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Observations of jupiter'S cloud structure near 8.5 μ
Published online by Cambridge University Press: 14 August 2015
Abstract
Measurements of the distribution of thermal flux along polar and equatorial scans across Jupiter suggest that the increase in brightness temperature near 8.5 μ observed by Gillett et al. may be caused by flux coming from near the cloud tops. Other possible sources are discussed and observational tests suggested which should clarify the thermal structure of the upper atmosphere.
- Type
- Part III: Outer Planets
- Information
- Symposium - International Astronomical Union , Volume 40: Planetary Atmospheres , 1971 , pp. 359 - 362
- Copyright
- Copyright © Reidel 1971