VLA observations of narrow-band decimetric burst emission

Details VLA observations of narrow-band decimetric burst emission VLA observations of narrow-band decimetric burst emission

Mar 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985soph...96..199w&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 96, March 1985, p. 199-207.

Physics

11

Circular Polarization, Cyclotron Radiation, Decimeter Waves, Masers, Solar Corona, Solar Radio Bursts, Solar X-Rays, Brightness Temperature, Flare Stars, Goes Satellites, Gyrofrequency, Magnetic Poles, Stellar Activity, Very Large Array (Vla)

Scientific paper

The Very Large Array was used to observe a multiply-impulsive solar radio burst at several wavelengths near 20 cm. The observations indicate that the impulsive emission was nearly 100% circularly polarized and originated in small regions of ≡10arcsec - 20arcsec in size. For one of the impulsive spikes, the author finds evidence of narrow-band emission that could be attributed to an electron-cyclotron maser. The radio data are also compared with soft X-ray data and interpreted in light of a model in which the coronal plasma is heated by maser burst emission.

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