The polarization of U-shaped solar radio bursts

Details The polarization of U-shaped solar radio bursts The polarization of U-shaped solar radio bursts

Apr 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977a%26a....56..123b&link_type=abstract

Astronomy and Astrophysics, vol. 56, no. 1-2, Apr. 1977, p. 123-127. Research supported by the Swiss National Science Foundatio

Astronomy and Astrophysics

Astrophysics

10

Circular Polarization, Magnetic Field Configurations, Solar Flares, Solar Magnetic Field, Type 3 Bursts, Electromagnetic Wave Transmission, Field Strength, Magnetic Flux, Solar Activity Effects, Sunspots

Scientific paper

Circular-polarization measurements of 11 U-shaped solar radio bursts observed at 237 MHz are reported which contradict the expectation that the received polarization should have different signs in the two branches. The mean polarization of these bursts is found to be about 7% righthanded for the ascending branch and about 6% in the same sense for the descending branch. An attempt is made to discuss the observed constancy of the sign of polarization in terms of coronal propagation properties above the source region.

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