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

Домашня сторінка
→
Фізико-технічні та математичні науки
→
Відділення фізики і астрономії
→
Advances in Astronomy and Space Physics
→
Advances in Astronomy and Space Physics, 2012, том 2
→
Advances in Astronomy and Space Physics, 2012, вип. 2
→
Переглянути статтю

dc.contributor.author	Glubokova, S.K.
dc.contributor.author	Chashei, I.V.
dc.contributor.author	Tyul'bashev, S.A.
dc.date.accessioned	2017-06-04T19:41:01Z
dc.date.available	2017-06-04T19:41:01Z
dc.date.issued	2012
dc.identifier.citation	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.	uk_UA
dc.identifier.issn	2227-1481
dc.identifier.uri	http://dspace.nbuv.gov.ua/handle/123456789/119192
dc.description.abstract	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. 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.sponsorship	This 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.language.iso	en	uk_UA
dc.publisher	Головна астрономічна обсерваторія НАН України	uk_UA
dc.relation.ispartof	Advances in Astronomy and Space Physics
dc.title	Small-scale solar wind density turbulence spectrum from interplanetary scintillation observations	uk_UA
dc.type	Article	uk_UA
dc.status	published earlier	uk_UA