A three-dimensional azimuthally symmetric model atmosphere for Io 1. Photochemistry and the accumulation of a nightside atmosphere

Journal of Geophysical Research: Planets

Volumn 101, Issue E10, 1996, Pages 23243-23254

  Wong, Mau C ^a   Johnson, Robert E ^a  

^a University of Virginia   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 15944424388     PISSN: 01480227     EISSN: None     Source Type: Journal    
DOI: 10.1029/96JE02510     Document Type: Article

References (7)

1. 2 Atmosphere on Io with the Hubble Space Telescope, Icarus 111, 2-17, 1994.
2. Bird, R.B., W.E. Stewart, and E.N. Lightfoot, Transport Phenomena, John Wiley, New York, 1960.
3. 2 atmosphere on the nightside, Icarus 118, 418-422, 1995.
4. Fanale, F.P., W.B. Banerdt, L.S. Elson, T.V. Johnson, and R.W. Zurek, Io's surface: Its phase composition and influences on Io's atmosphere and Jupiter's magnetosphere, in Satellites of Jupiter, edited by D. Morrison, pp. 756-781, Univ. of Arizona Press, Tucson, 1982.
5. Fuller, E.N., P.D. Schattler, and J.C. Giddings, A new method for prediction of binary gas-phase diffusion coefficients, Ind. Eng. Chem., 58(5), 19-27, 1966.
6. Hapke, B., F. Graham, Spectral properties of condensed phases of disulfur monoxide, polysulfur oxide, and irradiated sulfur, Icarus, 79, 47-55, 1989.
7. Wong, M.C. and R.E. Johnson, A three-dimensional azimuthally symmetric model atmosphere for Io 2, Plasma effect on the surface, J. Geophys. Res., this issue.