globalchange  > 过去全球变化的重建
DOI: 10.1007/s00382-013-1925-3
Scopus记录号: 2-s2.0-84899910217
论文题名:
Central antarctic climate response to the solar cycle
作者: Volobuev D.M.
刊名: Climate Dynamics
ISSN: 9307575
出版年: 2014
卷: 42, 期:2017-09-10
起始页码: 2469
结束页码: 2475
语种: 英语
英文关键词: Antarctic climate ; IHCP ; Solar cycle
英文摘要: Antarctic "Vostok" station works most closely to the center of the ice cap among permanent year-around stations. Climate conditions are exclusively stable: low precipitation level, cloudiness and wind velocity. These conditions can be considered as an ideal model laboratory to study the surface temperature response on solar irradiance variability during 11-year cycle of solar activity. Here we solve an inverse heat conductivity problem: calculate the boundary heat flux density (HFD) from known evolution of temperature. Using meteorological temperature record during (1958-2011) we calculated the HFD variation about 0.2-0.3 W/m2 in phase with solar activity cycle. This HFD variation is derived from 0.5 to 1 °C temperature variation and shows relatively high climate sensitivity per 0.1 % of solar radiation change. This effect can be due to the polar amplification phenomenon, which predicts a similar response 0.3-0.8 °C/0.1 % (Gal-Chen and Schneider in Tellus 28:108-121, 1975). The solar forcing (TSI) is disturbed by volcanic forcing (VF), so that their linear combination TSI + 0.5VF empirically provides higher correlation with HFD (r = 0.63 ± 0.22) than TSI (r = 0.50 ± 0.24) and VF (r = 0.41 ± 0.25) separately. TSI shows higher wavelet coherence and phase agreement with HFD than VF. © 2013 Springer-Verlag Berlin Heidelberg.
资助项目: RFBR, Russian Foundation for Basic Research ; RFBR, Russian Foundation for Basic Research
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资源类型: 期刊论文
标识符: http://119.78.100.158/handle/2HF3EXSE/54390
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作者单位: Pulkovo Observatory, 196140, Pulkovskoe sh. 65/1, Saint Petersburg, Russian Federation

Recommended Citation:
Volobuev D.M.. Central antarctic climate response to the solar cycle[J]. Climate Dynamics,2014-01-01,42(2017-09-10)
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