Summary of full-disk solar fluxes between 250 and 1940 A

Details Summary of full-disk solar fluxes between 250 and 1940 A Summary of full-disk solar fluxes between 250 and 1940 A

Aug 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977jgr....82.3307h&link_type=abstract

Journal of Geophysical Research, vol. 82, Aug. 1, 1977, p. 3307-3310.

Physics

25

Chromosphere, Far Ultraviolet Radiation, Radiant Flux Density, Solar Corona, Solar Spectra, Electron Transitions, Line Spectra, Rocket-Borne Instruments, Solar Radio Emission, Ultraviolet Spectrometers

Scientific paper

A summary of full-disk solar fluxes for the wavelength region between 250 and 1940 A is presented which was compiled from data obtained from six rocket spectrometers flown during the period 1969-1976. The intense spectral lines in the wavelength region from 300 to 1220 A are emitted predominantly from the solar chromosphere and the chromosphere-corona transition region. The data indicate that the flux in this wavelength region increases generally by less than 10% with increasing values of the solar 10.7-cm radio-emission flux density from 70 to 177 in units of 10 to the -22nd power W/sq m per Hz.

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