The X-ray emission of subflares

Details The X-ray emission of subflares The X-ray emission of subflares

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ge%26ae..23..666v&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 23, July-Aug. 1983, p. 666-668. In Russian.

Mathematics

H Alpha Line, Solar Flares, Solar X-Rays, Prognoz Satellites, Solar Spectra, Thermal Radiation

Scientific paper

Optical observations of subflares in the active region Mc Math 14553 in the period 8-15 December, 1976 are compared with the X-ray emission bursts measured during the same period by the X-ray photometer on board the Prognoz-5 automatic observatory. X-ray emissions with energies 2-7 and 6-10 keV are used in the analysis presented here. It is found that energy release in the X-ray emissions is directly proportional to the area of the H-alpha flare events over a wide range of flare intensities, i.e., from subflares to high-power flares of the class 3B.

Affiliated with

Also associated with

No associations

Rating

The X-ray emission of subflares 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 The X-ray emission of subflares, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The X-ray emission of subflares will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-742183