Gyrosynchrotron process of a rare large type-IV μ burst associated with coronal mass ejection.

Details Gyrosynchrotron process of a rare large type-IV μ burst associated with coronal mass ejection. Gyrosynchrotron process of a rare large type-IV μ burst associated with coronal mass ejection.

Dec 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999pyuno....s.451j&link_type=abstract

Publications of the Yunnan Observatory, Suppl. 1999, p. 451 - 455

Physics

Solar Microwave Bursts: Energetic Particles

Scientific paper

A large type IV μ solar radio burst was observed at Yunnan Observatory on December 16, 1988. The burst was associated by a coronal mass ejection (CME) with the radio signature of type II and type IV bursts. On the basis of Beijing Huairou magnetogram of AR 5278, power-law distribution of electrons of the source region is calculated. It is suggested that the type IV μ burst associated with CME was due to the gyrosynchrotron radiation of high energy electrons trapped by magnetic field.

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