Radiation signatures from a locally energized flaring loop

Details Radiation signatures from a locally energized flaring loop Radiation signatures from a locally energized flaring loop

Nov 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...242..359e&link_type=abstract

Astrophysical Journal, Part 1, vol. 242, Nov. 15, 1980, p. 359-373.

Astronomy and Astrophysics

Astrophysics

65

Coronal Loops, High Energy Electrons, Magnetohydrodynamic Flow, Solar Flares, Astronomical Models, Chromosphere, Extreme Ultraviolet Radiation, Solar Corpuscular Radiation, Solar X-Rays

Scientific paper

The radiation signatures from a locally energized solar flare loop based on the physical properties of the energy release mechanisms were consistent with hard X-ray, microwave, and EUV observations for plausible source parameters. It was found that a suprathermal tail of high energy electrons is produced by the primary energy release, and that the number of energetic charged particles ejected into the interplanetary medium in the model is consistent with observations. The radiation signature model predicts that the intrinsic polarization of the hard X-ray burst should increase over the photon energy range of 20 to 100 keV.

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