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Radiative Forcing of the Stratosphere of Jupiter: From Voyager to Cassini . Xi Zhang 1 , C. A. Nixon 2 , R. Shia 1 , R. A. West 3 , R. Morales-Juberias 4 , R. Cosentino 4 , P. G. Irwin 5 , T. Dowling 6 , M. A. Allen 3 , & Y. L. Yung 1
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Radiative Forcing of the Stratosphere of Jupiter:From Voyager to Cassini Xi Zhang1, C. A. Nixon2, R. Shia1, R. A. West3, R. Morales-Juberias4, R. Cosentino4, P. G. Irwin5, T. Dowling6, M. A. Allen3, & Y. L. Yung1 1Caltech; 2NASA GSFC/University of Maryland; 3JPL; 4New Mexico Institute of Mining and Technology; 5University of Oxford; 6University of Louisville
Radiative Forcing Longwave Cooling Shortwave Heating H2-H2 H2-He CH4 C2H2 C2H6 … CH4 Aerosol
Cooling Rates Voyager Cassini
Aerosol Retrieval (ISS) Equator CB3 MT3 UV1
Aerosol Retrieval (ISS) Mid-Latitude CB3 MT3 UV1
Aerosol Retrieval (ISS) North Pole CB3 MT3 UV1
Heating Rates CH4 + Aerosol CH4 Only
Radiative Forcing Voyager Cassini
Radiative Time Constant Conrath et al. (1990) This work