On the origin of narrowband and non-drifting microwave bursts

Details On the origin of narrowband and non-drifting microwave bursts On the origin of narrowband and non-drifting microwave bursts

Jun 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001pbeio..37...93y&link_type=abstract

Astrophysics Reports. Publications of the Beijing Astronomical Observatory, No. 37, p. 93 - 98 (2001). In: Proceedings of the Ei

Astronomy and Astrophysics

Astrophysics

Sun, Burst, Fine Structure

Scientific paper

The narrowband non-drifting bursts were observed in Beijing Astronomical Observatory on May 19, 1999 at 1.6-1.9 frequency range. It is proposed two models to explain the main characteristics of these bursts, based on the excitation plasma waves on the front of weak shock waves and based on the amplification of upper hybrid waves under double plasma resonance condition.

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