Computer Science
Scientific paper
Oct 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ge%26ae..34...86k&link_type=abstract
Geomagn. Aehron., Tom 34, No. 5, p. 86 - 90
Computer Science
Scientific paper
Hβ emission in aurora is calculated by simplified model based on results of precise Monte-Carlo simulation of proton-hydrogen atom (p-H) transport in the atmosphere. Comparisons with rocket measurements and with simultaneous satellite and groundbased observations were made. It was found that both altitude profile of emission rate and spatial distribution of column emission rate observed from the ground agree well with values calculated by measured downgoing proton flux.
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