Using L-alpha solar radiation flux for monitoring the spectrum in the EUV region

Details Using L-alpha solar radiation flux for monitoring the spectrum in the EUV region Using L-alpha solar radiation flux for monitoring the spectrum in the EUV region

Aug 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993geoae..33..167k&link_type=abstract

Geomagnetizm i Aehronomiya, vol. 33, p. 167

Physics

Solar Radiation, Far Ultraviolet Radiation, Solar Spectra, Lyman Alpha Radiation, Satellite Observation, Sunspots

Scientific paper

A study is made of the relationship between changes in solar ultraviolet fluxes within 5-nm intervals in the 130-210 nm region, in the L-alpha line, and at 10.7-cm. It is found that changes in the 10.7-cm flux usually precede changes in the EUV region by a day, whereas flux variations in the EUV region and in the L-alpha line are practically cophased. It is also found that L-alpha line flux reflects changes in EUV radiation more accurately than does the 10.7-cm flux.

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