Observations of a post-flare radio burst in X-rays

Details Observations of a post-flare radio burst in X-rays Observations of a post-flare radio burst in X-rays

Jan 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982soph...75..305s&link_type=abstract

Solar Physics, vol. 75, Jan. 1982, p. 305-329. Research supported by the Ministry for Education and Science of the Netherlands,

Astronomy and Astrophysics

Astronomy

95

Coronal Loops, Electron Density (Concentration), Solar Flares, Solar Maximum Mission, Solar Radio Bursts, X Ray Spectroscopy, Astronomical Models, Brightness, Energy Spectra, H Alpha Line, Radio Sources (Astronomy), Thermal Emission

Scientific paper

More than six hours after the two-ribbon flare of May 21, 1980, the hard X-ray spectrometer aboard the SMM imaged an extensive arch above the flare region which was found to be the lowest part of a stationary post-flare noise storm recorded at the same time at Culgoora. The bent crystal spectrometer aboard the SMM confirms that the arch emission was basically thermal. Variations in brightness and energy spectrum at one of the supposed footpoints of the arch are seen as correlation in time with radio brightness, suggesting that suprathermal particles from the radio noise regions dumped in variable quantities onto the low corona and transition layer.

Affiliated with

Also associated with

No associations

Rating

Observations of a post-flare radio burst in X-rays 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 Observations of a post-flare radio burst in X-rays, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Observations of a post-flare radio burst in X-rays will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1458906