A PARTIALLY COLLISIONAL MODEL OF THE TITAN HYDROGEN TORUS (SATURN).
A numerical model has been developed for atomic hydrogen densities in the Titan hydrogen torus. The effects of occasional collisions were included in order to accurately simulate physical conditions inferred from the Voyager 1 and 2 Ultraviolet Spectrometer (UVS) results of Broadfoot et al. (1981) a...
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| Language: | en |
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The University of Arizona.
1987
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| Online Access: | http://hdl.handle.net/10150/184064 |