FAD of G. calcarata is at C33n.85 (Cande-Kent tie point)Campanian
3006base C33rintv baseCampanian82.8750preset age: Base of C33r considered to be near base of Campanian = age calibration point on C-sequence. Dated in Songliao Basin mag-cycles by Ramezani et al (2017) as 83.07 ?0.15 (and revised ATS-Mag of 82.875 - Wu and Hinnov, PNAS, 2020) ""Base of Chron C33r is near the top of Santonian stage (placed near base of ""Late Santonian"" based on Chalk-version of Santonian in studies by Paul Montgomery, but seems that slightly ~0.2 myr ABOVE is more consistent with nannofossil ages relative to basal-boundary and pelagic outcrop studies -- used here)."" [NOTE: Implied duration, based on top set by cycle-strat, and base by Ar-Ar, is 3.4 myr, versus 4.6 myr in GTS04 => a much faster S.Atl. spreading (which is also seen for the above C32n cycle-mag)Campanian
3007base C33intv baseCampanian83.6500base CampanianCampanian
3516top M"-3"r setintv topAlbian102.9325-M"-3r" set reported in Late Albian, may occur at the end of the Prediscosphaera cretacea or within the Eiffellithus turriseiffeli nannoplankton zones (Tarduno et al., 1992) (put at FAD of E.turriseiffeli here; but not verified. Arbitrarily assigned 0.2 myr duration.base of CC9 = FAD E. turrisAlbian
3009base M"-3"r setintv baseAlbian103.1325base CC9M"-3r" set reported in Late Albian, may occur at the end of the Prediscosphaera cretacea or within the Eiffellithus turriseiffeli nannoplankton zones (Tarduno et al., 1992) (put at FAD of E.turriseiffeli here; but not verified. Arbitrarily assigned 0.2 myr duration.base of CC9 = FAD E. turrisAlbian
3515top M"-2"r setintv topAlbian107.3875-M"-2r" set of Middle Albian events reported near the boundary of the Biticinella breggiensis and Ticinella primula planktonic foraminifer zones (put at FAD of B.breggiensis here; but not verified. Arbitrarily assigned 0.2 myr duration.Albian
3011base M"-2"r setintv baseAlbian107.58750.0000 Ma offset from FAD Biticinella breggiensisM"-2r" set of Middle Albian events reported near the boundary of the Biticinella breggiensis and Ticinella primula planktonic foraminifer zones (put at FAD of B.breggiensis here; but not verified. Arbitrarily assigned 0.2 myr duration.Albian
3013top M"-1"rintv topAptian118.1390-M"-1r" (aka ISEA reversal) reported in late Aptian, has a biostratigraphic age near the base of the Globigerinelliodes algerianus planktonic foraminifer zone (put at base here). This subchron has also been called the "ISEA" event and has an estimated duration less than 100,000 years (Tarduno, 1990).Aptian
3947base M"-1"rintv baseAptian118.2390base Globigerinelloides algerianus pfZM"-1r" (aka ISEA reversal) reported in late Aptian, has a biostratigraphic age near the base of the Globigerinelliodes algerianus planktonic foraminifer zone (put at base here). This subchron has also been called the "ISEA" event and has an estimated duration less than 100,000 years (Tarduno, 1990).Aptian
3008base C34intv baseAptian120.9640preset age: from M-sequence timescale[subchron C34n is identical to chron C34 so it is a bit unpredictable which name will be used, hence both are included JRY]Aptian
4724base C34nintv baseAptian120.96400.0000 Ma offset from base C34[subchron C34n is identical to chron C34 so it is a bit unpredictable which name will beused, hence both are included JRY]Aptian
3015base M0rintv baseAptian121.4000preset age: age comes direct from the M-sequence time scale Aptian
3016base M1nintv baseBarremian123.7830preset age: age comes direct from the M-sequence time scale Barremian
3017base M1intv baseBarremian124.1690preset age: age comes direct from the M-sequence time scale Barremian
3018base M3nintv baseBarremian124.7170preset age: age comes direct from the M-sequence time scale Barremian
3019base M3intv baseHauterivian126.5140preset age: age comes direct from the M-sequence time scale Hauterivian
3020base M5nintv baseHauterivian127.5260preset age: age comes direct from the M-sequence time scale Hauterivian
3021base M5intv baseHauterivian127.9200preset age: age comes direct from the M-sequence time scale Hauterivian
3022base M6nintv baseHauterivian128.1450preset age: age comes direct from the M-sequence time scale Hauterivian
3023base M6intv baseHauterivian128.2940preset age: age comes direct from the M-sequence time scale Hauterivian
3024base M7nintv baseHauterivian128.5930preset age: age comes direct from the M-sequence time scale Hauterivian
3025base M7intv baseHauterivian128.9510preset age: age comes direct from the M-sequence time scale Hauterivian
3026base M8nintv baseHauterivian129.2820preset age: age comes direct from the M-sequence time scale Hauterivian
3027base M8intv baseHauterivian129.6010preset age: age comes direct from the M-sequence time scale Hauterivian
3028base M9nintv baseHauterivian129.9260preset age: age comes direct from the M-sequence time scale Hauterivian
3029base M9intv baseHauterivian130.2970preset age: age comes direct from the M-sequence time scale Hauterivian
3030base M10n normalintv baseHauterivian130.6830preset age: age comes direct from the M-sequence time scale Hauterivian
3031base M10intv baseHauterivian131.1250preset age: age comes direct from the M-sequence time scale Hauterivian
3032base M10Nn.1nintv baseHauterivian131.4620preset age: age comes direct from the M-sequence time scale Hauterivian
3033base M10Nn.1rintv baseHauterivian131.5090preset age: age comes direct from the M-sequence time scale Hauterivian
3034base M10Nn.2nintv baseHauterivian131.8290preset age: age comes direct from the M-sequence time scale Hauterivian
3035base M10Nn.2rintv baseHauterivian131.8520preset age: age comes direct from the M-sequence time scale Hauterivian
3036base M10Nn.3nintv baseHauterivian132.1390preset age: age comes direct from the M-sequence time scale Hauterivian
3068base M10Nintv baseHauterivian132.5520preset age: age comes direct from the M-sequence time scale Hauterivian
3037base M11nintv baseValanginian133.3230preset age: age comes direct from the M-sequence time scale Valanginian
3038base M11r.1rintv baseValanginian133.5650preset age: age comes direct from the M-sequence time scale Valanginian
3039base M11r.1nintv baseValanginian133.5880preset age: age comes direct from the M-sequence time scale Valanginian
3040base M11intv baseValanginian133.7850preset age: age comes direct from the M-sequence time scale Valanginian
3041base M11An.1nintv baseValanginian134.2940preset age: age comes direct from the M-sequence time scale Valanginian
3042base M11An.1rintv baseValanginian134.3480preset age: age comes direct from the M-sequence time scale Valanginian
3043base M11An.2nintv baseValanginian134.4260preset age: age comes direct from the M-sequence time scale Valanginian
3044base M11Aintv baseValanginian134.5150preset age: age comes direct from the M-sequence time scale Valanginian
3045base M12nintv baseValanginian134.7400preset age: age comes direct from the M-sequence time scale Valanginian
3046base M12r.1rintv baseValanginian135.5860preset age: age comes direct from the M-sequence time scale Valanginian
3047base M12r.1nintv baseValanginian135.6700preset age: age comes direct from the M-sequence time scale Valanginian
3048base M12intv baseValanginian135.8310preset age: age comes direct from the M-sequence time scale Valanginian
3049base M12Anintv baseValanginian136.1060preset age: age comes direct from the M-sequence time scale Valanginian
3050base M12Aintv baseValanginian136.2000preset age: age comes direct from the M-sequence time scale Valanginian
3051base M13nintv baseValanginian136.3930preset age: age comes direct from the M-sequence time scale Valanginian
3052base M13intv baseValanginian136.6590preset age: age comes direct from the M-sequence time scale Valanginian
3053base M14nintv baseValanginian136.9380preset age: age comes direct from the M-sequence time scale Valanginian
3054base M14intv baseValanginian137.6600preset age: age comes direct from the M-sequence time scale Valanginian
3055base M15nintv baseBerriasian138.0220preset age: age comes direct from the M-sequence time scale Berriasian
3056base M15intv baseBerriasian138.4840preset age: age comes direct from the M-sequence time scale Berriasian
3057base M16nintv baseBerriasian139.6520preset age: age comes direct from the M-sequence time scale Berriasian
3058base M16intv baseBerriasian140.1880preset age: age comes direct from the M-sequence time scale Berriasian
3059base M17nintv baseBerriasian140.4940preset age: age comes direct from the M-sequence time scale Berriasian
3060base M17intv baseBerriasian141.7540preset age: age comes direct from the M-sequence time scale Berriasian
3061base M18nintv baseBerriasian142.3070preset age: age comes direct from the M-sequence time scale Berriasian
3062base M18intv baseBerriasian142.6280preset age: age comes direct from the M-sequence time scale Berriasian
3063base M19n.1nintv baseBerriasian142.7420preset age: age comes direct from the M-sequence time scale Berriasian
3064base M19n.1rintv baseBerriasian142.7800preset age: age comes direct from the M-sequence time scale Berriasian
3065base M19n.2nintv baseTithonian143.7430preset age: age comes direct from the M-sequence time scale Tithonian
1base M19rintv baseTithonian143.9680preset age: NOTE: For GTS2020, Gale-Gradstein gave "FINAL AGES" for Early Cret; rather than use M-Seq fit to radiometric dates. Therefore, M-Seq was spline-fit to those ages (forced in E.Cret.; more flexible in Jurassic) to generate smoothed spreading rates -- see Sheet "MSeqSpline24Sept" in this workbookTithonian
3066base M19intv baseTithonian143.9700preset age: age comes direct from the M-sequence time scale Tithonian
2base M20n.1nintv baseTithonian144.2948@ 0.70 up in M20nTithonian
3base M20n.1rintv baseTithonian144.3509@ 0.65 up in M20nTithonian
4base M20nintv baseTithonian145.0465@ 0.38 up in M20Tithonian
5base M20rintv baseTithonian145.7160preset age: NOTE: For GTS2020, Gale-Gradstein gave "FINAL AGES" for Early Cret; rather than use M-Seq fit to radiometric dates. Therefore, M-Seq was spline-fit to those ages (forced in E.Cret.; more flexible in Jurassic) to generate smoothed spreading rates -- see Sheet "MSeqSpline24Sept" in this workbookTithonian
6base M21nintv baseTithonian146.5797@ 0.33 up in M21Tithonian
7base M21rintv baseTithonian147.0090preset age: NOTE: For GTS2020, Gale-Gradstein gave "FINAL AGES" for Early Cret; rather than use M-Seq fit to radiometric dates. Therefore, M-Seq was spline-fit to those ages (forced in E.Cret.; more flexible in Jurassic) to generate smoothed spreading rates -- see Sheet "MSeqSpline24Sept" in this workbookTithonian
8base M22n.1nintv baseTithonian148.3006@ 0.13 up in M22nTithonian
9base M22n.1rintv baseTithonian148.3437@ 0.10 up in M22nTithonian
8869base M22n.2nintv baseTithonian148.3897@ 0.07 up in M22nTithonian
2132base M22n.2rintv baseTithonian148.4311@ 0.04 up in M22nTithonian
11base M22nintv baseTithonian148.4936@ 0.29 up in M22Tithonian
12base M22rintv baseTithonian149.1000preset age: NOTE: For GTS2020, Gale-Gradstein gave "FINAL AGES" for Early Cret; rather than use M-Seq fit to radiometric dates. Therefore, M-Seq was spline-fit to those ages (forced in E.Cret.; more flexible in Jurassic) to generate smoothed spreading rates -- see Sheet "MSeqSpline24Sept" in this workbookTithonian
13base M22Anintv baseTithonian149.2374@ 0.59 up in M22ATithonian
14base M22Arintv baseKimmeridgian149.4310preset age: NOTE: For GTS2020, Gale-Gradstein gave "FINAL AGES" for Early Cret; rather than use M-Seq fit to radiometric dates. Therefore, M-Seq was spline-fit to those ages (forced in E.Cret.; more flexible in Jurassic) to generate smoothed spreading rates -- see Sheet "MSeqSpline24Sept" in this workbookKimmeridgian
15base M23nintv baseKimmeridgian149.8277@ 0.72 up in M23Kimmeridgian
16base M23r.1rintv baseKimmeridgian150.1353@ 0.70 up in M23rKimmeridgian
17base M23r.1nintv baseKimmeridgian150.1640@ 0.67 up in M23rKimmeridgian
