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Radio Physics and Radio Astronomy

Publicou 4 edições por ano

ISSN Imprimir: 2152-274X

ISSN On-line: 2152-2758

POLARIZATION OF DRIFTING PAIRS AT DECAMETER WAVES

Volume 1, Edição 2, 2010, pp. 107-110
DOI: 10.1615/RadioPhysicsRadioAstronomy.v1.i2.30
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RESUMO

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.

CITADO POR
  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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