Mathematics – Logic
Scientific paper
Jun 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995sowi.conf..107s&link_type=abstract
Finnish Meteorological Inst., International Solar Wind 8 Conference, p. 107
Mathematics
Logic
Computer Programs, Interplanetary Gas, Ionization, Lyman Alpha Radiation, Monte Carlo Method, Solar Cycles, Hydrogen, Solar Activity Effects, Time Dependence, Gas Dynamics
Scientific paper
We have developed a computer code which can be used to study 3-dimensional and time-dependent effects of the solar cycle on the interplanetary (IP) hydrogen distribution. The code is based on the inverted Monte Carlo simulation. In this work we have modelled the temporal behaviour of the solar ionisation rate. We have assumed that during the most of the time of the solar cycle there is an anisotopic latitudinal structure but right at the solar maximum the anisotropy disappears. The effects of this behaviour will be discussed both in regard to the IP hydrogen distribution and IP Lyman a a-intensity.
Kyroelae E.
Summanen Tuula
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