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- W648448358 abstract "Sunmwry: The intensity and polarization of solar radio bursts have been observed at 9400, 3750, 2000 and 1000 Mcj s since July, 1957. In this paper the results of observations dm·ing 6 months are described. In most bursts at microwave frequencies, the difference in the intensity of two circularly polarized components is observed. At 3750 Mc/ s, the bursts of small degree of polarization (less than 10~.,; ) are predominant, compared with other frequencies. At 2000 and 1000 Mc/ s the circularly polarized bursts were occasionally observed, but not at 9400 and 3750 Mc/ s and at 3750 Mc/ s the linearly polarized components were not observed. In most bursts observed at four frequencies, the sense of polarization reverses near 3750 or 2000 Mc/ s and the degree of polarization is generally small at 3750 Mc/ s. At 9400 Mcjs, it seems that the sense of polarization correlates with the position of the source on the solar disk. Further observations wi ll be continued to investigate the r elation between them." @default.
- W648448358 created "2016-06-24" @default.
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- W648448358 date "1958-03-25" @default.
- W648448358 modified "2023-09-23" @default.
- W648448358 title "POLARIZATION OF SOLAR RADIO BURSTS AT MICROWAVE FREQUENCIES I" @default.
- W648448358 hasPublicationYear "1958" @default.
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