18base M23rintv baseKimmeridgian150.8530preset age: NOTE: For GTS2020, Gale-Gradstein gave "FINAL AGES" for Early Cret; rather than use M-Seq fit to radiometric dates. Therefore, M-Seq was spline-fit to those ages (forced in E.Cret.; more flexible in Jurassic) to generate smoothed spreading rates -- see Sheet "MSeqSpline24Sept" in this workbookKimmeridgian
19base M24nintv baseKimmeridgian151.1177@ 0.75 up in M24Kimmeridgian
20base M24r.1rintv baseKimmeridgian151.6327@ 0.33 up in M24rKimmeridgian
21base M24r.1nintv baseKimmeridgian151.6613@ 0.30 up in M24rKimmeridgian
22base M24rintv baseKimmeridgian151.8910preset age: NOTE: For GTS2020, Gale-Gradstein gave "FINAL AGES" for Early Cret; rather than use M-Seq fit to radiometric dates. Therefore, M-Seq was spline-fit to those ages (forced in E.Cret.; more flexible in Jurassic) to generate smoothed spreading rates -- see Sheet "MSeqSpline24Sept" in this workbookKimmeridgian
23base M24Anintv baseKimmeridgian152.0351@ 0.67 up in M24AKimmeridgian
24base M24Arintv baseKimmeridgian152.3330preset age: NOTE: For GTS2020, Gale-Gradstein gave "FINAL AGES" for Early Cret; rather than use M-Seq fit to radiometric dates. Therefore, M-Seq was spline-fit to those ages (forced in E.Cret.; more flexible in Jurassic) to generate smoothed spreading rates -- see Sheet "MSeqSpline24Sept" in this workbookKimmeridgian
25base M24Bnintv baseKimmeridgian152.7363@ 0.30 up in M24BKimmeridgian
26base M24Brintv baseKimmeridgian152.9100preset age: NOTE: For GTS2020, Gale-Gradstein gave "FINAL AGES" for Early Cret; rather than use M-Seq fit to radiometric dates. Therefore, M-Seq was spline-fit to those ages (forced in E.Cret.; more flexible in Jurassic) to generate smoothed spreading rates -- see Sheet "MSeqSpline24Sept" in this workbookKimmeridgian
27base M25nintv baseKimmeridgian153.2372@ 0.39 up in M25Kimmeridgian
28base M25rintv baseKimmeridgian153.4420preset age: base M25n-base M27n Marine Magnetic Anomaly Series from Handschmacker et al (1988)Kimmeridgian
29base M25An.1nintv baseKimmeridgian153.5738@ 0.69 up in M25AnKimmeridgian
30base M25An.1rintv baseKimmeridgian153.6424@ 0.52 up in M25AnKimmeridgian
31base M25An.2nintv baseKimmeridgian153.7227@ 0.33 up in M25AnKimmeridgian
32base M25An.2rintv baseKimmeridgian153.8261@ 0.08 up in M25AnKimmeridgian
33base M25Anintv baseKimmeridgian153.8604@ 0.27 up in M25AKimmeridgian
34base M25Arintv baseKimmeridgian154.0160preset age: base M25n-base M27n Marine Magnetic Anomaly Series from Handschmacker et al (1988)Kimmeridgian
35base M26n.1nintv baseKimmeridgian154.1601@ 0.74 up in M26nKimmeridgian
36base M26n.1rintv baseKimmeridgian154.2286@ 0.61 up in M26nKimmeridgian
37base M26n.2nintv baseKimmeridgian154.2587@ 0.56 up in M26nKimmeridgian
38base M26n.2rintv baseKimmeridgian154.3195@ 0.45 up in M26nKimmeridgian
39base M26n.3nintv baseKimmeridgian154.4340@ 0.24 up in M26nKimmeridgian
40base M26n.3rintv baseKimmeridgian154.5409@ 0.04 up in M26nKimmeridgian
41base M26nintv baseKimmeridgian154.5639@ 0.28 up in M26Kimmeridgian
42base M26rintv baseKimmeridgian154.7780preset age: Kimmeridgian
1347base M27rintv baseOxfordian155.1280preset age: Oxfordian
1348base M28n.1nintv baseOxfordian155.4670preset age: Oxfordian
1349base M28n.1rintv baseOxfordian155.6370preset age: Oxfordian
1350base M28n.2nintv baseOxfordian155.7500preset age: Oxfordian
1351base M28n.2rintv baseOxfordian156.0160preset age: Oxfordian
1352base M28n.3nintv baseOxfordian156.2950preset age: Oxfordian
1353base M28n.3rintv baseOxfordian156.3990preset age: Oxfordian
1354base M28nintv baseOxfordian156.4910preset age: Oxfordian
1355base M28rintv baseOxfordian156.6170preset age: Oxfordian
1356base M29nintv baseOxfordian156.9060preset age: Oxfordian
1357base M29rintv baseOxfordian157.1770preset age: Oxfordian
1358base M30nintv baseOxfordian157.4540preset age: Oxfordian
1359base M30rintv baseOxfordian157.6400preset age: Oxfordian
1360base M31nintv baseOxfordian157.9730preset age: Oxfordian
1361base M31rintv baseOxfordian158.0690preset age: Oxfordian
1362base M32nintv baseOxfordian158.4410preset age: Oxfordian
1363base M32rintv baseOxfordian158.7520preset age: Oxfordian
1364base M33n.1nintv baseOxfordian158.9840preset age: Oxfordian
1365base M33n.1rintv baseOxfordian159.1410preset age: Oxfordian
1366base M33n.2nintv baseOxfordian159.2340preset age: Oxfordian
1367base M33n.2rintv baseOxfordian159.3160preset age: Oxfordian
1368base M33n.3nintv baseOxfordian159.3970preset age: Oxfordian
1369base M33n.3rintv baseOxfordian159.5310preset age: Oxfordian
1370base M33nintv baseOxfordian159.7850preset age: Oxfordian
1371base M33rintv baseOxfordian160.0280preset age: Oxfordian
1372base M34n.1nintv baseOxfordian160.1230preset age: Oxfordian
1373base M34n.1rintv baseOxfordian160.5860preset age: Oxfordian
1374base M34nintv baseOxfordian160.6950preset age: Oxfordian
1375base M34rintv baseOxfordian160.8410preset age: Oxfordian
1376base M35nintv baseOxfordian160.9200preset age: Oxfordian
1377base M35rintv baseOxfordian161.0960preset age: Oxfordian
1378base M36n.1nintv baseOxfordian161.4050preset age: Oxfordian
1379base M36n.1rintv baseCallovian161.5770preset age: Callovian
1380base M36nintv baseCallovian161.6610preset age: Callovian
1381base M36rintv baseCallovian161.8120preset age: Callovian
1382base M37n.1nintv baseCallovian162.1090preset age: Callovian
1383base M37n.1rintv baseCallovian162.2500preset age: Callovian
1384base M37nintv baseCallovian162.3860preset age: Callovian
1385base M37rintv baseCallovian162.5420preset age: Callovian
1386base M38n.1nintv baseCallovian162.6730preset age: Callovian
1387base M38n.1rintv baseCallovian162.7550preset age: Callovian
1388base M38n.2nintv baseCallovian162.8780preset age: Callovian
1389base M38n.2rintv baseCallovian162.9810preset age: Callovian
1390base M38n.3nintv baseCallovian163.0810preset age: Callovian
1391base M38n.3rintv baseCallovian163.2190preset age: Callovian
1392base M38n.4nintv baseCallovian163.5000preset age: Callovian
1393base M38n.4rintv baseCallovian163.6570preset age: Callovian
1394base M38nintv baseCallovian163.7640preset age: Callovian
1395base M38rintv baseCallovian163.9800preset age: Callovian
1396base M39n.1nintv baseCallovian164.0960preset age: Callovian
1397base M39n.1rintv baseCallovian164.4630preset age: Callovian
1398base M39n.2nintv baseCallovian165.0130preset age: Callovian
1399base M39n.2rintv baseCallovian165.2030preset age: Callovian
1400base M39n.3nintv baseCallovian165.2890preset age: Callovian
1401base M39n.3rintv baseBathonian165.4880preset age: Bathonian
1402base M39n.4nintv baseBathonian165.5880preset age: Bathonian
1403base M39n.4rintv baseBathonian165.7190preset age: Bathonian
1404base M39n.5nintv baseBathonian165.7970preset age: Bathonian
1405base M39n.5rintv baseBathonian165.9090preset age: Bathonian
1406base M39nintv baseBathonian166.0140preset age: Bathonian
1407base M39rintv baseBathonian166.1190preset age: Bathonian
1408base M40n.1nintv baseBathonian166.1800preset age: Bathonian
1409base M40n.1rintv baseBathonian166.3360preset age: Bathonian
1410base M40n.2nintv baseBathonian166.4800preset age: Bathonian
1411base M40n.2rintv baseBathonian166.5910preset age: Bathonian
1412base M40nintv baseBathonian166.6470preset age: Bathonian
1413base M40rintv baseBathonian167.1040preset age: Bathonian
1414base M41n.1nintv baseBathonian167.1780preset age: Bathonian
1415base M41n.1rintv baseBathonian167.2380preset age: Bathonian
1416base M41n.2nintv baseBathonian167.2840preset age: Bathonian
1417base M41n.2rintv baseBathonian167.3310preset age: Bathonian
1418base M41nintv baseBathonian167.5240preset age: Bathonian
1419base M41rintv baseBathonian167.9990preset age: Bathonian
1420base M42n.1nintv baseBathonian168.1690preset age: Bathonian
1421base M42n.1rintv baseBajocian168.5490preset age: Bajocian
1422base M42n.2nintv baseBajocian168.6670preset age: Bajocian
1423base M42n.2rintv baseBajocian168.7660preset age: Bajocian
1424base M42n.3nintv baseBajocian168.9280preset age: Bajocian
1425base M42n.3rintv baseBajocian168.9650preset age: Bajocian
1426base M42nintv baseBajocian169.2740preset age: Bajocian
1427base M42rintv baseBajocian169.4560preset age: Bajocian
1428base M43n.1nintv baseBajocian169.5290preset age: Bajocian
1429base M43n.1rintv baseBajocian169.8310preset age: Bajocian
1430base M43n.2nintv baseBajocian169.9820preset age: Bajocian
1431base M43n.2rintv baseBajocian170.1450preset age: Bajocian
1432base M43nintv baseBajocian170.2910preset age: Bajocian
1433base M43rintv baseBajocian170.4710preset age: Bajocian
1434base M44n.1nintv baseBajocian170.7870preset age: Bajocian
1435base M44n.1rintv baseAalenian171.3430preset age: Aalenian
1436base M44n.2nintv baseAalenian171.5330preset age: Aalenian
1437base M44nintv baseAalenian171.5330preset age: Aalenian
1964top Opal-N2intv topAalenian172.6600@ 0.05 up in Ludwigia murchisonae TAZusing definition of base murch-RAalenian
1876base Opal-N2intv baseAalenian172.8000@ 0.95 up in Leioceras opalinum TAZbase = 0.95 of opalinumAalenian
1877base Opal-R2intv baseAalenian173.0000@ 0.85 up in Leioceras opalinum TAZbase = 0.85 of opalinumAalenian
1878base Opal-N1intv baseAalenian173.7000@ 0.50 up in Leioceras opalinum TAZbase = 0.5 of opalinumAalenian
1879base Opal-R1intv baseAalenian174.0000@ 0.35 up in Leioceras opalinum TAZbase = 0.35 of opalinumAalenian
1880base Aalen-Nintv baseAalenian174.7000base AalenianGTS2012 had included the main Play. aalensis in this "N" also; but now a brief "R" is at uppermost Toarcian, so put as base-Aalenian. Basal Aalenian polarity chron "Aalen-N" is assumed to extend to the mid-P. aalensis zone of latest Toarcian based on the S. Switzerland magnetics, which corresponds to an "no data" interval in the Thouars-Airvault section. However, the Switzerland polarity zonation did not resolve the "R" that comprises the Late Toarcian P. macta s.z.Aalenian
1881base Mochras T-R9intv baseToarcian174.8810@ 0.85 up in Pleydellia aalensis BAZMinor R. 85% up in Pley aalensis on Xu et al. (2018) synthesis figureToarcian
1882base Mochras T-N9intv baseToarcian175.6049@ 0.25 up in Pleydellia aalensis BAZMajor N. 25% up in Pley aalensis on Xu et al. (2018) synthesis figureToarcian
1883base Mochras T-R8intv baseToarcian175.8462@ 0.05 up in Pleydellia aalensis BAZ5% up in Pley aalensis on Xu et al. (2018) synthesis figureToarcian
1884base Mochras T-N8intv baseToarcian176.9087@ 0.55 up in Dumortieria levesquei BAsZMajor N. 55% up in Dumort. levesquei S.Z. on Xu et al. (2018) synthesis figureToarcian
1885base Mochras T-R7intv baseToarcian177.2197@ 0.10 up in Dumortieria levesquei BAsZ10% up in Dumort. levesquei S.Z. on Xu et al. (2018) synthesis figureToarcian
1886base Mochras T-N7intv baseToarcian177.4248@ 0.60 up in Phlyseogrammoceras dispansum BAsZ60% up in Phly. dispansum on Xu et al. (2018) synthesis figureToarcian
1887base Mochras T-R6intv baseToarcian177.9151@ 0.60 up in Grammoceras thouarsense BAZ60% up in Gram. thoarsense on Xu et al. (2018) synthesis figure. In their sub-Boreal subzones, this was also mid-way in a Ps. fallaciosum S.Z., which they show as spanning the upper 80% of that entire zone!Toarcian
1888base Mochras T-N6intv baseToarcian178.1297@ 0.30 up in Grammoceras thouarsense BAZ30% up in Gram. thoarsense on Xu et al. (2018) synthesis figure.Toarcian
1889base Mochras T-R5intv baseToarcian178.4923@ 0.90 up in Haugia variabilis BAZ90% up in Haugia variabilis on Xu et al. (2018) synthesis figure.Toarcian
1890base Mochras T-N5intv baseToarcian179.3804@ 0.30 up in Haugia variabilis BAZMajor N. 30% up in Haugia variabilis on Xu et al. (2018) synthesis figure.Toarcian
1891base Mochras T-R4intv baseToarcian179.8244base Haugia variabilis BAZBase of Haugia variabilis on Xu et al. (2018) synthesis figure.Toarcian
1892base Mochras T-N4intv baseToarcian180.0035@ 0.60 up in Catacoeloceras crassum BAsZ60% up in Sub-Boreal C. crassum s.z. of c on Xu et al. (2018) synthesis figure.Toarcian
