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Changes in the spectral index of the interplanetary plasma turbulence in the period of low solar activity from observations of strongly scintillating source 3C 298

We present the results of the analysis of temporal power spectra of interplanetary scintillation for the strong radio source 3C 298 observed at 111 MHz with radio telescope BSA LPI in the period near the solar activity minimum. The velocity of the solar wind plasma irregularities and the power expon...

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Bibliographic Details
Main Authors: Glubokova, S.K., Chashei, I.V., Tyul'bashev, S.A., Shishov, V.I.
Format: Article
Language:English
Published: Головна астрономічна обсерваторія НАН України 2013
Series:Advances in Astronomy and Space Physics
Online Access:http://dspace.nbuv.gov.ua/handle/123456789/119619
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