A continuous spectrum of a white-light flare

Details A continuous spectrum of a white-light flare A continuous spectrum of a white-light flare

Sep 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982soph...80..113h&link_type=abstract

Solar Physics, vol. 80, Sept. 1982, p. 113-127.

Physics

35

Atmospheric Heating, Continuous Spectra, Energy Dissipation, Photosphere, Solar Flares, Solar Spectra, Absorption Spectra, Data Reduction, Emission Spectra, Line Spectra, Solar Magnetic Field

Scientific paper

White-light continuum was observed at the Norikura Solar Observatory in a 2B flare of 10 September 1974 in the spectral region between 3600 A and 4000 A. The duration of continuum emission was 8-12 min. The continuum shows a Balmer free-bound component, but the main contribution to the continuum between 3646 A and 4000 A is H(-) emission. The white-light continuum, therefore, is thought to be of photospheric origin. The energy loss in the continuum is 10 to the 27th erg/s.

Affiliated with

Also associated with

No associations

Rating

A continuous spectrum of a white-light flare does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with A continuous spectrum of a white-light flare, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A continuous spectrum of a white-light flare will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1262924