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Radio Physics and Radio Astronomy

Erscheint 4 Ausgaben pro Jahr

ISSN Druckformat: 2152-274X

ISSN Online: 2152-2758

POLARIZATION OF DRIFTING PAIRS AT DECAMETER WAVES

Volumen 1, Ausgabe 2, 2010, pp. 107-110
DOI: 10.1615/RadioPhysicsRadioAstronomy.v1.i2.30
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ABSTRAKT

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.

REFERENZIERT VON
  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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