Physics
Scientific paper
Aug 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980p%26ss...28..815k&link_type=abstract
Planetary and Space Science, vol. 28, Aug. 1980, p. 815-821.
Physics
Gas Ionization, Hydrogen Ions, Interplanetary Gas, Interstellar Gas, Charge Transfer, Photoionization, Solar Protons, Solar Wind
Scientific paper
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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