Propagation of type II burst shock waves along the radial magnetic field in the solar corona

Details Propagation of type II burst shock waves along the radial magnetic field in the solar corona Propagation of type II burst shock waves along the radial magnetic field in the solar corona

Mar 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985basi...13...62s&link_type=abstract

Astronomical Society of India, Bulletin, vol. 13, March 1985, p. 62-67.

Astronomy and Astrophysics

Astronomy

1

Coronal Holes, Magnetohydrodynamic Waves, Shock Wave Propagation, Solar Corona, Solar Magnetic Field, Type 2 Bursts, Magnetic Field Configurations, Radial Distribution, Solar Activity

Scientific paper

The authors present an analysis which indicates that in several cases
coronal holes exist in the vicinity of active regions producing type II
bursts. It is inferred that shock waves which produce type II bursts
essentially travel along the coronal magnetic field.

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