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, C2H2 and C2H6, retrieved from the Cassini and Voyager observations in the latitude and vertical plane, with a careful error analysis. The non-LTE effe...
Prif Awduron: | Zhang, X, Nixon, C, Shia, R, West, R, Irwin, P, Yelle, R, Allen, M, Yung, Y |
---|---|
Fformat: | Journal article |
Iaith: | English |
Cyhoeddwyd: |
Elsevier
2013
|
Eitemau Tebyg
-
Radiative forcing of the stratosphere of Jupiter, Part I: Atmospheric cooling rates from Voyager to Cassini
gan: Zhang, X, et al.
Cyhoeddwyd: (2013) -
Abundances of Jupiter's trace hydrocarbons from Voyager and Cassini
gan: Nixon, C, et al.
Cyhoeddwyd: (2010) -
Abundances of Jupiter's trace hydrocarbons from Voyager and Cassini
gan: Nixon, C, et al.
Cyhoeddwyd: (2010) -
Jupiter's auroral-related stratospheric heating and chemistry I: Analysis of Voyager-IRIS and Cassini-CIRS spectra
gan: Sinclair, J, et al.
Cyhoeddwyd: (2017) -
From Voyager-IRIS to Cassini-CIRS: Interannual variability in Saturn's stratosphere?
gan: Sinclair, J, et al.
Cyhoeddwyd: (2014)