A metric type III burst asymmetry relative to simple bipolar active regions

Details A metric type III burst asymmetry relative to simple bipolar active regions A metric type III burst asymmetry relative to simple bipolar active regions

May 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986soph..105..123j&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 105, May 1986, p. 123-132.

Physics

2

Solar Activity, Type 3 Bursts, Magnetic Field Configurations, Polarization (Waves), Position (Location), Solar Electrons, Solar Magnetic Field

Scientific paper

Metric type III solar radio burst positions are compared spatially and temporally to underlying active region geometry. The positions of these radio bursts have an asymmetric location distribution relative to simple bipolar regions. The type III bursts show a tendency to occur nearer the leading active region - an association shown before from type III burst and magnetic field polarity measurements. The type III bursts also generally occur to the left of the outward to inward directed magnetic field. The asymmetry relative to the outward directed magnetic field has a sense that is consistent with a mechanism of type III burst production that involves a pre-existing coronal current system situated between expanding closed and open magnetic field lines.

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