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Photoemission Phenomena in the Solar System

Slanger, TG; Cravens, TE; Crovisier, J; Miller, S; Strobel, DF; (2008) Photoemission Phenomena in the Solar System. In: UNSPECIFIED (267 - 310). SPRINGER

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Abstract

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.

Type: Book chapter
Title: Photoemission Phenomena in the Solar System
DOI: 10.1007/s11214-008-9387-3
Keywords: Nightglow, Dayglow, Mars, Earth, Venus, Jupiter, Saturn, Uranus, Neptune, Titan, Comets, X-rays, Aurora, X-RAY-EMISSION, EXTREME-ULTRAVIOLET OBSERVATIONS, HUBBLE-SPACE-TELESCOPE, GROUND-BASED OBSERVATIONS, JOVIAN AURORAL ELECTRONS, TITANS UPPER-ATMOSPHERE, LYMAN-ALPHA EMISSION, OH PROMPT EMISSION, PLANET HD 209458B, COMET HALE-BOPP
UCL classification: UCL > Provost and Vice Provost Offices
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Science and Technology Studies
URI: http://discovery.ucl.ac.uk/id/eprint/101225
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