The achievements and potential of ISO archive for planetary studies

被引：0

作者：

Fouchet, T ^{[1
]}

机构：

[1] Univ Oxford, Atmospher Ocean & Planetary Phys, Oxford OX1 3PU, England

来源：

PROCEEDINGS OF THE SYMPOSIUM ON EXPLOITING THE ISO DATA ARCHIVE: INFRARED ASTRONOMY IN THE INTERNET AGE | 2003年 / 511卷

关键词：

ISO; solar system; planets;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The ISO observations of planetary objects have given several outstanding results. However, the potential from the ISO archive is still high as many observations, or some spectral ranges have not been analysed yet. The most striking example being the ISOCAM observations of Jupiter and Saturn. This situation is due to the difficulty to reduce and calibrate the high flux (Up to 10(6) Jy) planetary observations, to the lack of spectroscopic data or numerical tools to accurately analyse the data, and also because the planetary community focused on the most unexpected observations. The achievements and potential from ISO archive encompasses the atmospheric isotopic composition, the oxygen and hydrocarbon stratospheric chemistry in the Giant Planets and Titan, the cloud structure of Jupiter and Saturn, and the composition of planetary surfaces.

引用

页码：41 / 46

页数：6

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