1893base Mochras T-R3intv baseToarcian180.9439@ 0.50 up in Dactylioceras commune BAsZMajor R. 50% up in Sub-Boreal C. crassum s.z. of Hild. bifrons on Xu et al. (2018) synthesis figure.the notes in the table place this event at 0.5 C. crassum TAsZ, but the equation and TSC output place at .05 D. commune TAsZ - this also makes more sense for the decrion of the interval as a "major" reversal (placement in C.. crassum TAsZ would make it a very short reversal)Toarcian
1894base Mochras T-N3intv baseToarcian181.2125@ 0.95 up in Harpoceras falciferum BAsZ95% up in Sub-Boreal Harp. falciferum s.z. of Harp. serpentinum on Xu et al. (2018) synthesis figure.Toarcian
1895base Mochras T-R2intv baseToarcian181.6157@ 0.50 up in Harpoceras falciferum BAsZ50% up in Sub-Boreal Harp. falciferum s.z. of Harp. serpentinum on Xu et al. (2018) synthesis figure.Toarcian
1896base Mochras T-N2intv baseToarcian182.8303@ 0.30 up in Harpoceras exaratum BAsZMajor N. 30% up in Sub-Boreal Harp. exaratum s.z. of Harp. serpentinum on Xu et al. (2018) synthesis figure.Toarcian
1897base Mochras T-R1intv baseToarcian183.1041@ 0.05 up in Harpoceras exaratum BAsZ5% up in Sub-Boreal Harp. exaratum s.z. of Harp. serpentinum on Xu et al. (2018) synthesis figure.Toarcian
1898base Mochras T-N1intv baseToarcian183.9658@ 0.90 up in Protogrammoceras paltus BAsZMajor N. 90% up in Tethyan "mirabile" s.z. of Dacty. tenuicostatum at Toarcian auxiliary GSSP at Almonacid de la Cuba on Xu et al. (2018) synthesis figure' which, based on relative brief duration in that zone is assumed equivalent to P. paltus s.z.Toarcian
1899base Mochras T-R0intv baseToarcian184.1793@ 0.08 up in Protogrammoceras paltus BAsZ8% up in Tethyan "mirabile" s.z. of Dacty. tenuicostatum at Toarcian auxiliary GSSP at Almonacid de la Cuba on Xu et al. (2018) synthesis figure' which, based on relative brief duration in that zone is assumed equivalent to P. paltus s.z.Toarcian
1900base Spin-N4intv basePliensbachian184.3387@ 0.67 up in Pleuroceras hawskerense BAsZTop of Pliensbachian = short N (upper 1/3rd of Hawskerense zone at Toarcian auxiliary GSSP at Almonacid de la Cuba Pliensbachian
1901base Spin-R3.1rintv basePliensbachian184.8161@ 0.56 up in Pleuroceras spinatum BAZ56% up in Spinatum (partly adjusted from Spain)Pliensbachian
1902base Spin-R3.1nintv basePliensbachian184.8581@ 0.53 up in Pleuroceras spinatum BAZ53% up in Spinatum (very brief) (partly adjusted from Spain)Pliensbachian
1903base Spin-R3.2rintv basePliensbachian184.9701@ 0.45 up in Pleuroceras spinatum BAZ45% up in Spinatum (partly adjusted from Spain)Pliensbachian
1904base Spin-N2intv basePliensbachian185.1941@ 0.29 up in Pleuroceras spinatum BAZ29% up in SpinatumPliensbachian
1905base Spin-R2intv basePliensbachian185.3341@ 0.19 up in Pleuroceras spinatum BAZ19% up in SpinatumPliensbachian
1906base Spin-N1intv basePliensbachian185.4601@ 0.10 up in Pleuroceras spinatum BAZ10% up in SpinatumPliensbachian
1907base Spin-R1intv basePliensbachian185.6001base Pleuroceras spinatum BAZBase of Spinatum ZonePliensbachian
1908base Marg-N5intv basePliensbachian185.6961@ 0.96 up in Amaltheus margaritatus BAZ96% up in MargaritatusPliensbachian
1909base Marg-R5intv basePliensbachian185.7441@ 0.94 up in Amaltheus margaritatus BAZ94% up in MargaritatusPliensbachian
1910base Marg-N4.1nintv basePliensbachian185.8041@ 0.92 up in Amaltheus margaritatus BAZ91.5% up in MargaritatusPliensbachian
1911base Marg-N4.1rintv basePliensbachian185.8401@ 0.90 up in Amaltheus margaritatus BAZ90% up in MargaritatusPliensbachian
1912base Marg-N4.2nintv basePliensbachian185.9601@ 0.85 up in Amaltheus margaritatus BAZ85% up in MargaritatusPliensbachian
1913base Marg-N4.3rintv basePliensbachian185.9841@ 0.84 up in Amaltheus margaritatus BAZ84% up in MargaritatusPliensbachian
1914base Marg-N4.3nintv basePliensbachian186.0801@ 0.80 up in Amaltheus margaritatus BAZ80% up in MargaritatusPliensbachian
1915base Marg-R4.1rintv basePliensbachian186.1521@ 0.77 up in Amaltheus margaritatus BAZ77% up in MargaritatusPliensbachian
1916base Marg-R4.1nintv basePliensbachian186.1761@ 0.76 up in Amaltheus margaritatus BAZ76% up in MargaritatusPliensbachian
1917base Marg-R4.2rintv basePliensbachian186.4161@ 0.66 up in Amaltheus margaritatus BAZ66% up in MargaritatusPliensbachian
1918base Marg-N3intv basePliensbachian186.5121@ 0.62 up in Amaltheus margaritatus BAZ62% up in MargaritatusPliensbachian
1919base Marg-R3intv basePliensbachian187.3521@ 0.27 up in Amaltheus margaritatus BAZ27% up in MargaritatusPliensbachian
1920base Marg-N2intv basePliensbachian187.4481@ 0.23 up in Amaltheus margaritatus BAZ23% up in MargaritatusPliensbachian
1921base Marg-R2intv basePliensbachian187.6401@ 0.15 up in Amaltheus margaritatus BAZ15% up in MargaritatusPliensbachian
1922base Marg-N1.n1intv basePliensbachian187.7001@ 0.13 up in Amaltheus margaritatus BAZ12.5% up in MargaritatusPliensbachian
1923base Marg-N1.r1intv basePliensbachian187.7121@ 0.12 up in Amaltheus margaritatus BAZ12% up in MargaritatusPliensbachian
1924base Marg-N1.r2intv basePliensbachian187.8801@ 0.05 up in Amaltheus margaritatus BAZ5% up in MargaritatusPliensbachian
1925base Marg-R1intv basePliensbachian187.9281@ 0.03 up in Amaltheus margaritatus BAZ3% up in MargaritatusPliensbachian
1926base Dav-Nintv basePliensbachian188.4001base Prodactylioceras davoei BAZBase of DavoeiPliensbachian
1927base Ibex-R5intv basePliensbachian188.9401@ 0.70 up in Tragophylloceras ibex BAZ70% up in IbexPliensbachian
1928base Ibex-N5intv basePliensbachian189.0301@ 0.65 up in Tragophylloceras ibex BAZ65% up in IbexPliensbachian
1929base Ibex-R4intv basePliensbachian189.2101@ 0.55 up in Tragophylloceras ibex BAZ55% up in IbexPliensbachian
1930base Ibex-N4intv basePliensbachian189.3361@ 0.48 up in Tragophylloceras ibex BAZ48% up in IbexPliensbachian
1931base Ibex-R3intv basePliensbachian189.3901@ 0.45 up in Tragophylloceras ibex BAZ45% up in IbexPliensbachian
1932base Ibex-N3intv basePliensbachian189.4981@ 0.39 up in Tragophylloceras ibex BAZ39% up in IbexPliensbachian
1933base Ibex-R2intv basePliensbachian189.5881@ 0.34 up in Tragophylloceras ibex BAZ34% up in IbexPliensbachian
1934base Ibex-N2intv basePliensbachian189.6421@ 0.31 up in Tragophylloceras ibex BAZ31% up in IbexPliensbachian
1935base Ibex-R1intv basePliensbachian189.9301@ 0.15 up in Tragophylloceras ibex BAZ15% up in IbexPliensbachian
1936base Ibex-N1intv basePliensbachian190.0561@ 0.08 up in Tragophylloceras ibex BAZ8% up in IbexPliensbachian
1937base James-R3intv basePliensbachian190.4971@ 0.89 up in Uptonia jamesoni BAZ89% up in U. jamesoniPliensbachian
1938base James-N2intv basePliensbachian190.7401@ 0.80 up in Uptonia jamesoni BAZ80% up in U. jamesoniPliensbachian
1939base James-R2intv basePliensbachian191.4421@ 0.54 up in Uptonia jamesoni BAZ54% up in U. jamesoniPliensbachian
1940base James-N1intv basePliensbachian192.1441@ 0.28 up in Uptonia jamesoni BAZ26% up in U. jamesoniPliensbachian
1941base James-R1.r1intv basePliensbachian192.3061@ 0.22 up in Uptonia jamesoni BAZ22% up in U. jamesoniPliensbachian
1942base James-R1.n1intv basePliensbachian192.4141@ 0.18 up in Uptonia jamesoni BAZ18% up in U. jamesoniPliensbachian
1943base James-R1.r2intv basePliensbachian192.7111@ 0.07 up in Uptonia jamesoni BAZ7% up in U. jamesoni; in Paris basin core and near base of Italian section.Pliensbachian
1944base Rari-Nintv baseSinemurian193.6719@ 0.50 up in Echioceras raricostatum BAZN (top KH); 50% up in RaricostatumSinemurian
1945base Rari-Rintv baseSinemurian194.4436base Echioceras raricostatum BAZBase of RaricostatumSinemurian
1946base oxynotintv baseSinemurian195.2151base Oxynoticeras oxynotum BAZEntire Oxynotum zoneSinemurian
1947base Obtu-N2intv baseSinemurian196.0835@ 0.25 up in Asteroceras obtusum BAZ25% up in Obtusum in core-version; N (upper KH)Sinemurian
1948base Obtu-R1intv baseSinemurian196.1992@ 0.15 up in Asteroceras obtusum BAZ15% up in Obtusum in core-versionSinemurian
1949base Obtu-N1intv baseSinemurian196.3150@ 0.05 up in Asteroceras obtusum BAZ5% up in Obtusum in core-version; N (upper KH)Sinemurian
1950base Turner-Rintv baseSinemurian197.1450base Caenisites turneri BAZBase of Turneri in poor core biostrat (condensed interval for this zone)Sinemurian
1951base Semi-N?intv baseSinemurian197.2607@ 0.90 up in Arnioceras semicostatum BAZ90% up in Semicostatum; according to poor core biostratSinemurian
1952base Semi-Rintv baseSinemurian198.4180@ 0.90 up in Arietites bucklandi BAZ90% up in Bucklandi; R-dominated in core; spans middle Sinemurian, probably large R of Austria (Steiner-Ogg)Sinemurian
1953base Buck-N3intv baseSinemurian198.5917@ 0.75 up in Arietites bucklandi BAZN (mid-KH); 75% up in Bucklandi; N-dominated in coreSinemurian
1954base Buck-R3intv baseSinemurian198.6727@ 0.68 up in Arietites bucklandi BAZ68% up in Bucklandi; R-dominated in coreSinemurian
1955base Buck-N2intv baseSinemurian198.7074@ 0.65 up in Arietites bucklandi BAZN (lower mid-KH); 65% up in Bucklandi; N-dominated in coreSinemurian
1956base Buck-R2intv baseSinemurian198.9390@ 0.45 up in Arietites bucklandi BAZ45% up in Bucklandi; R-dominated in coreSinemurian
1957base Buck-N1intv baseSinemurian199.2600base Buck-N1calibration of event age from duration and age of underlying chronSinemurian
1958base Buck-R1intv baseSinemurian199.4100base Buck-R1calibration of event age from duration and age of underlying chronSinemurian
1959base Hett-N3intv baseHettangian199.6200base Hett-N3calibration of event age from duration and age of underlying chronHettangian
1960base Hett-R2intv baseHettangian199.6600base Hett-R2calibration of event age from duration and age of underlying chronHettangian
1961base Hett-N2intv baseHettangian199.9800base Hett-N2calibration of event age from duration and age of underlying chronHettangian
1962base Hett-R1intv baseHettangian200.0400base Hett-R1calibration of event age from duration and age of underlying chronHettangian
9018base intv baseHettangian-Hettangian
9019base Within Basalts; and pre-GSSPintv baseRhaetian-Rhaetian
1963base E24n / H24nintv baseRhaetian201.5900preset age: Base of E24n assigned by Kent-Olsen-Muttoni (2015)calibration of event age from duration and age of underlying chronRhaetian
9020base E24nintv baseRhaetian201.5900preset age: Kent-Olsen table has top of sediment record of E24n as 202 Ma (overlain by basalt of this age). However, it is drawn as ~0.8 myr on their figures (2 more 400 kyr cycles, above Basalt) => extension upward to 201.2 Ma, which I’ve used here.Rhaetian
9021base E23rintv baseRhaetian201.6000preset age: E23r is important potential correlation level; but . . . Rhaetian
9022base E23nintv baseRhaetian202.4900preset age: Rhaetian
9023base E22rintv baseRhaetian202.8000preset age: Rhaetian
9024base E22n.2nintv baseRhaetian203.0300preset age: Rhaetian
9025base E22n.1rintv baseRhaetian203.0400preset age: Rhaetian
9026base E22n.1nintv baseRhaetian203.4100preset age: Rhaetian
9027base E21r.3rintv baseRhaetian203.7300preset age: Rhaetian
9028base E21r.2nintv baseRhaetian203.7500preset age: Rhaetian
9029base E21r.2rintv baseRhaetian203.8800preset age: Rhaetian
9030base E21r.1nintv baseRhaetian203.9300preset age: Rhaetian
9031base E21r.1rintv baseRhaetian204.1200preset age: Rhaetian
9032base E21nintv baseRhaetian204.6500preset age: Rhaetian
9033base E20r.2rintv baseNorian206.0300preset age: Proposed marker for base-Rhaetian Pignola-Abriola (southern Italy) GSSP canddiate is the FAD of Misikella posthernsteini (sensu stricto) as recognized and calibrated by Maron et al. (2015) as being in the lower part of reversed-polarity zone they suggests is about 20% up in Chron E20r.2r of Newark polarity scale.Norian
9034base E20r.1nintv baseNorian206.0700preset age: Norian
9035base E20r.1rintv baseNorian206.2400preset age: Norian
9036base E20nintv baseNorian206.3600preset age: Norian
9037base E19rintv baseNorian207.0500preset age: Norian
9038base E19nintv baseNorian207.2000preset age: Norian
9039base E18rintv baseNorian207.5800preset age: Norian
