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

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dc.contributor.authorGlubokova, S.K.
dc.contributor.authorChashei, I.V.
dc.contributor.authorTyul'bashev, S.A.
dc.date.accessioned2017-06-04T19:41:01Z
dc.date.available2017-06-04T19:41:01Z
dc.date.issued2012
dc.description.abstractThe 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. Estimates of the angular size and the turbulence parameters are obtained for the strong scintillating source 3C 48 observed during April-May of 2007-2009. During these periods the interplanetary plasma was comparatively quiet.uk_UA
dc.description.sponsorshipThis work was supported by RFBR Grant 10-02-00078 and Program "Fundamental problems of the solar system study" of the Russian Academy of Sciences.uk_UA
dc.identifier.citationSmall-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.uk_UA
dc.identifier.issn2227-1481
dc.identifier.urihttps://nasplib.isofts.kiev.ua/handle/123456789/119192
dc.language.isoenuk_UA
dc.publisherГоловна астрономічна обсерваторія НАН Україниuk_UA
dc.relation.ispartofAdvances in Astronomy and Space Physics
dc.statuspublished earlieruk_UA
dc.titleSmall-scale solar wind density turbulence spectrum from interplanetary scintillation observationsuk_UA
dc.typeArticleuk_UA

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Advances in Astronomy and Space Physics, 2012, вип. 2