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Radio Physics and Radio Astronomy

年間 4 号発行

ISSN 印刷: 2152-274X

ISSN オンライン: 2152-2758

POLARIZATION OF DRIFTING PAIRS AT DECAMETER WAVES

巻 1, 発行 2, 2010, pp. 107-110
DOI: 10.1615/RadioPhysicsRadioAstronomy.v1.i2.30
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要約

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.

によって引用された
  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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