9040base E18nintv baseNorian208.1000preset age: Norian
9041base E17rintv baseNorian209.4900preset age: Norian
9042base E17nintv baseNorian209.9500preset age: Norian
9043base E16rintv baseNorian210.2500preset age: Norian
9044base E16nintv baseNorian212.0500preset age: Norian
9045base E15r.2rintv baseNorian212.3600preset age: Norian
9046base E15r.1nintv baseNorian212.4000preset age: Norian
9047base E15r.1rintv baseNorian212.6000preset age: Norian
9048base E15nintv baseNorian213.4400preset age: Norian
9049base E14rintv baseNorian214.9200preset age: Norian
9050base E14nintv baseNorian216.1600preset age: Norian
9051base E13rintv baseNorian216.9700preset age: Norian
9052base E13n.2nintv baseNorian217.8900preset age: Norian
9053base E13n.1rintv baseNorian217.9300preset age: Norian
9054base E13n.1nintv baseNorian218.4600preset age: Norian
9055base E12rintv baseNorian219.2900preset age: Norian
9056base E12nintv baseNorian219.4600preset age: Norian
9057base E11rintv baseNorian221.4700preset age: Norian
9058base E11nintv baseNorian221.7500preset age: Norian
9059base E10rintv baseNorian222.2400preset age: Norian
9060base E10nintv baseNorian222.7400preset age: Norian
9061base E9rintv baseNorian224.0100preset age: Norian
8964base UT14nintv baseNorian224.5247@ 0.02 up in Malayites paulckei TAZPaul-N1/UT14n -- Base = 0.015 of Malayites paulckei Zone so that underlying UT13r matches duration of E8r of Newark if the base of Malayites palchkei is 95% up in E8r. Norian
9062base E9nintv baseNorian224.5400preset age: Norian
9063base E8rintv baseNorian226.1500preset age: Norian
8965base UT13r (E8r)intv baseNorian226.2818@ 0.38 up in Guembelites jandianus TAZJand-R1/UT13r -- Base = 0.38 of G. jandianus Zone to equal Newark ASSUMING TOP of G. janianus is 95% up in Chron E8r. BUT, uncertain; Hounslow-Muttoni'10 indicate it could be entirely within G. jandianus; or entirely in the overlying M. paulckei Zone => would affect scaling of all other polarity zones above/below. Norian
8966base UT13n.2nintv baseNorian226.4694@ 0.31 up in Guembelites jandianus TAZJand-N1.n2/UT13n.2n (of Hounslow-Muttoni) -- Base = 0.31 of G. jandianus Zone. Norian
8967base UT13n.1rintv baseNorian226.5765@ 0.27 up in Guembelites jandianus TAZJand-N1.r1/UT13n.1r (of Hounslow-Muttoni) - Base = 0.27 of G. jandianus Zone. Norian
8968base UT13n.1nintv baseNorian226.7500base E8nJand-N1.n1/UT13n.1n = E8n (set here). Norian
9064base E8nintv baseNorian226.7500preset age: Base Newark E8n had been used as Working assignment of age for Base-Norian using Pizzo Mondella "top of PM4r". Age of E8n from Kent-Olsen-Mutton 2017. But new M. parvus study (Mazza et al., 2019) puts this preferred base-Norian marker as high in E7n equivalent in Pizzo Mondello candidate GSSP.Norian
8969base PM4rintv baseNorian227.1000base E7rUT12r.2r/PM4r = E7r (FIXED here) -- Base = 0.95 of Tuvalian using Wendy Zhang's Carnian summary (2020), (or ca. 90% up in A. spinosus Zone) in Hounslow-Muttoni 2010 synthesis based on relative durations at Pizzo Mondello. Shortened from Concise GTS of 0.77 of A. spinosus Zone. The recommended Norian GSSP level at Pizzo Mondello coincides with the TOP of a narrow reversed-polarity zone (polarity zone “PM4r” in local terminology; or “UT12r” in the synthesis of Hounslow and Muttoni, 2010 -- which they show as quite narrow; but other reference sections indicate as relatively long). Norian
9065base E7rintv baseNorian227.1000preset age: Norian
8971base PM4nintv baseCarnian228.3500base E7nPizzo Mondella GSSP PM4n = Germanic Carnian "MK5n.2 - upper N" is 80% up in Tuvalian (Wendy Zhang summary figure, 2020) or equivalent to Newark E7n (FIXED here). Spino-N2/UT12n -- Base = 0.60 of Tuvalian 3 (A. spinosus Zone) in Hounslow-Muttoni 2010 synthesis based on relative durations at Pizzo Mondello. Shortened from Concise GTS of 0.25 of A. spinosus Zone. Carnian
9066base E7nintv baseCarnian228.3500preset age: Carnian
8972base PM3rintv baseCarnian228.6500base E6rBase of Germanic Carnian "MK5n.2.u (uncertain) but definitely have a PM3r = Newardk E6r" (FIXED HERE) is ca. 75% up in Tuvalian (Wendy Zhang summary figure, 2020). -- Verified as PM3r at Pizzo Mondello (which was UT11r of Hounslow-Muttoni; which had drawn Base = 0.51 of Tuvalian 3 (A. spinosus Zone) in their synthesis based on relative durations at Pizzo Mondello. Shortened from Concise GTS of 0.19 of A. spinosus. Was 0.16 of A. spinosus Zone in Concise GTS; but Hounslow-Muttoni'10 show as more narrow. Carnian
9067base E6rintv baseCarnian228.6500preset age: Carnian
8973base MK5n.2.1nintv baseCarnian229.5050@ 0.65 up in TuvalianBase of Germanic Carnian "MK5n.2 - upper N" is ca. 65% up in Tuvalian (Wendy Zhang summary figure, 2020). Spino-N1/UT11n.2n -- Base = 0.20 of Tuvalian 3 (A. spinosus Zone) in Hounslow-Muttoni 2010 synthesis based on relative durations at Pizzo Mondello. Shortened from Concise GTS of 0.02 of A. spinosus Zone. Poorly resolved minor subchron (single sample) Carnian
8974base MK5n.1rintv baseCarnian230.0090@ 0.57 up in TuvalianBase of Germanic Carnian "MK5n.1r" is ca. 57% up in Tuvalian (Wendy Zhang summary figure, 2020). Fits Spino-N1/UT11n.1r -- Base = 0.18 of Tuvalian 3 (A. spinosus Zone) in Hounslow-Muttoni 2010 synthesis based on relative durations at Pizzo Mondello. Shortened from Concise GTS of 0.99 of T. subbullatus Zone Carnian
8975base MK5n..1n.2nintv baseCarnian231.7730@ 0.29 up in TuvalianBase of Germanic Carnian "MK5n.1n.2n" is 29% up in Tuvalian (Wendy Zhang summary figure, 2020). MUCH LONGER than former Spino-N1/UT11n.1n -- Base = 0.10 of A. spinosus Zone to bring equal to base of Newark E4n in this "long Rhaetian" correlation version. Shortened from Concise GTS where Base of Gallet composite is probably Channell SB.2n.1n short normal = 0.85 of T. subbullatus Zone. They assign as E5n, but this really compacts their section. NOTE: Hounslow-Muttoni put this entirely into A. spinosus Zone (plus uppermost UT10r) => adjusted to be 0.1 up in A. sphasus zone (and all ones above are shifted/compacted accordingly). Carnian
8976base MK5n.1n.1rintv baseCarnian231.8360@ 0.28 up in TuvalianBase of Germanic Carnian "MK5n.1n.1r" (very brief) is 28% up in Tuvalian (Wendy Zhang summary figure, 2020). MUCH SHORTER than former Subb-R/UT10r -- Chanell SB.2r base = about 70% up in former P. carpathica zone (merged with next higher zone here due to changes in definition). They assign as E4r, but this really compacts their section. Carnian
8977base MK5n.1n.1nintv baseCarnian232.6550@ 0.15 up in TuvalianBase of Germanic Carnian "MK5n.1n.1n" is 15% up in Tuvalian (Wendy Zhang summary figure, 2020). = similar to base of Subb-N/UT10n -- Channel SB.2n base = about 20% up in former P. carpathica zone (merged with next higher zone here due to changes in definition) (hence about base of T. subbullatus ammonite zone). They assign as E4n, but this really compacts their section. Carnian
8978base MK4rintv baseCarnian233.6000-3.4000 Ma offset from base CarnianAge of 233.55 from independent Carnian ammonite-subzone scaling method fits the Cycle-Mag from S.China plus most of Carnian Pluvial event. Decided to FIX in GTS2020 as a rounded 3.4 myr above base of Carnian (as used in Wendy Zhang's Carnian Fig.9 age model); and DASH base-Julian at this level. Carnian
8979base MK4nintv baseCarnian233.8000@ 0.75 up in Austrotrachyceras austriacum TAZAustro-N2/UT5n- Top = Top of A. austriacum Zone. Base = 0.75 of A. austriacum Zone (was 0.87 of A. austriacum Zone in Concise; but see note that R below was too short). (not used in Hounslow-Muttoni'10; but they show a set of 5 schematic equal-N/R pairs (to fit their preferred Newark model). Carnian
8980base W1r.3rintv baseCarnian234.0800@ 0.40 up in Austrotrachyceras austriacum TAZAustro-R1/UT4r- Base = 0.4 of A. austriacum Zone (was 0.47 of A. austriacum Zone, making Reversed is relatively twice as long as in DTS version -- so partly adjusted in GTS2012) Carnian
8981base W1r.2nintv baseCarnian234.2800@ 0.15 up in Austrotrachyceras austriacum TAZAustro-N1/UT4n -- Base = 0.15 of A. austriacum Zone. (was 0.35 of A. austriacum Zone in Concise; but see note below on R that it was "twice as long" as original). Carnian
8982base W1r.2rintv baseCarnian235.20001.6000 Ma offset from base MK4rS.China cyclestrat implies base is ca. 1.6 myr below base of MK4r. In GTS2016, Trachy-R2/UT3r -(upper) - Base = 0.3 of Trachy. aoniodes s.z. This Reversed in Concise was relatively twice as long as in DTS version; therefore GTS2012 has lowered N boundary above. Carnian
8983base WY1r.1nintv baseCarnian235.4400@ 0.20 up in Trachyceras aonoides TAZTrachy-R2.n1/UT3n - Base = 0.2 of Trachy. aonoides Carnian
8984base WY1r.1rintv baseCarnian235.5700@ 0.10 up in Trachyceras aonoides TAZTrachy-R2.r1/UT2r - Base = lowered to 0.1 of Trachy. aoniodes s.z. (had been 0.3 in GTS2012; but lowered to attain the 1.3myr total duration of polarity zone from S.China) Carnian
8985base WY1n.2nintv baseCarnian235.7455@ 0.35 up in WY1nTrachy-N/UT2n (upper) Base = 35% up in UT2n [=WY1n] Carnian
8986base WY1n.r1intv baseCarnian235.7725@ 0.25 up in WY1nTrachy-N/UT2n (very brief R) Base = 25% up in UT2n (Hounslow-Muttoni) [=WY1n] Carnian
8987base WYn.1nintv baseCarnian235.8400@ 0.80 up in Trachyceras aon TAZTrachy-N/UT2n -- Base = 0.8 of Trachy. aon s.z. (was 0.7; but moved up to fit Zhuganpo cycle-mag) Carnian
8988base WY0rintv baseCarnian236.1900@ 0.30 up in Trachyceras aon TAZTrachy-R1/UT1r -- Base = 0.3 of Trachy. aon s.z. based on 0.35myr cycle-duration in Zhuganpo. the chron this ievent is base of has changed name from UT1r to WY0rCarnian
8989base MA5n.2nintv baseCarnian236.8473@ 0.30 up in MA5nDaxa-N/UT1n (upper) -- ca. 30% up in total UT1n in Hounslow-Muttoni'10 Carnian
8990base MA5n.1rintv baseCarnian236.8943@ 0.25 up in MA5nDaxa-N/UT1n (brief R of 0.05) -- ca. 60% up in total UT1n [now = MA5n] in Hounslow-Muttoni'10; but 25% up in Maron et al. (2019; used here). NOTE: Seceda "brief R" relative placement was the logic used by Hounslow-Muttoni, but apparently not by Muttoni in Maron et al, who preferred Mayerling as the reference section. Carnian
8991base MA5n.1nintv baseLadinian237.1290@ 0.90 up in Frankites regoledanus TAZDaxa-N/UT1n (lower) -- Apparently a long-Normal-polarity zone, spanning lower T. aon, entire Daxatina canadensis, and uppermost (to 0.9 in Hounslow-Muttoni; versus 0.62 in Concise GTS) F. regoledanus Zones. Ladinian
8992base MA4rintv baseLadinian237.2500preset age: Numerical age from Maron et al. (2019).Regole-R/MT13r -- was Base = 0.7 up in Frank. regoledanus zone; (was 0.19 of Frank. regoledanus s.z. in Concise GTS; but shown as thinner and higher by Hounslow-Muttoni'10) Ladinian
8993base MA4nintv baseLadinian237.8500preset age: Numerical age from Maron et al. (2019).Numerical age from Maron et al. (2018) Ladinian
8994base MA3rintv baseLadinian237.9500preset age: Numerical age from Maron et al. (2018) Ladinian
8995base MA3nintv baseLadinian238.6000preset age: Neum-N/MT13n -- was Long-N2/MT13 -- Base = 0.4 of Protrachy. neumayri s.z. Ladinian
8996base MA2rintv baseLadinian238.8000preset age: Neum-R.r1/M12r -- was Base = 0.96 of Protrachy. longobardicum s.z. Ladinian
8997base MA2nintv baseLadinian239.0500preset age: Arch-N2/M12n -- was Base = 0.87 of Protrachy. longobardicum s.z. Ladinian
8998base SC4r.3rintv baseLadinian239.0940@ 0.92 up in SC4rca. 92% up in SC4r Ladinian
8999base SC4r.2nintv baseLadinian239.1325@ 0.85 up in SC4rca. 85% up in SC4r Ladinian
9000base SC4r.2rintv baseLadinian239.2315@ 0.67 up in SC4rca. 67% up in SC4r Ladinian
9001base SC4r.1nintv baseLadinian239.2700@ 0.60 up in SC4rca. 60% up in SC4r Ladinian
9002base SC4r1rrintv baseLadinian239.6000preset age: Numerical age from Maron et al. (2019).Numerical age from Maron et al. (2018) Ladinian
9003base SC4nintv baseLadinian240.4000preset age: Numerical age from Maron et al. (2019).Numerical age from Maron et al. (2018) Ladinian
