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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

INVESTIGATION OF LARGE-SCALE STRUCTURE OF SOLAR WIND AT SPATIALLY SEPARATED RADIOTELESCOPES

巻 3, 発行 2, 2012, pp. 113-122
DOI: 10.1615/RadioPhysicsRadioAstronomy.v3.i2.30
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要約

Expressions for the second and fourth field moments which account for the solar wind flow structure are obtained with the Feynman path-integrals method. The expressions for scintillations of power spectra for the radiation received by a single antenna and by two spatially separated antennas are obtained and analyzed. For different solar wind models it was shown that the method of the dispersion analysis of phase speed, along with the scintillation method, allows to most fully investigate the solar wind flow structure at distances from the Sun exceeding 1 AU. This method enables to define not only the presence of solar wind flows of various speeds but also their extent and parameters.

によって引用された
  1. Olyak M.R., Large-scale structure of solar wind and geomagnetic phenomena, Journal of Atmospheric and Solar-Terrestrial Physics, 86, 2012. Crossref

  2. Ulyanov O. M., Skoryk A. O., Shevtsova A. I., Plakhov M. S., Ulyanova O. O., Detection of the fine structure of the pulsar J0953+0755 radio emission in the decametre wave range, Monthly Notices of the Royal Astronomical Society, 455, 1, 2016. Crossref

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