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Survival probabilities for interstellar hydrogen flowing into the interplanetary system from far regions of the heliosphere
Authors:Joseph A Kunc
Institution:Space Sciences Institute, University of Southern California, University Park, Los Angeles, CA 90007, U.S.A.
Abstract:The expressions for “survival” probabilities are presented for an atomic hydrogen particle moving on a trajectory from far regions of the heliosphere to the vicinity of the Sun. Three “destroying” processes have been considered; photoionization, charge transfer and electron ionization. The solar wind has been assumed to be a two-flux steady stream radially expanding with constant flow velocity. Recent profiles of solar-wind electron temperature have been used. The results can be useful for theoretical analyses as well as for analysis of spaceflight observations.
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