Astronomical tuning of the end-Permian extinction and the Early Triassic Epoch of South China and Germany
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- 作者：Mingsong Lia ; b ; mli69@jhu.edu" class="auth_mail" title="E-mail the corresponding author ; James Ogga ; c ; jogg@purdue.edu" class="auth_mail" title="E-mail the corresponding author ; Yang Zhanga ; c ; zhan2214@purdue.edu" class="auth_mail" title="E-mail the corresponding author ; Chunju Huanga ; huangcj@cug.edu.cn" class="auth_mail" title="E-mail the corresponding author ; Linda Hinnovb ; d ; lhinnov@gmu.edu" class="auth_mail" title="E-mail the corresponding author ; Zhong-Qiang Chena ; zhong.qiang.chen@cug.edu.cn" class="auth_mail" title="E-mail the corresponding author ; Zhuoyan Zoua ; zouzhyqd@gmail.com" class="auth_mail" title="E-mail the corresponding author
- 关键词：Triassic time scale ; cyclostratigraphy ; magnetostratigraphy ; mass extinction ; recovery ; end-Permian
- 刊名：Earth and Planetary Science Letters
- 出版年：2016
- 出版时间：1 May 2016
- 年：2016
- 卷：441
- 期：Complete
- 页码：10-25
- 全文大小：5662 K
文摘
- •
Astrochronology of four sections in South China yields an Early Triassic timescale.
- •
The end-Permian extinction duration was <40 kyr, and
excursion was <6 kyr.- •
The Smithian–Spathian boundary event and the
shift lasted 50 kyr.- •
The Induan and Olenekian stage durations are 2.0±0.1 myr and 3.1±0.1 myr.
- •
Duration of the Early Triassic Epoch is 5.1±0.1 myr.