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无线电物理和天文学期刊

每年出版 4 

ISSN 打印: 2152-274X

ISSN 在线: 2152-2758

POLARIZATION OF DRIFTING PAIRS AT DECAMETER WAVES

卷 1, 册 2, 2010, pp. 107-110
DOI: 10.1615/RadioPhysicsRadioAstronomy.v1.i2.30
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摘要

Observation data on polarization of solar "drift pair" bursts (DP) are shown. All bursts were recorded during Type III storm on 12-18 July, 2002 with the URAN-2 radio telescope. Over 300 DPs are analyzed. The DP polarization is found to depend on the position of a DP-related active region on the solar disk. The average polarization degree of both "forward" and "reverse" DPs makes about 30 %. The investigated time profile of polarization degree shows substantial difference for those "forward" and "reverse" DPs.

对本文的引用
  1. Stanislavsky A. A., Konovalenko A. A., Yerin S. N., Bubnov I. N., Zakharenko V. V., Shkuratov Yu. G., Tokarsky P. L., Yatskiv Ya. S., Brazhenko A. I., Frantsuzenko A. V., Dorovskyy V. V., Rucker H. O., Zarka Ph., Solar bursts as can be observed from the lunar farside with a single antenna at very low frequencies, Astronomische Nachrichten, 339, 7-8, 2018. Crossref

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