Other
Scientific paper
Nov 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992esasp.348..331s&link_type=abstract
In ESA, Proceedings of the First SOHO Workshop: Coronal Streamers, Coronal Loops, and Coronal and Solar Wind Composition p 331-3
Other
Hydrogen, Interplanetary Gas, Lyman Alpha Radiation, Solar Corpuscular Radiation, Solar Radiation, Density Distribution, Ionization Potentials, Mathematical Models, Prognoz Satellites, Rates (Per Time), Solar Wind
Scientific paper
Four Prognoz-6 Lyman alpha intensity measuring sessions right after the solar minimum were used to study the latitudinal change of the solar ionization rate at 1 AU. The measurements were performed during two and a half months in 1977. The model results, based on the so called thermal model for the interstellar wind and the optically thin model for the scattering process, were compared with the intensity measurements. This comparison resulted in the model for the solar ionization rate at 1 AU. The ionization rates differ from a session to another, but there are two similar characteristics in each session. The common features are the enhanced ionization rate near the heliographic equatorial plane and the broad plateaus of the constant rate around +/- 30 to +/- 70 deg.
Bertaux Jean-Loud
Kyrola Erkki
Lallement Rosine
Summanen Tuula
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