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米兰科维奇理论与季风。

Milankovitch theory and monsoon.

作者信息

Cheng Hai, Li Hanying, Sha Lijuan, Sinha Ashish, Shi Zhengguo, Yin Qiuzhen, Lu Zhengyao, Zhao Debo, Cai Yanjun, Hu Yongyun, Hao Qingzhen, Tian Jun, Kathayat Gayatri, Dong Xiyu, Zhao Jingyao, Zhang Haiwei

机构信息

Institute of Global Environmental Change, Xi'an Jiaotong University, Xi'an 710049, China.

State Key Laboratory of Loess and Quaternary Geology, Institute of Earth Environment, Chinese Academy of Sciences, Xi'an 710061, China.

出版信息

Innovation (Camb). 2022 Oct 19;3(6):100338. doi: 10.1016/j.xinn.2022.100338. eCollection 2022 Nov 8.

DOI:10.1016/j.xinn.2022.100338
PMID:36353675
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC9637977/
Abstract

The widely accepted "Milankovitch theory" explains insolation-induced waxing and waning of the ice sheets and their effect on the global climate on orbital timescales. In the past half century, however, the theory has often come under scrutiny, especially regarding its "100-ka problem." Another drawback, but the one that has received less attention, is the "monsoon problem," which pertains to the exclusion of monsoon dynamics in classic Milankovitch theory even though the monsoon prevails over the vast low-latitude (∼30° N to ∼30° S) region that covers half of the Earth's surface and receives the bulk of solar radiation. In this review, we discuss the major issues with the current form of Milankovitch theory and the progress made at the research forefront. We suggest shifting the emphasis from the ultimate outcomes of the ice volume to the causal relationship between changes in northern high-latitude insolation and ice age termination events (or ice sheet melting rate) to help reconcile the classic "100-ka problem." We discuss the discrepancies associated with the characterization of monsoon dynamics, particularly the so-called "sea-land precession-phase paradox" and the "Chinese 100-ka problem." We suggest that many of these discrepancies are superficial and can be resolved by applying a holistic "monsoon system science" approach. Finally, we propose blending the conventional Kutzbach orbital monsoon hypothesis, which calls for summer insolation forcing of monsoons, with Milankovitch theory to formulate a combined "Milankovitch-Kutzbach hypothesis" that can potentially explain the dual nature of orbital hydrodynamics of the ice sheet and monsoon systems, as well as their interplays and respective relationships with the northern high-latitude insolation and inter-tropical insolation differential.

摘要

被广泛接受的“米兰科维奇理论”解释了日照量导致冰盖的消长及其在轨道时间尺度上对全球气候的影响。然而,在过去的半个世纪里,该理论经常受到审视,尤其是关于其“10万年问题”。另一个缺点,但较少受到关注的是“季风问题”,这涉及到经典米兰科维奇理论中排除了季风动力学,尽管季风在覆盖地球表面一半且接收大部分太阳辐射的广阔低纬度(约北纬30°至南纬30°)地区占主导地位。在这篇综述中,我们讨论了当前形式的米兰科维奇理论的主要问题以及前沿研究取得的进展。我们建议将重点从冰量的最终结果转移到北半球高纬度日照量变化与冰期终止事件(或冰盖融化速率)之间的因果关系上,以帮助调和经典的“10万年问题”。我们讨论了与季风动力学特征相关的差异,特别是所谓的“海陆岁差相位悖论”和“中国10万年问题”。我们认为其中许多差异是表面的,可以通过应用整体的“季风系统科学”方法来解决。最后,我们建议将传统的库兹巴赫轨道季风假说(该假说要求夏季日照量强迫季风)与米兰科维奇理论相结合,形成一个综合的“米兰科维奇 - 库兹巴赫假说”,该假说有可能解释冰盖和季风系统轨道流体动力学的双重性质,以及它们之间的相互作用和与北半球高纬度日照量和热带日照量差异的各自关系。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b37b/9637977/a35ac0d6fdae/gr10.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b37b/9637977/54ba1259fdf1/fx1.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b37b/9637977/ba554cdb6440/gr1.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b37b/9637977/f0211aab3599/gr2.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b37b/9637977/3e4b3531ccaf/gr3.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b37b/9637977/2319797a77f4/gr4.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b37b/9637977/0dca36fe1a73/gr5.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b37b/9637977/c9e0bc9e296d/gr6.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b37b/9637977/44e891e8bedb/gr7.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b37b/9637977/65a27bf5672f/gr8.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b37b/9637977/5de02c9dc42c/gr9.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b37b/9637977/a35ac0d6fdae/gr10.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b37b/9637977/54ba1259fdf1/fx1.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b37b/9637977/ba554cdb6440/gr1.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b37b/9637977/f0211aab3599/gr2.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b37b/9637977/3e4b3531ccaf/gr3.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b37b/9637977/2319797a77f4/gr4.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b37b/9637977/0dca36fe1a73/gr5.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b37b/9637977/c9e0bc9e296d/gr6.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b37b/9637977/44e891e8bedb/gr7.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b37b/9637977/65a27bf5672f/gr8.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b37b/9637977/5de02c9dc42c/gr9.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b37b/9637977/a35ac0d6fdae/gr10.jpg

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