SOLAR-RADIATION INCIDENT ON THE MARTIAN SURFACE

被引:115
作者
KUHN, WR
ATREYA, SK
机构
[1] Department of Atmospheric and Oceanic Science, The University of Michigan, Ann Arbor, 48109, Michigan
关键词
Mars; Solar radiation;
D O I
10.1007/BF01732367
中图分类号
Q5 [生物化学]; Q7 [分子生物学];
学科分类号
071010 ; 081704 ;
摘要
Calculations indicate that the maximum daily solar radiation reaching the Martian surface is about 325 cal/cm2 during southern hemisphere summer at latitude of about 40°S. In the ultraviolet region of the spectrum, the radiation reaching the surface at wavelengths greater than 2800 Å is within 10% of the radiation incident on the atmosphere. There is significant extinction of radiation in the spectral region near 2500 Å in mid and high latitudes due to absorption of radiation by ozone; radiation reaching the surface may be reduced to one one-thousandth of that incident on the atmosphere during winter. Virtually no radiation of wavelengths less than 1900 Å reaches the surface because of absorption by the large column abundance of carbon dioxide. Daily and latitudinal distributions of radiation are presented for wavelengths of 3000, 2500 and 2000 Å. © 1979 Springer-Verlag.
引用
收藏
页码:57 / 64
页数:8
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