Photoemission Phenomena in the Solar System

被引：20

作者：

Slanger, T. G. ^{[1
]}

Cravens, T. E. ^{[2
]}

Crovisier, J. ^{[3
]}

Miller, S. ^{[4
]}

Strobel, D. F. ^{[5
]}

机构：

[1] SRI Int, Mol Phys Lab, Menlo Pk, CA 94025 USA

[2] Univ Kansas, Dept Phys & Astron, Lawrence, KS 66045 USA

[3] Observ Paris, LESIA, F-92195 Meudon, France

[4] UCL, Dept Phys & Astron, London WC1E 6BT, England

[5] Johns Hopkins Univ, Dept Earth & Planetary Sci, Baltimore, MD 21218 USA

来源：

SPACE SCIENCE REVIEWS | 2008年 / 139卷 / 1-4期

关键词：

Nightglow; Dayglow; Mars; Earth; Venus; Jupiter; Saturn; Uranus; Neptune; Titan; Comets; X-rays; Aurora;

D O I：

10.1007/s11214-008-9387-3

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Much of what we know about the atmospheres of the planets and other bodies in the solar system comes from detection of photons over a wide wavelength range, from X-rays to radio waves. In this chapter, we present current information in various categories-measurements of the airglows of the terrestrial planets, the dayglows of the outer planets and satellites, aurora throughout the solar system, observations of cometary spectra, and the emission of X-rays from a variety of planetary bodies.

引用

页码：267 / 310

页数：44

共 263 条

[1] Titan airglow spectra from Cassini Ultraviolet Imaging Spectrograph (UVIS): EUV analysis [J].