select * from arkL_intervals where id=2647

View/Edit arkL Database interval - C-Sequence

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The age-window currently being used to search for terms for autocompletion is -49.9998 -> 133.65 Ma.
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parent-intervals:; this interval:C-Sequencesub-intervals: C29; C30; C31; C32; C33; C29r; C30n; C30r; C31n; C31r; C32n.1n; C32n.1r; C32n.2n; C32r.1r; C32r.1n; C32r.2r; C33n; C33r; C33r EXTENSION GTS2020; C1; C2; C2A; C3; C3A; C3B; C4; C4A; C5; C5A; C5AA; C5AB; C5AC; C5AD; C5B; C5C; C5D; C5E; C6; C6A; C6AA; C6B; C6C; C7; C7A; C8; C9; C10; C11; C12; C13; C15; C16; C17; C18; C19; C20; C21; C22; C23; C24; C25; C26; C27; C28; C1n (Brunhes); C1r.1r (Matuyama); C1r.1n (Jaramillo); C1r.2r (Matuyama continued); C1r.2n (Cobb Mountain); C1r.3r (Matuyama continued); C2n (Olduvai); C2r.1r (Matuyama continued); C2r.1n (Feni); C2r.2r (Matuyama continued); C2An.1n (Gauss); C2An.1r (Kaena); C2An.2n (Gauss continued); C2An.2r (Mammoth); C2An.3n (Gauss continued); C2Ar (Gilbert); C3n.1n (Cochiti); C3n.1r (Gilbert continued); C3n.2n (Nunivak); C3n.2r (Gilbert continued); C3n.3n (Sidufjall); C3n.3r (Gilbert continued); C3n.4n (Thvera); C3r ((Gilbert continued); C3An.1n; C3An.1r; C3An.2n; C3Ar; C3Bn; C3Br.1r; C3Br.1n; C3Br.2r; C3Br.2n; C3Br.3r; C4n.1n; C4n.1r; C4n.2n; C4r.1r; C4r.1n; C4r.2r; C4r.2r-1; C4An; C4Ar.1r; C4Ar.1n; C4Ar.2r; C4Ar.2n; C4Ar.3r; C5n.1n; C5n.1r; C5n.2n; C5r.1r; C5r.1n; C5r.2r; C5r.2r-1; C5r.2n; C5r.3r; C5An.1n; C5An.1r; C5An.2n; C5Ar.1r; C5Ar.1n; C5Ar.2r; C5Ar.2n; C5Ar.3r; C5AAn; C5AAr; C5ABn; C5ABr; C5ACn; C5ACr; C5ADn; C5ADr; C5Bn.1n; C5Bn.1r; C5Bn.2n; C5Br; C5Cn.1n; C5Cn.1r; C5Cn.2n; C5Cn.2r; C5Cn.3n; C5Cr; C5Dn; C5Dr.1r; C5Dr.1n; C5Dr.2r; C5En; C5Er; C6n; C6r; C6An.1n; C6An.1r; C6An.2n; C6Ar; C6AAn; C6AAr.1r; C6AAr.1n; C6AAr.2r; C6AAr.2n; C6AAr.3r; C6Bn.1n; C6Bn.1r; C6Bn.2n; C6Br; C6Cn.1n; C6Cn.1r; C6Cn.2n; C6Cn.2r; C6Cn.3n; C6Cr; C7n.1n; C7n.1r; C7n.2n; C7r; C7An; C7Ar; C8n.1n; C8n.1r; C8n.2n; C8r; C9n; C9r; C10n.1n; C10n.1r; C10n.2n; C10r; C11n.1n; C11n.1r; C11n.2n; C11r; C12n; C12r; C13n; C13r; C15n; C15r; C16n.1n; C16n.1r; C16n.2n; C16r; C17n.1n; C17n.1r; C17n.2n; C17n.2r; C17n.3n; C17r; C18n.1n; C18n.1r; C18n.2n; C18r; C19n; C19r; C20n; C20r; C21n; C21r; C22n; C22r; C23n.1n; C23n.1r; C23n.2n; C23r; C24n.1n; C24n.1r; C24n.2n; C24n.2r; C24n.3n; C24r; C25n; C25r; C26n; C26r; C27n; C27r; C28n; C28r; C29n; C1n; C1r; C2n; C2r; C2An; C2Ar; C3n; C3r; C3An; C3Br; C4n; C4r; C4Ar; C5n; C5r; C5An; C5Ar; C5Bn; C5Cn; C5Dr; C6An; C6AAr; C6Bn; C6Cn; C7n; C8n; C10n; C11n; C16n; C17n; C18n; C23n; C24n;
interval below:Cretaceous Normal Super-Chron ("Cretaceous Quiet Zone")

Interval data

intervalx:has added abv?id: 2647  sort:1
alternative_term:block label:
formal term:
interval_type:mfs
parent_interval:
dataset: magnetochronology (dataset id = 4)
alt dataset: (dataset id = )
subdataset:
TSC Column: id:125
stage:
polarity:
colour: Lithology:(id)
interval_notes:
compilation_notes:
refs to add:
linked refs:
preset_duration:
preset_duration_notes:
tracecode; Q2top from event age; Q1base from event age; Q3a duration from base & top


age2020ageeventevent_idpupin intervalageage2020
Top:0.0002 <--- 5881 0.0000 0.0002 00000.0000
Base:83.6500 <--- 30070.0000Campanian83.6500 00083.6500
base
notes
comp notes

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Interval References

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