Optical properties of the Martian aerosols in the visible spectral range

被引：7
|
作者：
Markiewicz, WJ
Keller, HU
Thomas, N
Titov, D
Forget, F
机构：
[1] Max Planck Inst Aeron, D-37191 Katlenburg Lindau, Germany
[2] Univ Paris 06, CNRS, Lab Mtorol Dynam, F-75252 Paris 05, France
来源：
PLANETARY ATMOSPHERES | 2002年 / 29卷 / 02期
关键词：
D O I：
10.1016/S0273-1177(01)00567-1
中图分类号：
V [航空、航天];
学科分类号：
08 ; 0825 ;
摘要：
Imager for Mars Pathfinder (IMP) obtained data of sky brightness as a function of the scattering angle, wavelength, time of day and Sol. This data set is fitted with model calculations to extract the size distribution, shape and the refractive index of the aerosols suspended in the atmosphere. The inferred optical parameters are discussed in context of diurnal variations and compared to those derived from Viking Landers cameras and Phobos KRFM radiometer data. The effects of the scattering and absorption of the solar radiation by the atmospheric aerosols are discussed in terms of their influence on the spectrophotometry of the Martian surface. (C) 2002 COSPAR. Published by Elsevier Science Ltd. All rights reserved.
引用
收藏
页码：175 / 181
页数：7
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