Solar microwave burst emission relation to X-ray radiation.

Details Solar microwave burst emission relation to X-ray radiation. Solar microwave burst emission relation to X-ray radiation.

Oct 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996a%26a...314..947p&link_type=abstract

Astronomy and Astrophysics, v.314, p.947-956

Astronomy and Astrophysics

Astrophysics

8

Sun: Flares, Sun: Radio Radiation, Sun: X-Rays

Scientific paper

We have calculated the thermal bremsstrahlung component for 87 microwave bursts observed at a near-millimeter wavelength (37GHz), using a well-known procedure for computing the plasma temperature and emission measure from the GOES soft X-ray data. The calculated values showed good correlation with the observed fluxes in gradual rise and fall-type bursts. In the majority of impulsive type bursts a bremsstrahlung component was found to be present, often as a post-burst increase. Some bursts without a thermal component were found and they could be connected with higher energy electrons producing hard X-ray radiation and gyrosynchrotron emission at microwaves. Those microwave bursts that were recorded at hard X-rays during CGRO-BATSE observing times are discussed in more detail.

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