The EUV continuum emission /1400-1960 A/ in a solar flare observed from SKYLAB

Details The EUV continuum emission /1400-1960 A/ in a solar flare observed from SKYLAB The EUV continuum emission /1400-1960 A/ in a solar flare observed from SKYLAB

Oct 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978soph...59..361c&link_type=abstract

Solar Physics, vol. 59, Oct. 1978, p. 361-371.

Physics

9

Continuous Spectra, Emission Spectra, Far Ultraviolet Radiation, Solar Flares, Solar Spectra, Ultraviolet Spectra, H Alpha Line, Skylab Program, Solar X-Rays

Scientific paper

The total radiative output in the EUV continuum (1400-1960 A) from the 5 September 1973 flare has been obtained from the EUV spectra of the flare observed with the NRL slit spectrograph (SO82B) on Skylab. The radiative energy in the EUV continuum is of the order of 10 to the 29th ergs, which is more than a factor of 2 greater than those radiated in soft X-rays (8-20 A) and in H-alpha for the flare. Thus, the EUV continuum emission is an important radiative energy loss, and should be included in the consideration of the energy balance of the flare.

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