arkL edit interval

arkL

select id,columnx from arkL_columns where dataset_id like 10

View/Edit arkL Database interval - G. havanensis pfZ

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The age-window currently being used to search for terms for autocompletion is 24.201 -> 125.0559 Ma.

	interval above:	G. aegyptiaca pfZ
parent-intervals:	this interval:	G. havanensis pfZ	sub-intervals:
	interval below:	R. calcarata pfZ

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Interval data

intervalx:	G. havanensis pfZhas added abv?yesid: 3499 sort:
alternative_term:	G. havanensis zoneblock label:
formal term:	Globotruncanella havanensis pfZ
interval_type:
parent_interval:
dataset:	forams - planktic (dataset id = 10)
alt dataset:	(dataset id = )
TSC Column:	id:104
stage:
colour:
interval_notes:	DASHED (Used C33n.85, which is Gubbio level (Coccioni et al., 2015); see age discussion). Gap zone (LAD at base; FAD at top); which some zonations extend upward to FAD of G. gansseri as a "Globotruncana falsostuarti Zone". Calcarata was previously assigned to genus Globotruncanita. DASH -- SEPM’98 places at Chron C33n.85 (74.47 Ma on GTS04 magnetics); but Huber et al’08 assign as 75.57 Ma relative to those magnetics (which would be C33n.75; although their text says C32n.92).
compilation_notes:
refs to add:
linked refs:
preset_duration:
preset_duration_notes:
tracecode	; Q1base from event age; Q2top from event age; Q3a duration from base & top

	age2020	age		event	event_id	pup	in interval	age	age2020
Top:		74.2010	<---	FAD Globotruncana aegyptiaca	4354	0.0000	C32r.2r	74.201	00074.2000
Base:		75.0559	<---	LAD Radotruncana calcarata	4355	0.8500	C33n	75.0559	00075.0600
base notes	Radotruncana calcarata:<br>Datum calibration/notes = DASHED (Used C33n.85, which is Gubbio level (Coccioni et al., 2015); see age discussion). Gap zone (LAD at base; FAD at top); which some zonations extend upward to FAD of G. gansseri as a "Globotruncana falsostuarti Zone". Calcarata was previously assigned to genus Globotruncanita. DASH -- SEPM’98 places at Chron C33n.85 (74.47 Ma on GTS04 magnetics); but Huber et al’08 assign as 75.57 Ma relative to those magnetics (which would be C33n.75; although their text says C32n.92). .				comp notes

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Interval References

Dataset References