Microwave, Soft and Hard X-Ray Observations of Solar Flares - a Self-Consistent Model of the Flare Site

Details Microwave, Soft and Hard X-Ray Observations of Solar Flares - a Self-Consistent Model of the Flare Site Microwave, Soft and Hard X-Ray Observations of Solar Flares - a Self-Consistent Model of the Flare Site

Oct 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998soph..182..459c&link_type=abstract

Solar Physics, v. 182, Issue 2, p. 459-476 (1998).

Physics

3

Scientific paper

High-resolution microwave observations of several flares performed with the Westerbork Synthesis Radio Telescope (WRST) on 3 and 4 July 1993 are compared with Yohkoh observations in the soft and hard X-ray domain. Only for one flare, among the six analyzed, was the hard X-ray spectrum between 20 and 200keV available from the Wide Bragg Spectrometer, supplying the energy spectrum of non-thermal particles responsible for this radiation and for the radio emission. A complete model of this flare is derived which accounts for all available observations in the X-ray and radio wavelengths.

Affiliated with

Also associated with

No associations

Rating

Microwave, Soft and Hard X-Ray Observations of Solar Flares - a Self-Consistent Model of the Flare Site 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 Microwave, Soft and Hard X-Ray Observations of Solar Flares - a Self-Consistent Model of the Flare Site, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Microwave, Soft and Hard X-Ray Observations of Solar Flares - a Self-Consistent Model of the Flare Site will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1100906