Variation of the full Sun hydrogen Lyman α and β profiles with the activity cycle

Details Variation of the full Sun hydrogen Lyman α and β profiles with the activity cycle Variation of the full Sun hydrogen Lyman α and β profiles with the activity cycle

Jun 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.508..219l&link_type=abstract

In: Proceedings of the SOHO 11 Symposium on From Solar Min to Max: Half a Solar Cycle with SOHO, 11-15 March 2002, Davos, Switze

Computer Science

23

Sun, Chromosphere, Star, Hydrogen

Scientific paper

Full Sun hydrogen Lyman α and β profiles obtained through the activity cycle are needed to compare with stars, to understand the hydrogen distribution in the heliosphere and to evaluate the processes in the upper planetary atmospheres. Using the SUMER/SOHO telesocope scattered light properties, we have measured the Lyman α and β profiles at different epochs of the solar activity cycle. Here we report modifications in the intensity and the shape of the profiles.

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