9004base SC3rintv baseLadinian240.5000preset age: Numerical age from Maron et al. (2019).Numerical age from Maron et al. (2018) Ladinian
9005base SC3n.3nintv baseLadinian240.5910@ 0.87 up in SC3nCa.87% up in SC3n. Gred-N2.n1/MT10n -- was Base = 0.68 of Euprotrachy. gredleri s.z. Ladinian
9006base SC3n.2rintv baseLadinian240.6400@ 0.80 up in SC3nCa.80% up in SC3n. Gred-R1/MT9r -- was Base = 0.50 of Euprotrachy. gredleri s.z. Ladinian
9007base SC3n.2nintv baseLadinian240.8200-0.0300 Ma offset from base SC3n.1rBase is 0.03 above SC3n.1r Ladinian
9008base SC3n.1rintv baseLadinian240.8500@ 0.50 up in SC3nBrief (0.03) R begins 50% up in SC3n of Maron et al. (2019). Gred-R1/MT9n.1r -- was Base = 0.10 of Euprotrachy. gredleri s.z. Assumed to be the brief R in Hounslow-Muttoni (2010) -- would need to tract down sets that I used. Ladinian
9009base SC3n.1nintv baseLadinian241.2000preset age: Numerical age from Maron et al. (2019).Numerical age from Maron et al. (2019). Margar-N/MT9n.1n -- This long-Normal-polarity zone extends from upper (0.7) Eoprotrachy. curionii Zone through entire Protrachy. margaritosum to lowermost Euprotrachy. gredleri (see continuation in "secondary" column). Top in "Primary" column shown as top of Protrachy. margaritosum s.z. for "splice" purposes. Ladinian
9011base MT8r.2nintv baseLadinian241.2396@ 0.90 up in SC2rBrief (0.03) N begins 90% up in SC2r of Maron et al. (2019). Fass-R/MT8r -- 67% up in Curionii zone (brief-N based on general pattern in Hounslow-Muttoni'10) Ladinian
9010base SC2r.3rintv baseLadinian241.26960.0300 Ma offset from base MT8r.2nBegins 0.03 above SC2r.1n. Fass-R/MT8r -- 68% up in Curionii zone (based on general pattern in Hounslow-Muttoni'10) Ladinian
9012base SC2r.2rintv baseLadinian241.4600base LadinianAGE = BASE-LADINIAN. Curionii-R/MT8r.1r -- was Long-Reversed-polarity zone begins at base of Curionii ammonite zone (base of Ladinian) in Hounslow-Muttoni 2010 summaryLadinian
9068base SC2r.1nintv baseLadinian241.51000.0500 Ma offset from base LadinianBrief N (0.05) with top at base of Ladinian = marker for boundary.. Illy-N3/MT8n -- Base of MT8n = ca. 0.9 of Nevadites secedensis Zone in Hounslow-Muttini 2010. Even though it is brief, Hounslow-Muttoni (2010) give it a separate designation (MT8n), because the Top (base of long Reversed) is a marker for Ladinian/Anisian boundary.Ladinian
9069base SC2r.1rintv baseAnisian241.5964@ 0.56 up in Nevadites secedensis TAZIlly-R2/MT7r -- Base = ca. 0.56 of Nevadites secedensis Zone.Anisian
9070base SC2nintv baseAnisian241.7218@ 0.75 up in MT7SC2n of Maron et al. (2019) scaling of Seceda begins ca. 75% up in larger MT7n [=MT7] of Hounslow-Muttoni (2010) equivalent. Illy-N2.2n/MT7n.3n -- Base = 53% up in MT7n interval on Hounslow-Muttoni (2010) diagram (used here); or 0.2 of Nevadites secedensis Zone.Anisian
9071base SC1rintv baseAnisian241.8722@ 0.45 up in MT7SCIr of Maron et al. (2019) scaling of Seceda begins ca. 45% up in larger MT7n of Hounslow-Muttoni (2010) equivalent. Illy-N2.2n/MT7n.2r -- Base = 45% up in MT7n interval on Hounslow-Muttoni (2010) diagram (used here); or 0.1 of Nevadites secedensis Zone.MT7 is not divided into MT7n and MT7rAnisian
9072base SC1nintv baseAnisian241.9474@ 0.30 up in MT7SCI/GD7n of Maron et al. (2019) scaling of Seceda-Guandao begins ca. 30% up in larger MT7n of Hounslow-Muttoni (2010) equivalent. Illy-N2.2n/MT7n.2n -- Base = 32% up in MT7n interval on Hounslow-Muttoni (2010) diagram (used here)MT7 is not divided into MT7n and MT7r, so claibration is changed here from 0.3 MT7n to 0.3 MT7 Anisian
9074base GD6nintv baseAnisian242.0978@ 0.45 up in E24 ChLIlly-N2.2r/MT7n.1n -- Base MT7n = 0.19 of Hungarites Zone; or (using published Lehrmann et al 2015 magstrat diagram) is 45% up in Guadao cycle E24 (Mingsong Li, 2015, in prep; used here)Anisian
9073base GD6rintv baseAnisian242.0627@ 0.07 up in MT7GD6r of Maron et al. (2019) scaling of Guandao begins ca. 7% up in larger MT7n [=MT7] of Hounslow-Muttoni (2010) equivalent. Illy-N2.1r/MT7n.1r -- Base = 26% up in MT7n interval on Hounslow-Muttoni (2010) diagram (used here).Anisian
9075base MT6rintv baseAnisian243.0191@ 0.30 up in MT5n-6rIlly-R1/MT6r -- Base = 30% up (see below) in Paraceratites zone; or 40% up in MT5n-6r interval on Hounslow-Muttoni (2010) diagram (used here).Anisian
9076base MT6nintv baseAnisian243.1508@ 0.20 up in MT5n-6rIll-N1/MT6n -- Base = 20% up in Paraceratites zone; or 20% up in MT5n-6r interval on Hounslow-Muttoni (2010) diagram (used here). However, this was 0.26 myr duration; but "GD5" of Maron et al. (2018) was only 0.10 => top lowered.Anisian
9077base MT5rintv baseAnisian243.3482@ 0.05 up in MT5n-6rnote that in TSC ther are two intervals MT5r - this is the upper one Anisian
9078base MT5nintv baseAnisian243.4140@ 0.20 up in E21 ChLPelson-R.n1/MT5n -- Base MT5n (based on conodont biostrat for base-Illyrian being above this normal-polarity interval that is truncated by covered-gap in higher part) is about 20% up in E21 at Guandao (Mingsong Li, 2015, used here). Base = 0.86 of Balatonites Zone in composite by Hounslow-Muttoni 2010. Apparently MT5n not used in Maron et al. (2019).Anisian
9628base MT4r-5rintv baseAnisian244.0418@ 0.65 up in E19 ChLPelson-R.r1 /MT4r -- Base MT4r is 65% up in cycle E19 at Guandao (Mingsong Li, 2015, in prep; used here); or Base = 0.29 of Balatonites ZoneAnisian
9079base MT4n.2nintv baseAnisian244.2880@ 0.68 up in MT4nBith-N.n2/MT4n.2n -- base is 68% up in MT4n on Hounslow-Muttoni (2010) composite diagram (based on Svalbard)Anisian
9080base MT4n.1rintv baseAnisian244.3881@ 0.55 up in MT4nBith-N.r1/MT4n.1r -- base is 55% up in MT4n on Hounslow-Muttoni (2010) composite diagram (based on Svalbard)Anisian
9081base MT4n1nintv baseAnisian244.8113@ 0.75 up in E17 ChLBith-N.n1/MT4n1n -- Bith-N.n1/MT4n1n (base GD4n of Maron et al., 2019) = Base MT4n is tentatively about 75% up in E17 at Guandao (Mingsong Li, in prep 2015; used here). Base CG12n = about 80% up in Cycle s7.8 (used here); or about 5% up in Kocaelia Zone (superzone for entire Bithynian) = just above base of Bithynian (following Hounslow-Muttoni revision; Concise GTS had as base of Bith.) BUT, perhaps CG12n of Szurlies => could be used to give Aegean duration.Anisian
9083base MT3r.2nintv baseAnisian245.0350@ 0.35 up in MT3rDrawn as 35% up in complex MT3r in Hounslow-Muttoni (2010) composite diagram (used here)Anisian
9082base MT3r.3rintv baseAnisian244.9834@ 0.50 up in MT3rAeg-2r/CG11r -- Base = base of Bithynian in Hounslow-Muttoni (2010) composite diagram. Drawn as 50% up in complex MT3r in Hounslow-Muttoni (2010) composite diagram (used here)Anisian
9084base MT3r.2rintv baseAnisian245.0867@ 0.20 up in MT3rDrawn as 20% up in complex MT3r in Hounslow-Muttoni (2010) composite diagram (used here)Anisian
9085base MT3r.1nintv baseAnisian245.1211@ 0.10 up in MT3rDrawn as 10% up in complex MT3r in Hounslow-Muttoni (2010) composite diagram (used here)Anisian
9086base MT3r.1rintv baseAnisian245.1555@ 0.90 up in E16 ChLAeg-2r/CG11r -- Base MT3r is about 90% up in E16 at Guandao (Mingsong Li, revised preliminary; used here). Was drawn in Houslow-Muttoni as about 90% up in Aegean; and was tentatively CG11r of Szurlies (in uppermost Rot Fm, or about middle of his Germanic cycle s7.7 (or 7.11 using Menning’s 2013 scale which indicated a gap of 3 cycles below the one-cycle "R" at 7.11) -- which would be about 0.5 myr lower; however that study didn’t extend high enough, and cyclicity may not always be 100kyr?) GTS04 -- Base = 0.75 of Paracrochordiceras Zone, which projected to nearly same level after adjusting base-Anisian age!Anisian
9087base MT3n.2nintv baseAnisian245.5572@ 0.72 up in MT3nAeg-1n/CG11n/MT3n -- ca. 72% up in main MT3n in Hounslow-Muttoni (2010) diagramAnisian
9088base MT3n.1rintv baseAnisian245.6576@ 0.65 up in MT3nAeg-1n/CG11n/MT3n -- ca. 65% up in main MT3n in Hounslow-Muttoni (2010) diagramAnisian
9089base MT3n.1nintv baseAnisian246.5900base s7.3 DeLAeg-1n/CG11n/MT3n -- Set to base of CG11n of Szurlies’07 (lowermost Rot, put 2 cycles up as base of Germanic cycle s7.3 to be consistent with Guandao cycle-mag and Wantou mag-UPb age model (YanChen’19 EPSL) relative to base-Ch. timorensis. However, it is drawn in Houslow-Muttoni as about 25% up in Aegean. A better scaling might require shifting "MT1n-MT1n" to be in Spathian (which may just be a problem relating base-Rot to GSSP in Romania)Anisian
9090base MT2rintv baseAnisian246.6580@ 0.60 up in MT1 -2Aeg-1r/MT1-2 -- Was ca. 60% up in combined MT1n-2r [=MT1 -2] in Hounslow-Muttoni (2010) diagramAnisian
9091base MT2nintv baseAnisian246.6835@ 0.45 up in MT1 -2Aeg-1r/MT1-2 -- Was ca. 40% up in combined MT1n-2r [=MT1 -2] in Hounslow-Muttoni (2010) diagram; but Wantou implies a slightly higher level (longer M1n) => 45% used hereAnisian
9092base MT1rintv baseAnisian246.7175@ 0.25 up in MT1 -2Aeg-1r/MT1-2 -- Was ca. 20% up in combined MT1n-2r in Hounslow-Muttoni (2010) diagram; but Wantou implies a slightly longer duration => 25% used hereAnisian
9093base MT1nintv baseOlenekian246.7600@ 0.30 up in s7.1 DeLAeg-1r/MT1-2 -- Base of Ch. timorensis conodont considered to be of Aegean substage = base of polarity zone MT1n (using Hounslow proposed definition based on magnetostrat of Romanian GSSP candidate and the Guandao China GSSP candidate). Base Magzone sn10 shown in Hounslow as beginning about 5% up in Rot; but just slightly above base of R??t used here following Menning/Kozur/Szurlies = about 30% up in s7.1 to fit YanChen’19 (Wantou GSSP in EPSL). BUT, see note on MT3n.1n above => relative to base-Rot, may be in traditional "German Spathian". K?rschner and Herngreen, 2010 place base-Anisian might be one cycle lower => 0.1 myr older; however, this would not fit the magnetostrat of the Romanian or S.China GSSP candidates. In contrast, the Zurich group prefer to have base-Anisian higher than FAD of Ch. timorensis.Olenekian
9094base CG10rintv baseOlenekian246.9700preset age: set as 246.97 Ma following YanChen’19 (Wantou GSSP in EPSL)CG10r/LT9r -- CG10r base set as 246.97 Ma following YanChen’19 (Wantou GSSP in EPSL). Was was ca. 35% up in s6.3 (Szurlies’07; Fig.6), which would be 246.92 Ma (and was 20% up in s6.4 in Szurlies’04). Upper part across base-Anisian has more detail (MT1-MT2) following Hounslow-Muttoni (2010)Olenekian
9095base CG10nintv baseOlenekian247.0700@ 0.20 up in s6.2 DeLCG10n/LT9n -- Base of CG10n is 20% up in s6.2 (Szurlies’07; Fig. 6)Olenekian
9096base CG9rintv baseOlenekian247.1200@ 0.70 up in s6.1 DeLCG9r at ca. 70% up in s6.1 (Szurlies’07; Fig. 6) -- NOTE that this is a BRIEF reversed-zone; and therefore 9n-10n are one major zone.Olenekian
9097base CG9n.3nintv baseOlenekian247.6000@ 0.90 up in s5.10 DeLCG9n.3n base at ca. 90% up in s5.10 (Szurlies’07; fig. 7)Olenekian
9098base CG9n.2rintv baseOlenekian247.6400@ 0.50 up in s5.10 DeLBrief CG9n.2r subchron base at at middle of s5.10 (Szurlies’07, Fig. 7)Olenekian
9099base CG9n.2nintv baseOlenekian247.9650@ 0.25 up in s5.7 DeLCG9n.2n base ca. 25% up in s5.7 (Szurlies’07; Fig.7)Olenekian
9100base CG9n.1rintv baseOlenekian248.0250@ 0.65 up in s5.6 DeLCG9n.1r subchron base ca. 65% up in s5.6 (Szurlies’07; Fig.7)Olenekian
9101base CG9n.1nintv baseOlenekian248.1250@ 0.65 up in s5.5 DeLCB9n base ca. 65% up in s5.5 (Szurlies’07; Fig.7) (was base of s5.8 in Szurliles’04)Olenekian
9102base CG8rintv baseOlenekian248.2400@ 0.50 up in s5.4 DeLCG8r base in middle of s5.4 (Szurlies’07; Fig.7) (was base of s5.6 in Szurliles’04); Top of Smithian placed at top of "SmN3?Olenekian
9103base CG8nintv baseOlenekian248.7400@ 0.50 up in s4.3 DeLCG8n base at middle of cycle s4.3 (dashed)Olenekian
9104base CG7rintv baseOlenekian248.9400@ 0.50 up in s4.1 DeLCG7r base at middle of cycle s4.1 (dashed)Olenekian
9105base CG7nintv baseOlenekian249.2900base s3.10 DeLsn5 (CG7n) base at base of cycle s3.10. Szurlies, 2004 shows as base of upper of 9 cycles in s3; but there are 12 cycles, therefore adjusted downward.Olenekian
