The dominant photochemical reactions taking place in the ionospheres of Venus, Saturn, and Comet P/Halley are presented. It is shown that the differences in the ionospheres of these celestial bodies result from the different chemistry, energetics, and dynamics of the respective atmospheres. The role of photochemistry in the formation of the individual ionospheres is discussed.
Photochemistry of planetary ionospheres
Advances in Space Research ; 7 , 12 1
1987-01-01
Miscellaneous
No indication
English
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