Форма представления | Зарубежные монографии |
Год публикации | 2016 |
Язык | английский |
|
Балабанов Юрий Павлович, автор
|
|
Hounslow Mark W, автор
|
Библиографическое описание на языке оригинала |
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. |
Аннотация |
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. |
Ключевые слова |
geomagnetic polarity, Kiaman Superchron, Illawarra Superchron, normal magnetochrons, reverse polarity magnetochron |
Пожалуйста, используйте этот идентификатор, чтобы цитировать или ссылаться на эту карточку |
https://repository.kpfu.ru/?p_id=148303 |
Полная запись метаданных |
Поле DC |
Значение |
Язык |
dc.contributor.author |
Балабанов Юрий Павлович |
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/?p_id=148303 |
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 |
Зарубежные монографии |
ru_RU |
|