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

页码：1277 / 1290

页数：14

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