Abstract
The spatial distribution of hydrogen atoms emitted from the rings of Saturn with a range of emission speeds are simulated by a Monte Carlo technique. This method makes it possible to examine the spatial profiles of the ring atmosphere under a variety of physical conditions.
Original language | English |
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Pages (from-to) | 8843-8849 |
Number of pages | 7 |
Journal | Journal of Geophysical Research E: Planets |
Volume | 89 |
Issue number | A10 |
DOIs | |
State | Published - 1984 |