Variations in solar magnetic activity during the last 200,000 years: is there a Sun-climate connection?

被引：36

作者：

Sharma, M ^{[1
]}

机构：

[1] Dartmouth Coll, Dept Earth Sci, Hanover, NH 03755 USA

来源：

EARTH AND PLANETARY SCIENCE LETTERS | 2002年 / 199卷 / 3-4期

基金：

美国国家科学基金会;

关键词：

solar activity; climate change; Be-10; cosmogenic elements; magnetic field; Milankovitch theory; solar cycles;

D O I：

10.1016/S0012-821X(02)00516-2

中图分类号：

P3 [地球物理学]; P59 [地球化学];

学科分类号：

0708 ; 070902 ;

摘要：

The production of Be-10 in the Earth's atmosphere depends on the galactic cosmic ray influx that, in turn, is affected by the solar surface magnetic activity and the geomagnetic dipole strength. Using the estimated changes in Be-10 production rate and the geomagnetic field intensity, variations in solar activity are calculated for the last 200 ka. Large variations in the solar activity are evident with the Sun experiencing periods of normal, enhanced and suppressed activity. The marine delta(18)O record and solar modulation are strongly correlated at the 100 ka timescale. It is proposed that variations in solar activity control the 100 ka glacial-interglacial cycles. However, the Be-10 production rate variations may have been under-estimated during the interval between 115 ka and 125 ka and may have biased the results. Future tests of the hypothesis are discussed. (C) 2002 Elsevier Science B.V. All rights reserved.

引用

页码：459 / 472

页数：14

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