An imaging spectrometer operating in the visible near infrared for the study of planetary surfaces

被引：1
|
作者：
Bellucci, G [1 ]
Formisano, V
Capaccioni, F
机构：
[1] CNR, Ist Fis Spazio Interplanetario, I-00133 Rome, Italy
[2] CNR, Ist Astrofis Spaziale, I-00133 Rome, Italy
来源：
PLANETARY AND SPACE SCIENCE | 1998年 / 46卷 / 9-10期
关键词：
D O I：
10.1016/S0032-0633(98)00032-4
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
This paper summarizes the capabilities, performances, and technical solutions of the Visible and Near InfraRed (VNIR) imaging spectrometer designed,for remote sensing of planetary surfaces from a satellite platform. The VNIR consists of a multichannel camera with a spectral range 0.35 < lambda < 1.05 mu m which acquires data in 288 spectral channels with a spectral resolution of 24.3 Angstrom. The instantaneous field of view of the instrument is 0.4 x 0.4 mrad. The simultaneous acquisition of both spatial and spectral data provides a powerful means for investigating the mineralogical and chemical composition of surfaces of solar system objects. The paper also reports some results from the first campaign of ground-based telescopic observations intended to test the instrument. (C) 1998 Elsevier Science Ltd. All rights reserved.
引用
收藏
页码：1277 / 1290
页数：14
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