Astronomy and Astrophysics – Astronomy
Scientific paper
Feb 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990soph..125..371r&link_type=abstract
Solar Physics (ISSN 0038-0938), vol. 125, Feb. 1990, p. 371-388.
Astronomy and Astrophysics
Astronomy
12
Kilometric Waves, Radio Sources (Astronomy), Type 3 Bursts, Interplanetary Magnetic Fields, Solar Limb, Spaceborne Astronomy
Scientific paper
The radio azimuths for many kilometric type III bursts that originate near or behind the limb of the sun are observed to drift far to the east or far to the west of the spacecraft-sun line. It is shown that the behavior of the observed burst parameters for these events corresponds to the response of a spinning dipole antenna to halolike sources of radiation around the sun. These results provide evidence for a previous suggestion that behind-the-limb type III events should appear as halolike sources of radiation to an observer on the opposite side of the sun, due to scattering of the radiation from the primary source back around the sun.
Reiner M. J.
Stone Robert G.
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