9106base CG6rintv baseOlenekian249.8650@ 0.25 up in s3.4 DeLsr4 (CG6r) base at about 25% up in Germanic cycle s3.4 (Szurlies, 2004)Olenekian
9107base CG6nintv baseInduan249.9250@ 0.65 up in s3.3 DeLsn4 (CG6n) base in middle (65% used here to fit Chaoho offset of base-Olenekian) of Germanic cycle s3.3 (Szurlies, 2004). Top of Dienerian placed at base of SmN1Induan
9108base CG5rintv baseInduan250.3620@ 0.20 up in s2.8 DeLLT3r (Hounslow), sr3 (Szurlies), with base (Szurlies, 2003) at 10% up in Germanic cycle s2.8. GTS04 -- Base (estimated) = 0.28 of Dienerian (about 0.6 of P. candidus Zone, Arctic)Induan
9109base CG5nintv baseInduan250.5400@ 0.90 up in s2.3 DeLLT2n (Hounslow), sn3 (Szurlies), with base (Szurlies, 2003) at 90% up in Germanic cycle s2.3. GTS04 -- Base (estimated) = 0.03 of Dienerian (about 0.2 of P. candidus Zone, Arctic)Induan
9110base CG4rintv baseInduan251.0100@ 0.20 up in s1.9 DeLTop of Griesbachian placed in upper GR2. LT2r (Hounslow), GR2 (Ogg) and sr2 (Szurlies), with base (Szurlies, 2003) at 20% up in Germanic cycle s1.9. Middle of sr2 = base of Dienerian. GTS04 -- Base GR2 (estimated) = 0.65 of combined P. strigatus and O. communes Zones, Arctic.Induan
9111base CG4nintv baseInduan251.1200@ 0.10 up in s1.8 DeLLT2n (Hounslow), GN2 (Ogg), sn2 (Szurlies’03), and CG4n (Szurlies’07)with base (Szurlies, 2003) at 10% up in Germanic cycle s1.8. Age from proportional scaling of ammonite zonal units. GTS04 - Base (estimated) = 0.4 of combined P. strigatus and O. communes Zones, ArcticInduan
9112base CG3rintv baseInduan251.1800@ 0.50 up in s1.7 DeLLT1r (Hounslow), GR1 (Ogg) sr1 (Szurlies’03) and CG3r (Szurlies’07), with base (Szurlies, 2003) at 40% up in Germanic cycle s1.7. GTS04 approx -- Base (estimated) = 0.88 of new T. pascoei Zone, ArcticInduan
9113base CG3nintv baseInduan251.9000@ 0.30 up in z7.u DeLLT1n (Hounslow), GN1 (Ogg), sn1 (Szurlies’03) and CG3n (Szurlies’07), with base (Szurlies, 2007) at about 30% up in Germanic cycle z7.b [=s7.u] GTS04 -- Base (estimated) = 0.2 of O. concavum Zone, Arctic. Kozur (2003) estimates base at 0.2 myr below P/T from German cycles, which fits projection in GTS04. He also implies that top is 0.4 myr above P/T, which fits UPb of Meishan for its limits (but GTS2004 had as much longer, based on "equal ammonite subzones")Induan
9114base CG2rintv baseChanghsingian252.0300base z7.1 DeLLT1n.1r (Hounslow), lowermost GN1 (Ogg) and zrz (Szulies), with base (Szurlies, 2003) at about base of Germanic cycle z7.1.Changhsingian
9115base CG2nintv baseChanghsingian252.4300base z4.3 DeLLT1n.1n (Hounslow), lowermost GN1 (Ogg) and zrn (Szurlies), with base (Szurlies, 2003) at about base of 400-kyr Germanic cycle z4.3. GTS04 -- had been lower GN1 with base in lowermost O. concavum. NOTE: Permian version used Steiner instead, which has a longer R extending down from base of sn1 to 251.62 (0.4 myr, instead of 0.13 here), then a brief N.Changhsingian
10761base Chang-R chronintv baseChanghsingian252.8605@ 0.59 up in Changhsingian59% above base of ChanghsingianChanghsingian
10760base Chang-N.1n subchronintv baseChanghsingian253.3524@ 0.38 up in Changhsingian38% above base of ChanghsingianChanghsingian
10759base Chang-N.1r subchronintv baseChanghsingian253.4461@ 0.34 up in Changhsingian34% above base of ChanghsingianChanghsingian
10758base Chang-N.2n subchronintv baseChanghsingian253.8444@ 0.17 up in Changhsingian17% above base of ChanghsingianChanghsingian
10757base Chang-N.2r subchronintv baseChanghsingian253.8912@ 0.15 up in Changhsingian15% above base of ChanghsingianChanghsingian
10755base Chang-N.3r subchronintv baseChanghsingian254.1489@ 0.04 up in ChanghsingianBase of ChanghsingianChanghsingian
10756base Chang-N.3n subchronintv baseChanghsingian254.1489@ 0.04 up in Changhsingian4% above base of ChanghsingianChanghsingian
10754base Chang-N chronintv baseWuchiapingian255.9400@ 0.68 up in Wuchiapingian68% above base in WuchiapingianWuchiapingian
10753base Wuchchia-R.1r subchronintv baseWuchiapingian257.8496@ 0.32 up in Wuchiapingian32% above base in WuchiapingianWuchiapingian
10752base Wuchchia-R.2n subchronintv baseWuchiapingian258.0087@ 0.29 up in Wuchiapingian29% above base in WuchiapingianWuchiapingian
10751base Wuchchia-R chronintv baseCapitanian259.8346@ 0.94 up in Capitanian94% above base in CapitanianCapitanian
10750base Capit-N.1n subchronintv baseCapitanian260.4099@ 0.82 up in Capitanian82% above base in CapitanianCapitanian
10749base Capit-N.1r subchronintv baseCapitanian260.5537@ 0.79 up in Capitanian79% above base in CapitanianCapitanian
10748base Capit-N chronintv baseCapitanian261.2249@ 0.65 up in Capitanian65% above base in Capitanian. Kirschvink et al (2015; PPP) imply the base might be about 80% up in Yabeina foram zone, which would be ca. 1 myr lower. However, they do not resolve age of the top of this N-dominated upper Capitanian due to barren interval at the top.Capitanian
10747base Capit-R.1r subchronintv baseCapitanian262.4234@ 0.40 up in Capitanian40% above base in CapitanianCapitanian
10746base Capit-R.1n subchronintv baseCapitanian262.5672@ 0.37 up in Capitanian37% above base in Capitanian; although it might be lower (Kirschvink et al., 2015, PPP)Capitanian
10745base Capit-R chronintv baseWordian265.5583@ 0.75 up in Wordian75% above base in WordianWordian
10744base Word-N chronintv baseWordian267.2624@ 0.40 up in Wordian40% above base in Wordian (unlike GTS04; see evaluation in Steiner, 2006); but Kirschvink et al. (2015) find an N-zone indications near Roadian-Wordian boundary (upper N. craticulifera and lower N. margaritae foram zones)Wordian
10743top Kiaman-R.u1 subchronintv topArtinskian286.6382@ 0.54 up in Artinskian44% above base in Artinskian. This Reversed-zone, and all underlying R-dominated interval, is the Kiaman Reversed Hyperchron.MISTAKE? the notes say 44% above base but equation gives 54%Artinskian
10742base Kiaman-R.u1 subchronintv baseArtinskian286.9122@ 0.50 up in Artinskian41% above base in Artinskian. In GTS04 diagram, but not explained in text => made 'U'MISTAKE? the notes say 41% above base but equation gives 49%Artinskian
10741top Kiaman-R.u2 subchronintv topAsselian295.8030@ 0.60 up in Uskalykian RuSt60% up in Uskalykian Russian stage; Davydov'12 chart. GTS08 = 23% above base in AsselianAsselian
10740base Kiaman-R.u2 subchronintv baseAsselian296.3520@ 0.40 up in Uskalykian RuStMiddle (40 to 60%) of Uskalykian Russian stage. GTS08 = 20% above base in Asselian. In Davydov's compilation (after Khramov), but not well verified.Asselian
10739top Kartamyshian N subchronintv topGzhelian299.1452@ 0.80 up in Melekhovian RuSt80% up in Melekhovian Regional stage. GTS08 = 98% above base in GzhelianGzhelian
10738base Kartamyshian N subchronintv baseGzhelian299.4641@ 0.55 up in Melekhovian RuSt55-80% up in Melekhovin Regional stage in Gzhelian (Davydov'12 chart). Marker for Perm-Carb boundary (see GTS2004, page 235, right column; citing Davydov and Khramov'91)Gzhelian
10737top Kiaman-R.u3 subchronintv topGzhelian300.5121@ 0.70 up in Noginskian RuSt70% up in Noginian Regional stage in Gzhelian (Davydov'12 chart). GTS08 = 37% above base in GzhelianGzhelian
10736base Kiaman-R.u3 subchronintv baseGzhelian300.6852@ 0.55 up in Noginskian RuSt55-70% up in Noginian Regional stage in Gzhelian (Davydov'12 chart). GTS08 = 36 % above base in Gzhelian. In Davydov's compilation (after Khramov), but not well verified.Gzhelian
10735top Kiaman-R.u4 subchronintv topGzhelian300.9160@ 0.35 up in Noginskian RuSt35% up in Noginian Regional stage in Gzhelian (Davydov'12 chart). GTS08 = 30% above base in GzhelianGzhelian
10734base Kiaman-R.u4 subchronintv baseGzhelian301.0892@ 0.20 up in Noginskian RuSt20-35% up in Noginian Regional stage in Gzhelian (Davydov'12 chart). GTS08 = 29% above base in Gzhelian. In Davydov's compilation (after Khramov), but not well verified.Gzhelian
10733top Kiaman-R.u5 subchronintv topKasimovian304.8622@ 0.08 up in Dorogomilovian RuSt8% up in Dorogomilovian Regional stage in Gzhelian (Davydov'12 chart). GTS08 = 46% above base in KasimovianKasimovian
10732base Kiaman-R.u5 subchronintv baseKasimovian304.9650base Dorogomilovian RuSt0-8% up in Dorogomilovian Regional stage in Gzhelian (Davydov'12 chart). GTS08 = 43% above base in Kasimovian. This, and underlying normal-polarity events were called Donetzian Mixed-polarity Hyperchron (GTS04), but not verified outside of Khramov's work.Kasimovian
10731top Kiaman-R.u6 subchronintv topMoscovian308.5002@ 0.28 up in Myachkovian RuSt28% up in Myachkovian Regional stage in Moscovian (Davydov'12 chart). GTS08 = 73% above base in MoscovianCHECK - the equation placed the event at 28% up between base Myachkovian and base Peskovian horizon, but thiswasprobably a mistake so I have used 28% up in MyachkovianMoscovian
10730base Kiaman-R.u6 subchronintv baseMoscovian308.6646@ 0.20 up in Myachkovian RuSt20-28% up in Myachkovian Regional stage in Moscovian (Davydov'12 chart). GTS08 = 71% above base in Moscovian. Khramov had a set of 3 normal-polarity events as part of Donetzian Mixed-polarity Hyperchron (GTS04), but not yet verified outside of his work.CHECK as with previous event the equation was probably misentered. Moscovian
10729top Kiaman-R.u7 subchronintv topMoscovian311.2628@ 0.10 up in Podolskian RuSt10% up in Podolian Regional stage in Moscovian (Davydov'12 chart). GTS08 = 53% above base in MoscovianMoscovian
10728base Kiaman-R.u7 subchronintv baseMoscovian311.3843@ 0.05 up in Podolskian RuSt5-10% up in Podolian Regional stage in Moscovian (Davydov'12 chart). GTS08 = 51% above base in Moscovian. Khramov had a set of 3 normal-polarity events as part of Donetzian Mixed-polarity Hyperchron (GTS04), but not yet verified outside of his work.Moscovian
10727top Kiaman-R.u8 subchronintv topMoscovian312.7694@ 0.48 up in Kashirian RuSt48% up in Kashirian Regional stage in Moscovian (Davydov'12 chart). GRS08 = 34% above base in MoscovianMoscovian
10726base Kiaman-R.u8 subchronintv baseMoscovian312.9638@ 0.40 up in Kashirian RuSt40-48% up in Kashirian Regional stage in Moscovian (Davydov'12 chart). GTS08 = 33% above base in Moscovian. Khramov had a set of 3 normal-polarity events as part of Donetzian Mixed-polarity Hyperchron (GTS04), but not yet verified outside of his work.Moscovian
10725base Kiaman Reversed-polarity Hyperchronintv baseBashkirian315.5860@ 0.60 up in Melekessian RuSt60% up in Melekesian Regional stage (Davydov'12 chart). GTS08 = 93 % above base (+Gap) in BashkirianBashkirian
10724base Bashk-R.u1 subchronintv baseBashkirian316.0252@ 0.42 up in Melekessian RuSt42-60% up in Melekesian Regional stage (Davydov'12 chart). GTS08 = 89% above base (+Gap) in BashkirianBashkirian
10723top Bashk-R.u2 subchronintv topBashkirian316.3180@ 0.30 up in Melekessian RuSt30% up in Melekesian Regional stage (Davydov'12 chart). GTS08 = 85% above base (+Gap) in BashkirianBashkirian
10722base Bashk-R.u2 subchronintv baseBashkirian316.4400@ 0.25 up in Melekessian RuSt25-30% up in Melekesian Regional stage (Davydov'12 chart). GTS08 = 83% above base (+Gap) in BashkirianBashkirian
10721top Bashk-R.u3 subchronintv topBashkirian316.7084@ 0.14 up in Melekessian RuSt14% up in Melekesian Regional stage (Davydov'12 chart). GTS08 = 781% above base (+Gap) in BashkirianBashkirian
10720base Bashk-R.u3 subchronintv baseBashkirian316.8304@ 0.09 up in Melekessian RuSt9-14% up in Melekesian Regional stage (Davydov'12 chart). GTS08 = 79% above base (+Gap) in BashkirianBashkirian
10719top Bashk-R.u4 subchronintv topBashkirian317.0500base Melekessian RuStBase of Melekesian Regional stage (Davydov'12 chart). GTS08 = 76% above base (+Gap) in BashkirianBashkirian
10718base Bashk-R.u4 subchronintv baseBashkirian317.1305@ 0.95 up in Cheremshanian RuSt95% up in Cheremshanian Regional stage (Davydov'12 chart). GTS08 = 74% above base (+Gap) in BashkirianBashkirian
10717base Bashk-R.r4 subchronintv baseBashkirian317.3559@ 0.81 up in Cheremshanian RuSt81% up in Cheremshanian Regional stage (Davydov'12 chart). 71% above base (+Gap) in BashkirianBashkirian
