KFU. Card publication. A geomagnetic polarity timescale for the Permian, calibrated to stage boundaries

KAZAN
FEDERAL UNIVERSITY

- RUS
- 中文
- ES

A GEOMAGNETIC POLARITY TIMESCALE FOR THE PERMIAN, CALIBRATED TO STAGE BOUNDARIES

Form of presentation

International monographs

Year of publication

2016

��

��

Authors, employees of KFU

Balabanov Yuriy Pavlovich, author

Other authors

Hounslow Mark W, author

Bibliographic description in the original language

MARK W. HOUNSLOW & YURI P. BALABANOV A geomagnetic polarity timescale for the Permian, calibrated to stage boundaries / Lucas, S. G. & Shen, S. Z. (eds) The Permian Timescale. Geological Society, London, Special Publications, 43 p.

Annotation

The reverse polarity Kiaman Superchron has strong evidence for at least three, or probably four, normal magnetochrons during the early Permian. Normal magnetochrons are during the early Asselian (base CI1r.1n at 297.94+0.33 Ma), late Artinskian (CI2n at 281.24+2.3 Ma), mid-Kungurian (CI3n at 275.86+2.0 Ma) and Roadian (CI3r.an at 269.54+1.6 Ma). The mixed-polarity Illawarra Superchron begins in the early Wordian at 266.66+0.76 Ma. The Wordian? Capitanian interval is biased to normal polarity, but the basal Wuchiapingian begins the beginning of a significant reverse polarity magnetochron LP0r, with an overlying mixed-polarity interval through the later Lopingian.

Keywords

geomagnetic polarity, Kiaman Superchron, Illawarra Superchron, normal magnetochrons, reverse polarity magnetochron

Please use this ID to quote from or refer to the card

https://repository.kpfu.ru/eng/?p_id=148303&p_lang=2

Full metadata record

Field DC	Value	Language
dc.contributor.author	Balabanov Yuriy Pavlovich	ru_RU
dc.contributor.author	Hounslow Mark W	ru_RU
dc.date.accessioned	2016-01-01T00:00:00Z	ru_RU
dc.date.available	2016-01-01T00:00:00Z	ru_RU
dc.date.issued	2016	ru_RU
dc.identifier.citation	MARK W. HOUNSLOW & YURI P. BALABANOV A geomagnetic polarity timescale for the Permian, calibrated to stage boundaries / Lucas, S. G. & Shen, S. Z. (eds) The Permian Timescale. Geological Society, London, Special Publications, 43 p.	ru_RU
dc.identifier.uri	https://repository.kpfu.ru/eng/?p_id=148303&p_lang=2	ru_RU
dc.description.abstract	The reverse polarity Kiaman Superchron has strong evidence for at least three, or probably four, normal magnetochrons during the early Permian. Normal magnetochrons are during the early Asselian (base CI1r.1n at 297.94+0.33 Ma), late Artinskian (CI2n at 281.24+2.3 Ma), mid-Kungurian (CI3n at 275.86+2.0 Ma) and Roadian (CI3r.an at 269.54+1.6 Ma). The mixed-polarity Illawarra Superchron begins in the early Wordian at 266.66+0.76 Ma. The Wordian? Capitanian interval is biased to normal polarity, but the basal Wuchiapingian begins the beginning of a significant reverse polarity magnetochron LP0r, with an overlying mixed-polarity interval through the later Lopingian.	ru_RU
dc.language.iso	ru	ru_RU
dc.subject	geomagnetic polarity	ru_RU
dc.subject	Kiaman Superchron	ru_RU
dc.subject	Illawarra Superchron	ru_RU
dc.subject	normal magnetochrons	ru_RU
dc.subject	reverse polarity magnetochron	ru_RU
dc.title	A geomagnetic polarity timescale for the Permian, calibrated to stage boundaries	ru_RU
dc.type	International monographs	ru_RU