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The solar ionisation rate deduced from Ulysses measurements and its implications to interplanetary Lyman alpha-intensityWe 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.
Document ID
19960021503
Document Type
Conference Paper
Authors
Summanen, T. (Finnish Meteorological Inst. Helsinki, Finland)
Kyroelae, E. (Finnish Meteorological Inst. Helsinki, Finland)
Date Acquired
August 17, 2013
Publication Date
June 30, 1995
Publication Information
Publication: International Solar Wind 8 Conference
Subject Category
Astrophysics
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.