10716base N8? subchronintv baseBashkirian317.4203@ 0.77 up in Cheremshanian RuSt77-81% up in Cheremshanian Regional stage (Davydov'12 chart). GTS08 = 69% above base (+Gap) in BashkirianBashkirian
10715base Wanganui Reversed?-r1 subchronintv baseBashkirian318.1770@ 0.30 up in Cheremshanian RuSt30% up in Cheremshanian Regional stage (Davydov'12 chart). GTS08 = 59% above base (+Gap) in Bashkirian. Note that Opdyke et al (2000) interpret Australian 'Wanganui Reversed' to include a N-polarity event 'N7' in Appalachians.Bashkirian
10714base N7? subchronintv baseBashkirian319.4940@ 0.40 up in Prikamian RuSt40% up in Prikamian Regional stage (Davydov'12 chart). GTS08 = 44% above base (+Gap) in Bashkirian. This event of Davydov's compilation might fit the lower-Morrowan N-zone of Opkyke et al (2000); which implies that their thin N6 (shortly above N5) might be merged here with N5 (as is the case in Australia?).Bashkirian
10713base Wanganui Reversed?-r2 subchronintv baseBashkirian322.5058@ 0.70 up in Voznesenian RuStProjected as 70% up in Voznesenian Regional stage (Davydov'12 chart). GTS08 = 4% above base (+Gap) in BashkirianBashkirian
10712base N5 subchronintv baseBashkirian323.2084@ 0.15 up in Voznesenian RuStProjected as 15% up in Voznesenian Regional stage (Davydov'12 chart). GTS08 = Base of Bashkirian (above Gap)Bashkirian
10711top N2? subchronintv topSerpukhovian323.7685@ 0.70 up in Zapaltjubian RuStProjected as 70% up in Zapaltyubian Regional stage (Davydov'12 chart). Considered to be Reversed-zone on Davydov'12 chart; but seems U would be better (gap in Appalachian strat). GTS08 = Spans GAPs (large version). GTS04 magstrat assumed to fit Eurasia strat, but across GapsSerpukhovian
10710base N2? subchronintv baseSerpukhovian324.3213@ 0.25 up in Zapaltjubian RuStProjected as 25% up in Zapaltyubian Regional stage (Davydov'12 chart). GTS08 = 98% above base in Serpukhovian (minus top Gap). Opdyke et al (2000) have brief N2 and N1 in in uppermost Chesterian (below hiatus). But, Davydov'12 has only a single N zone (assigned here as N2?)Serpukhovian
10709base Serp-R subchronintv baseSerpukhovian329.7229@ 0.60 up in Tarusian RuStProjected as 60% up in Tarusian Regional stage (Davydov'12 chart). GTS08 = 32% above base in Serpukhovian (minus top Gap)Serpukhovian
10708base N1? subchronintv baseSerpukhovian329.9800@ 0.35 up in Tarusian RuStProjected as 35-60% up in Tarusian Regional stage (Davydov'12 chart). GTS08 = 20% above base in Serpukhovian (minus top Gap). Opdyke et al (2000) have an N1 in mid-Chesterian, but no magnetic record below.Serpukhovian
10707base Vis-R1 subchronintv baseVisean331.2497@ 0.50 up in Venevian RuSt50% up in Venevian Regional stage (Davydov'12 chart). GTS08 = 97% above base in ViseanVisean
10706base Vis-N1 subchronintv baseVisean331.7954@ 0.20 up in Venevian RuStProjected as 20-50% up in Venevian Regional stage (Davydov'12 chart). GTS08 = 89% above base in ViseanVisean
10705base Vis-R2.r1 subchronintv baseVisean332.0501@ 0.06 up in Venevian RuSt6% up in Venevian Regional stage (Davydov'12 chart). GTS08 = 84% above base in ViseanVisean
10704base Vis-R2.n2 subchronintv baseVisean332.1229@ 0.02 up in Venevian RuStProjected as 2-6% up in Venevian Regional stage (Davydov'12 chart). GTS08 = 82% above base in ViseanVisean
10703base Vis-R2.r2 subchronintv baseVisean332.3025@ 0.92 up in Mikhailovian RuSt92% up in Mikhailovian Regional stage (Davydov'12 chart). GTS08 = 80.3% above base in ViseanVisean
10702base Vis-R2.n3 subchronintv baseVisean332.4099@ 0.86 up in Mikhailovian RuStProjected as 86-92% up in Mikhailovian Regional stage (Davydov'12 chart). GTS08 = 79.9% above base in ViseanVisean
10701base Vis-R2.r3 subchronintv baseVisean332.8931@ 0.59 up in Mikhailovian RuSt58% up in Mikhailovian Regional stage (Davydov'12 chart). GTS08 = 75% above base in ViseanVisean
10700base Vis-R2.n4 subchronintv baseVisean333.0184@ 0.52 up in Mikhailovian RuStProjected as 52-58% up in Mikhailovian Regional stage (Davydov'12 chart). GTS08 = 74% above base in ViseanVisean
10699base Vis-R2.r4 subchronintv baseVisean333.4301@ 0.29 up in Mikhailovian RuSt29% up in Mikhailovian Regional stage (Davydov'12 chart). GTS08 = 69% above base in ViseanVisean
10698base Vis-R2.n5 subchronintv baseVisean333.5553@ 0.22 up in Mikhailovian RuStProjected as 22-29% up in Mikhailovian Regional stage (Davydov'12 chart). GTS08 = 67% above base in ViseanVisean
10697base Vis-R2.r5 subchronintv baseVisean333.8596@ 0.05 up in Mikhailovian RuStProjected as 5% up in Mikhailovian Regional stage (Davydov'12 chart). GTS08 = 66% above base in ViseanVisean
10696base Vis-R2.n6 subchronintv baseVisean333.9898@ 0.98 up in Aleksinian RuSt98% up in Aleksian Regional stage (Davydov'12 chart). GTS08 = 64% above base in ViseanVisean
10695base Vis-R2.r7 subchronintv baseVisean334.3359@ 0.81 up in Aleksinian RuSt81% up in Aleksian Regional stage (Davydov'12 chart). GTS08 = 59% above base in ViseanVisean
10694base Vis-N2 subchronintv baseVisean334.8041@ 0.58 up in Aleksinian RuStProjected as 58-81% up in Aleksian Regional stage (Davydov'12 chart). GTS08 = 54% above base in ViseanVisean
10693base VisR3.1r subchronintv baseVisean335.8829@ 0.05 up in Aleksinian RuStProjected as 5% up in Aleksian Regional stage (Davydov'12 chart). GTS08 = 50% above base in ViseanVisean
10692base VisR3.2n subchronintv baseVisean336.1089@ 0.97 up in Tulian RuStProjected as 97% up in Tulian Regional stage (Davydov'12 chart). GTS08 = 47% above base in ViseanVisean
10691base VisR3.2r subchronintv baseVisean336.4401@ 0.89 up in Tulian RuSt89% up in Tulian Regional stage (Davydov'12 chart). GTS08 = 44% above base in ViseanVisean
10690base VisR3.3n subchronintv baseVisean336.5229@ 0.87 up in Tulian RuStProjected as 87-89% up in Tulian Regional stage (Davydov'12 chart). GTS08 = 43.6% above base in ViseanVisean
10689base VisR3.3nr subchronintv baseVisean340.8127@ 0.80 up in Bobrikian RuSt80% up in Bobrikovian Regional stage (Davydov'12 chart). GTS08 = 25% above base in ViseanVisean
10688base Vis-N3 subchronintv baseVisean342.7045@ 0.25 up in Bobrikian RuStProjected as 25-80% up in Bobrikovian Regional stage (Davydov'12 chart). GTS08 = 17% above base in ViseanVisean
10687base Vis-R3 subchronintv baseVisean344.0392@ 0.85 up in Radaevkian RuSt85% up in Radaevkian Regional stage (Davydov'12 chart). GTS08 = 12% above base in ViseanVisean
10686base Vis-N4 subchronintv baseVisean345.9386@ 0.25 up in Radaevkian RuStProjected as 25-85% up in Radaevkian Regional stage (Davydov'12 chart). GTS08 = 3% above base in ViseanVisean
10685base Vis-R4 subchronintv baseTournaisian348.0465@ 0.67 up in Kosvian RuStProjected as 67% up in Kosvinian Regional stage (Davydov'12 chart). GTS08 = 88% above base in TournaisianTournaisian
10684base Tourn-N1 subchronintv baseTournaisian353.4496@ 0.42 up in Cherepetian RuStMajor N interval. Projected as 42% up in Cherepetian Regional stage (Davydov'12 chart). GTS08 = 63% above base in TournaisianTournaisian
10683base Tourn-R1.r1 subchronintv baseTournaisian357.2637@ 0.32 up in Upinian RuSt32% up in Upinian Regional stage (Davydov'12 chart). GTS08 = 34% above base in TournaisianTournaisian
10682base Tourn-R1.n2 subchronintv baseTournaisian357.3517@ 0.25 up in Upinian RuStProjected as 25-32% up in Upinian Regional stage (Davydov'12 chart). GTS08 = 32% above base in TournaisianTournaisian
10681base Tourn-R1.r2 subchronintv baseTournaisian357.7049@ 0.90 up in Malevkian RuSt90% up in Malevkian Regional stage (Davydov'12 chart). GTS08 = 31% above base in TournaisianTournaisian
10680base Malevkian-N.1intv baseTournaisian357.7750@ 0.72 up in Malevkian RuStProjected as 72-90% up in Upinian Regional stage (Davydov'12 chart). GTS08 = 28% above base in Tournaisiannotes say this si interval within Upinan but equation (places it in MalevkianTournaisian
10679base Malevkian-N.2intv baseTournaisian358.0165@ 0.10 up in Malevkian RuStProjected as 20% up in Upinian Regional stage (Davydov'12 chart). GTS08 = 16 % above base in TournaisianCHECK/MISTAKE? - notes say this interval is within the Upinan but equation places it in Malevkian. Data at the end of Carbnoniferous is confused. I have taken the age of the base of this interval from the Devonian workbook & TSC, it is a bit lower in the Permo-Carb workbook - this results in placement at 0.1 Malevikian (as used here)Tournaisian
12818base AusC DevSubchronTournaisian358.7525@ 1.05 up in Famennian81% above base in FamennianTournaisian
12817base AusB DevSubchronFamennian362.5025@ 0.73 up in Famennian56% above base in FamennianFamennian
12816base AusA DevSubchronFamennian366.8567@ 0.60 up in Upper Palmatolepis marginifera fCdontzAbout 60% up in Upper MarginiferaFamennian
12815base N12 DevChronFamennian366.9228@ 0.50 up in Upper Palmatolepis marginifera fCdontzMid-Upper MarginiferaFamennian
12814base R12 DevChron-Famennian367.9140base Palmatolepis marginifera bCdontZAbout base of MarginiferaFamennian
12813base M11n DevChronFamennian368.2680base Upper Palmatolepis rhomboidea fCdontzBase of Upper RhomboideaFamennian
12812base R10 DevChronFamennian368.6220base Palmatolepis rhomboidea bCdontzBase of RhomboideaFamennian
12811base M9n DevChronFamennian370.2150@ 0.50 up in Upper Palmatolepis triangularis fCdontzMiddle of Upper TriangularisFamennian
12810base R8 DevChronFamennian370.7460base Middle Palmatolepis triangularis fCdontzBase of Middle TriangularisFamennian
12809base N7 DevChronFrasnian371.5481@ 0.50 up in 13b fCdontzmid-13b = crosses FF boundaryFrasnian
12808base R6 DevChronFrasnian371.8120@ 0.80 up in 13a fCdontzabout 80% up in 13aFrasnian
12807base M5n DevChronFrasnian372.2128@ 0.10 up in 13a fCdontzMaybe 10% up in 13aFrasnian
12806base R4 DevChronFrasnian372.5820@ 0.50 up in 12 fCdontzmid-12Frasnian
12805base N3 DevChronFrasnian373.1670@ 0.50 up in 11 fCdontzmid-11; would seem to be Base of Donetzian Mixed-polarity Hyperchron; which was schematically beginning 2/3rds up in Frasnian; mixed intervalFrasnian
12804base R2 DevChronFrasnian373.8300base 10 fCdontzBase of 10Frasnian
12803base N1.n3 DevSubchronFrasnian374.6100base 8 fCdontzBase of 8Frasnian
12802base N1.r2 DevSubchronFrasnian374.8830@ 0.50 up in 7 fCdontzmid-7Frasnian
12801base N1.n2s ubchronFrasnian375.1560base 7 fCdontzBase of 7Frasnian
12800base N1.r1 DevSubchronFrasnian375.4290@ 0.50 up in 6 fCdontzmid-6 conodontFrasnian
12799base N1 DevChronFrasnian376.5600base 5 fCdontzBase of Conodont 5 is bases of sectionFrasnian
12798base Dev Poortly Known Interval cGivetian379.4792@ 0.91 up in Givetian90% above base in Givetian [placement recalculated in the workbook to 0.91]Givetian
12797base Dev Poortly Known Interval bGivetian382.4789@ 0.44 up in Givetian43% above base in Givetian; mixed interval [placement recalculated in the workbook to 0.44]Givetian
12796base Dev Poortly Known Interval aEifelian389.5966@ 0.52 up in Eifelian82% above base in Eifelian [placement recalculated in the workbook to 0.52]Eifelian
12795base Sayan N4 DevSubchronEmsian394.3000base EifelianBase of EifelianEmsian
12794base Sayan R3 DevSubchronEmsian403.1977@ 0.45 up in Emsian77% above base in Eifelian [placement recalculated in the workbook to 0.45]Emsian
12793base Sayan N3 DevSubchronEmsian403.7084@ 0.42 up in Emsian72% above base in Eifelian [placement recalculated in the workbook to 0.42]Emsian
12792base Sayan R2 DevSubchronEmsian404.7039@ 0.36 up in Emsian61% above base in Eifelian [placement recalculated in the workbook to 0.36]Emsian
12791base Sayan N2 DevSubchronEmsian405.2130@ 0.33 up in Emsian56% above base in Eifelian [placement recalculated in the workbook to 0.33]Emsian
12790base Sayan R1 DevSubchronLochkovian416.5303@ 0.37 up in Lochkovian51% above base in Lochkovian [placement recalculated in the workbook to 0.37]Lochkovian
12789base Sayan N1 DevSubchronLochkovian418.0305@ 0.15 up in LochkovianBase of Sayan (Rn) ?; 20% above base in Lochkovian [placement recalculated in the workbook to 0.15]Lochkovian

