Hard X-ray emission in the solar flares of 2 and 11 August 1972

Details Hard X-ray emission in the solar flares of 2 and 11 August 1972 Hard X-ray emission in the solar flares of 2 and 11 August 1972

Nov 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977kosis..15..895k&link_type=abstract

Kosmicheskie Issledovaniia, vol. 15, Nov.-Dec. 1977, p. 895-900. In Russian.

Astronomy and Astrophysics

Astronomy

Microwave Emission, Radio Astronomy, Solar Flares, Solar X-Rays, Electron Emission, Plasma Density, Radiative Lifetime, Radio Spectroscopy, Time Dependence

Scientific paper

Consideration is given to the basic characteristics of X-ray and microwave emission in the solar flare events of 2 and 11 August 1972. Time dependencies of X-ray intensities are studied for the energy ranges 4-9.6, 35-52, 52-102, 102-202, and 202-287 keV and of microwave intensities at 9400 MHz are investigated. Information is obtained on plasma density from radio spectrum analysis. A number of solar flare parameters are examined, including plasma density, electron emission values, X-ray burst duration, and electron lifetime.

Affiliated with

Also associated with

No associations

Rating

Hard X-ray emission in the solar flares of 2 and 11 August 1972 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 Hard X-ray emission in the solar flares of 2 and 11 August 1972, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Hard X-ray emission in the solar flares of 2 and 11 August 1972 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1132493