Abstract
The projected source positions at 43, 80, and 160 MHz and the sense and degree of circular polarization in the range 24 to 220 MHz, as observed with the Culgoora radioheliograph and spectropolarimeter respectively, are used: (1) To substantiate the hypothesis that metric U bursts originate in high coronal, magnetic loops. (2) To strengthen the hypothesis that U-burst radiation is in the ordinary magneto-ionic mode.
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