Astronomy and Astrophysics – Astronomy
Scientific paper
Apr 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982soph...77..249s&link_type=abstract
Solar Physics, vol. 77, Apr. 1982, p. 249-254.
Astronomy and Astrophysics
Astronomy
3
Collisionless Plasmas, Magnetic Field Configurations, Shock Wave Propagation, Solar Magnetic Field, Solar Radio Bursts, Type 2 Bursts, Electron Acceleration, Plasma Waves, Shock Wave Generators, Spaceborne Astronomy
Scientific paper
An excellent example of a type III-V burst followed by a type II burst with fundamental and harmonic bands was observed on June 18, 1979 at the Clark Lake Radio Observatory. The observations are described in detail and their implications are discussed with regard to the problem of directionality with respect to the magnetic field lines of the collisionless MHD shock wave generated at the start of the flash phase. It is found that the positions of type III and type II (F) bursts at a number of frequencies are essentially the same, which implies that the shock responsible for the type II radiation follows the path of the type III exciter, that is, the shock propagates along the open field lines.
Gergely Tomas E.
Kundu Mukul R.
Sawant Hanumant S.
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