Radiative forcing of the stratosphere of Jupiter, Part I: Atmospheric cooling rates from Voyager to Cassini
We developed a line-by-line heating and cooling rate model for the stratosphere of Jupiter, based on two complete sets of global maps of temperature, CH and CH, retrieved from the Cassini and Voyager observations in the latitude and vertical plane, with a careful error analysis. The non-LTE effect i...
| Príomhchruthaitheoirí: | , , , , , , , |
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| Formáid: | Journal article |
| Foilsithe / Cruthaithe: |
2013
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