Observations of Martian aerosols with the imager for Mars pathfinder

被引：2

作者：

Thomas, N ^{[1
]}

Keller, HU ^{[1
]}

Markiewicz, WJ ^{[1
]}

Smith, PH ^{[1
]}

机构：

[1] UNIV ARIZONA,LUNAR & PLANETARY LAB,TUCSON,AZ 85721

来源：

PLANETARY ATMOSPHERES AND IONOSPHERES AND REFERENCE ATMOSPHERES | 1997年 / 19卷 / 08期

基金：

美国国家航空航天局;

关键词：

D O I：

10.1016/S0273-1177(97)00281-0

中图分类号：

V [航空、航天];

学科分类号：

08 ; 0825 ;

摘要：

The Imager for Mars Pathfinder (IMP) is a powerful tool for the analysis of Martian atmospheric aerosol content. This paper illustrates the capabilities of the IMP for this purpose and discusses some of the measurements that can be performed. The optical depth (by day and by night), sky brightness, atmospheric water content, the solar aureole structure, icy haloes, and cloud measurements can all be investigated by the IMP. A discussion of nighttime optical depth measurements is presented. The potential synergism between IMP atmospheric measurements and imaging of atmospheric phenomena from an orbiter is also briefly described. (C) 1997 COSPAR. Published by Elsevier Science Ltd.

引用

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页码：1271 / 1276

页数：6

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