Radio observations of interplanetary magnetic field structures out of the ecliptic

Details Radio observations of interplanetary magnetic field structures out of the ecliptic Radio observations of interplanetary magnetic field structures out of the ecliptic

Nov 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976stin...7711947f&link_type=abstract

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Computer Science

Bearing (Direction), Interplanetary Magnetic Fields, Solar Orbits, Solar Radio Bursts, Explorer 43 Satellite, Explorer 49 Satellite, Magnetic Measurement, Type 3 Bursts

Scientific paper

New observations of the out-of-the ecliptic trajectories of type 3 solar radio bursts have been obtained from simultaneous direction finding measurements on two independent satellite experiments, IMP-6 with spin plane in the ecliptic, and RAE-2 with spin plane normal to the ecliptic. Burst exciter trajectories were observed which originated at the active region and then crossed the ecliptic plane at about 0.8 AU. A considerable large scale north-south component of the interplanetary magnetic field is followed by the exciters. The apparent north-south and east-west angular source sizes observed by the two spacecraft are approximately equal, and range from 25 deg at 600 KHz to 110 deg at 80 KHz.

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