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Structure of the Martian atmosphere from ε-Gem occultation observations

✍ Scribed by W.B. Hubbard


Publisher
Elsevier Science
Year
1982
Tongue
English
Weight
176 KB
Volume
2
Category
Article
ISSN
0273-1177

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Solar occultation observations of the Martian atmosphere from the Phobos spacecraft resulted in nine vertical profiles of volume extinction coefficient at 3.7 and \(1.9 \mu \mathrm{m}\) in the altitude range of 12-35 km. Interpretation of the profiles in terms of the Mie scattering theory, with the