Small-scale solar wind density turbulence spectrum from interplanetary scintillation observations

The method of determining the angular sizes of compact radio sources and parameters of the plasma turbulence using temporal scintillation power spectra is described and tested. The observations were carried out with the radio telescope BSA of Lebedev Physical Institute at the frequency 111 MHz. Esti...

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Veröffentlicht in:Advances in Astronomy and Space Physics
Datum:2012
Hauptverfasser: Glubokova, S.K., Chashei, I.V., Tyul'bashev, S.A.
Format: Artikel
Sprache:English
Veröffentlicht: Головна астрономічна обсерваторія НАН України 2012
Online Zugang:https://nasplib.isofts.kiev.ua/handle/123456789/119192
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Назва журналу:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Zitieren:Small-scale solar wind density turbulence spectrum from interplanetary scintillation observations / S.K. Glubokova, I.V. Chashei, S.A. Tyul'bashev // Advances in Astronomy and Space Physics. — 2012. — Т. 2., вип. 2. — С. 164-166. — Бібліогр.: 12 назв. — англ.

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