Optical output of the 24 April 1984 white-light flare

Details Optical output of the 24 April 1984 white-light flare Optical output of the 24 April 1984 white-light flare

Nov 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994soph..155..199n&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 155, no.1, p. 199-202

Physics

5

Light Emission, Photometry, Solar Flares, Visible Spectrum, Balmer Series, Light Curve, Power Spectra, Solar X-Rays, Spectrum Analysis

Scientific paper

Results of quantitative, two-dimensional photographic photometry of the spectacular 24 April 1984 white-light flare (WLF) are presented, including measurements of optical continuum peak flux, spectrum, and power. The WLF light curve peaks nearly simultaneously with the flare hard x-rays, but precedes the peak soft x-ray thermal emission by several minutes.

Affiliated with

Also associated with

No associations

Rating

Optical output of the 24 April 1984 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 Optical output of the 24 April 1984 white-light flare, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Optical output of the 24 April 1984 white-light flare will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-950482