The Cassini visual and infrared mapping spectrometer (VIMS) investigation

被引：361

作者：

Brown, RH ^{[1
]}

Baines, KH ^{[1
]}

Bellucci, G ^{[1
]}

Bibring, JP ^{[1
]}

Buratti, BJ ^{[1
]}

Capaccioni, F ^{[1
]}

Cerroni, P ^{[1
]}

Clark, RN ^{[1
]}

Coradini, A ^{[1
]}

Cruikshank, DP ^{[1
]}

Drossart, P ^{[1
]}

Formisano, V ^{[1
]}

Jaumann, R ^{[1
]}

Langevin, Y ^{[1
]}

Matson, DL ^{[1
]}

Mccord, TB ^{[1
]}

Mennella, V ^{[1
]}

Miller, E ^{[1
]}

Nelson, RM ^{[1
]}

Nicholson, PD ^{[1
]}

Sicardy, B ^{[1
]}

Sotin, C ^{[1
]}

机构：

[1] Univ Arizona, Dept Planetary Sci, Tucson, AZ 85721 USA

来源：

SPACE SCIENCE REVIEWS | 2004年 / 115卷 / 1-4期

关键词：

Cassini; Saturn; infrared mapping spectrometer;

D O I：

10.1007/s11214-004-1453-x

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The Cassini visual and infrared mapping spectrometer (VIMS) investigation is a multidisciplinary study of the Saturnian system. Visual and near-infrared imaging spectroscopy and high-speed spectrophotometry are the observational techniques. The scope of the investigation includes the rings, the surfaces of the icy satellites and Titan, and the atmospheres of Saturn and Titan. In this paper, we will elucidate the major scientific and measurement goals of the investigation, the major characteristics of the Cassini VIMS instrument, the instrument calibration, and operation, and the results of the recent Cassini flybys of Venus and the Earth-Moon system.

引用

页码：111 / 168

页数：58

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