*(Revised) Manuscript, clean version Click here to download (Revised) Manuscript, clean version: Manuscript.pdf Click here to view linked References 1 2 3 4 5 Radiative Forcing of the Stratosphere of Jupiter, Part I: 6 7 Atmospheric Cooling Rates from Voyager to Cassini 8 9 10 a, b a c d e 11 X. Zhang *, C.A. Nixon , R.L. Shia , R.A. West , P.G. J. Irwin , R.V. Yelle , M.A. 12 a,c a 13 Allen , Y.L. Yung 14 15 16 17 18 a Division of Geological and Planetary Sciences, California Institute of Technology, 19 20 Pasadena, CA, 91125, USA 21 b 22 NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA 23 c 24 Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, 25 Pasadena, CA 91109, USA 26 d 27 Atmospheric, Oceanic, and Planetary Physics, University of Oxford, Clarendon 28 29 Laboratory, Parks Road, Oxford, OX1 3PU,UK 30 e 31 Department of Planetary Sciences, University of Arizona, Tucson, Arizona, USA 32 33 34 35 36 *Corresponding author at: Division of Geological and Planetary Sciences, California 37 38 Institute of Technology, Pasadena, CA, 91125, USA. 39 40 E-mail address:
[email protected] (X. Zhang) 41 42 43 44 45 46 47 Submitted to: 48 49 Plan. Space Sci. (PSS) Special issue on Outer planets systems 50 51 52 53 54 55 56 57 58 59 60 61 62 63 1 64 65 1 2 3 4 Abstract 5 6 7 8 We developed a line-by-line heating and cooling rate model for the stratosphere of 9 10 Jupiter, based on two complete sets of global maps of temperature, C2H2 and C2H6, 11 12 retrieved from the Cassini and Voyager observations in the latitude and vertical plane, 13 with a careful error analysis.