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Vertical profiles of dust and ozone in the martian atmosphere deduced from solar occultation measurements

✍ Scribed by Blamont, J. E.; Chassefiere, E.; Goutail, J. P.; Mege, B.; Nunes-Pinharanda, M.; Souchon, G.; Krasnopolsky, V. A.; Kryskot, A. A.; Moroz, V. I.


Book ID
109761458
Publisher
Nature Publishing Group
Year
1989
Tongue
English
Weight
401 KB
Volume
341
Category
Article
ISSN
0028-0836

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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