Infrared spectra of Mars were taken with the two complementary spectrometers onboard the European Space Agency's Infrared Space Observatory (ISO), in both moderate-and high-resolution mode. From the strengths of the observed water lines we derived information about the vertical distribution of water
โฆ LIBER โฆ
Exchange of water vapor between the atmosphere and surface of Mars
โ Scribed by C.B. Leovy
- Publisher
- Elsevier Science
- Year
- 1973
- Tongue
- English
- Weight
- 503 KB
- Volume
- 18
- Category
- Article
- ISSN
- 0019-1035
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