Physics
Scientific paper
Jul 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983jgr....88.5751l&link_type=abstract
Journal of Geophysical Research (ISSN 0148-0227), vol. 88, July 1, 1983, p. 5751-5759. NOAA-supported research.
Physics
54
Chromosphere, Lyman Alpha Radiation, Solar Flux Density, Solar Activity, Solar Cycles, Sunspots, Twenty-Seven Day Variation
Scientific paper
The variability of the Lyman alpha flux during 1969-1980 is calculated using a three-component model of the solar chromosphere, based on ground observations of the Ca II K chromosphere emission. Model predictions show that the Lyman alpha flux increases to as much as 5 x 10 to the 11 photons sq cm/s at the maximum of the solar cycle. The ratio of the average fluxes for December 1979 (cycle maximum) and July 1976 (cycle minimum) is determined to be 1.9. During the solar maximum the 27 day solar rotation is found to cause variations of 5-40 percent in the Lyman alpha flux. It is also shown that the Lyman alpha flux varies over intermediate time periods of 2-3 yr, as well as over the 11 yr sunspot cycle. It is concluded that, unlike the sunspot number and the 10.7 cm radio flux, the Lyman alpha flux had a variability that was approximately the same during each of the past three cycles.
Lean Judith L.
Skumanich Andrew
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