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Radio observations of interplanetary magnetic field structures out of the ecliptic

✍ Scribed by R. J. Fitzenreiter; J. Fainberg; R. R. Weber; H. Alvarez; F. T. Haddock; W. H. Potter

Publisher: Springer
Year: 1977
Tongue: English
Weight: 416 KB
Volume: 52
Category: Article
ISSN: 0038-0938
DOI: 10.1007/bf00149662

No coin nor oath required. For personal study only.

✦ Synopsis

New observations of the out-of-the ecliptic trajectories of type III 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. We find a considerable large scale north-south component of the interplanetary magnetic field 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 ~ at 600 kHz to 110 ~ at 80 kHz.

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