Dataset References

Cande, S. C. & Kent, D. V. (1995). Revised calibration of the Geomagnetic Polarity time scale for the Late Cretaceous and Cenozoic. Journal of Geophysical Research. 100: 6093-6095. gs

Hansma, J., et al. (2015). Late Devonian carbonate magnetostratigraphy from the Oscar and Horse Spring Ranges, Lennard Shelf, Canning Basin, Western Australia. Earth and Planetary Science Letters. 409: 232-242. gs

Hounslow, M. W. & Balabanov, Y. P. (2018). A geomagnetic polarity timescale for the Permian, calibrated to stage boundaries. In, Lucas, S. G. , and Shen, S. Z. (ed.) The Permian Timescale. Geological Society of London, Special Publications . 450: 61-103. gs

Hounslow, M. K. & Muttoni, G. (2010). The geomagnetic polarity timescale for the Triassic: linkage to stage boundary definitions. In, Lucas, S. G. (ed.) The Triassic Timescale. Geological Society of London, Special Publications . 334: 61-102. gs

Hounslow, M. W. (2020). A geomagnetic polarity time scale for the Carboniferous. Geological Society of London, Special Publications. in press.: -. gs

Husson, D., et al. (2011). Astronomical calibration of the Maastrichtian. Earth and Planetary Science Letters. 305: 328-340. gs

Kent, D. V., et al. (2018). Empirical evidence for stability of the 405-kiloyear Jupiter-Venus eccentricity cycle over hundreds of million years. Proceedings of the National Academy of Sciences, USA. 115(24): 6153-6158. gs

Ogg, J. G. (2020). Chapter 5 - Geomagnetic polarity time scale. In, Gradstein, F. M. , Ogg, J. G. , Schmitz, M. D. , and Ogg, G. M. (ed.) The Geologic Time Scale 2020. Elsevier, Boston, MA 1: 159-192. gs

Steiner, M. B. (2006). The magnetic polarity time scale across the Permian Triassic boundary. In, Lucas, S. G. , Cassinis, G. , and Schneider, J. W. (ed.) Non-Marine Permian Biostratigraphy and Biochronology. Geological Society of London, Special Publications . 265: 15-38. gs

Thibault, N., et al. (2012). Astronomical calibration of upper Campanian Maastrichtian carbon isotope events and calcareous plankton biostratigraphy in the Indian Ocean (ODP Hole 762C): implication for the age of the Campanian Maastrichtian boundary. Palaeogeography Palaeoclimatology Palaeoecology. 37- 378: 52-71. gs

Zhang, Y., et al. (2020). Late Triassic magnetostratigraphy from the Germanic Basin and the global correlation of the Carnian Pluvial Episode. Earth and Planetary Science Letters. 541: 1-15. gs


Column mock-up

This column mock-up plot is a simple plot of the data to allow visual comparison with the output from TimeScale Creator

The data plotted here are the columns from the magnetochronology dataset for the interval 0 - 500 Ma

The all events column is an optional extra column showing the interval tops and bases as well as the other events in the dataset. This does not correspond to a TSC column, but is useful for checking data.

finished!