A two-component model of variations of Lyman-alpha emission with solar-activity level

Details A two-component model of variations of Lyman-alpha emission with solar-activity level A two-component model of variations of Lyman-alpha emission with solar-activity level

Feb 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ge%26ae..31...40k&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 31, Jan.-Feb. 1991, p. 40-45. In Russian.

Computer Science

2

Emission Spectra, Lyman Alpha Radiation, Solar Activity, Solar Radiation, Ultraviolet Radiation, Solar Cycles, Solar Mesosphere Explorer, Spectral Line Width, Stellar Models

Scientific paper

The relationship between the intensity of solar UV radiation in the Lyman-alpha line and the 10.7-cm emission is analyzed on the basis of SME data for 1982-1988. It is shown that the closest correlation between these parameters corresponds to the hypothesis that the Lyman-alpha radiation is a superposition of two components: background and upwelling from active regions. It is pointed out that various characteristics of Lyman-alpha variations in an activity cycle can be explained with the two-component model.

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