The dependence of solar hard X-ray burst intensity on magnetic field strength

Details The dependence of solar hard X-ray burst intensity on magnetic field strength The dependence of solar hard X-ray burst intensity on magnetic field strength

Aug 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986soph..106..411p&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 106, Aug. 1986, p. 411-413.

Physics

1

Magnetic Flux, Solar Flares, Solar Magnetic Field, Solar Radio Bursts, Solar X-Rays, Electron Energy, Gyrofrequency, Magnetic Effects, Microwave Emission, Plasma Frequencies

Scientific paper

The measurements of peak intensities of hard X-ray bursts from hot flare plasma electrons as a function of peak frequency of associated microwave radio bursts are discussed. The latter is proportional to the magnetic field strength. The results suggest that the flare hard X-rays are emitted when the electron plasma frequency is comparable to the electron gyrofrequency. Thus, the hard X-ray peak intensity varies as B4.2, where B is the magnetic field strength.

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