globalchange  > 全球变化的国际研究计划
DOI: 10.1016/j.gloplacha.2014.06.002
论文题名:
The impact of astronomical forcing on the Late Devonian greenhouse climate
作者: De Vleeschouwer D.; Crucifix M.; Bounceur N.; Claeys P.
ISSN: 0921-8530
出版年: 2014
卷: 120
起始页码: 65
结束页码: 80
语种: 英语
英文关键词: Astronomical forcing ; General circulation model ; HadSM3 ; Late Devonian ; Obliquity ; Precession
Scopus关键词: Carbon dioxide ; Climate change ; Computer simulation ; Feedback control ; Geochronology ; Isotopes ; Stratigraphy ; Time series ; Vegetation ; Astronomical forcing ; General circulation model ; HadSM3 ; Late Devonian ; Obliquity ; Precession ; Climate models ; astronomy ; biostratigraphy ; boundary condition ; climate change ; Devonian ; general circulation model ; Gondwana ; numerical model ; paleoclimate ; Paleozoic ; proxy climate record ; snow cover ; Poland
英文摘要: The geological record of the Paleozoic often exhibits cyclic features, in many cases the result of changes in paleoclimate. However, a thorough understanding of the processes that were driving Paleozoic climate change has not yet been reached. The main reason is relatively poor time-control on Paleozoic paleoclimate proxy records. This problem can be overcome by the identification of cyclic features resulting from astronomical climate forcing in the stratigraphic record. To correctly identify these cyclic features, it is necessary to quantify the effects of astronomical climate forcing under conditions different from today. In this work, we apply Late Devonian (375Ma) boundary conditions to the Hadley Centre general circulation model (HadSM3). We estimate the response of Late Devonian climate to astronomical forcing by keeping all other forcing factors (e.g. paleogeography, pCO2, vegetation distribution) fixed. Thirty-one different "snapshots" of Late Devonian climate are simulated, by running the model with different combinations of eccentricity (e), obliquity (ε) and precession (ω~). From the comparison of these 31 simulations, it appears that feedback mechanisms play an important role in the conversion of astronomically driven insolation variations into climate change, such as the formation of sea-ice and the development of an extensive snow cover on Gondwana. We compare the "median orbit" simulation to lithic indicators of paleoclimate to evaluate whether or not HadSM3 validly simulates Late Devonian climates. This comparison suggests that the model correctly locates the major climate zones. This study also tests the proposed link between the formation of ocean anoxia and high eccentricity (De Vleeschouwer et al., 2013) by comparing the δ18Ocarb record of the Frasnian-Famennian boundary interval from the Kowala section (Poland) with a simulated time series of astronomically forced changes in mean annual temperature at the paleolocation of Poland. The amplitude of climate change suggested by the isotope record is greater than that of the simulated climate. Hence, astronomically forced climate change may have been further amplified by other feedback mechanisms not considered here (e.g. CO2 and vegetation). Finally, the geologic and simulated time series correlate best when the Frasnian-Famennian negative isotope excursion aligns with maximum mean annual temperature in Poland, which is obtained when eccentricity and obliquity are simultaneously high. This finding supports a connection between Devonian ocean anoxic events and astronomical climate forcing. © 2014 Elsevier B.V.
URL: https://www.scopus.com/inward/record.uri?eid=2-s2.0-84902965126&doi=10.1016%2fj.gloplacha.2014.06.002&partnerID=40&md5=eafe982a9b0c8848ab33ce19fb9cf70b
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被引频次[WOS]:40   [查看WOS记录]     [查看WOS中相关记录]
资源类型: 期刊论文
标识符: http://119.78.100.158/handle/2HF3EXSE/11436
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作者单位: Earth System Sciences and Department of Geology, Vrije Universiteit Brussel, Pleinlaan 2, B-1050 Brussels, Belgium

Recommended Citation:
De Vleeschouwer D.,Crucifix M.,Bounceur N.,et al. The impact of astronomical forcing on the Late Devonian greenhouse climate[J],2014-01-01,120.
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