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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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Головна астрономічна обсерваторія НАН України
2012
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Series: | Advances in Astronomy and Space Physics |
Online Access: | http://dspace.nbuv.gov.ua/handle/123456789/119192 |
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irk-123456789-1191922017-06-05T03:04:02Z Small-scale solar wind density turbulence spectrum from interplanetary scintillation observations Glubokova, S.K. Chashei, I.V. Tyul'bashev, S.A. 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. 2012 Article 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. 2227-1481 http://dspace.nbuv.gov.ua/handle/123456789/119192 en Advances in Astronomy and Space Physics Головна астрономічна обсерваторія НАН України |
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Digital Library of Periodicals of National Academy of Sciences of Ukraine |
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DSpace DC |
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English |
description |
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. |
format |
Article |
author |
Glubokova, S.K. Chashei, I.V. Tyul'bashev, S.A. |
spellingShingle |
Glubokova, S.K. Chashei, I.V. Tyul'bashev, S.A. Small-scale solar wind density turbulence spectrum from interplanetary scintillation observations Advances in Astronomy and Space Physics |
author_facet |
Glubokova, S.K. Chashei, I.V. Tyul'bashev, S.A. |
author_sort |
Glubokova, S.K. |
title |
Small-scale solar wind density turbulence spectrum from interplanetary scintillation observations |
title_short |
Small-scale solar wind density turbulence spectrum from interplanetary scintillation observations |
title_full |
Small-scale solar wind density turbulence spectrum from interplanetary scintillation observations |
title_fullStr |
Small-scale solar wind density turbulence spectrum from interplanetary scintillation observations |
title_full_unstemmed |
Small-scale solar wind density turbulence spectrum from interplanetary scintillation observations |
title_sort |
small-scale solar wind density turbulence spectrum from interplanetary scintillation observations |
publisher |
Головна астрономічна обсерваторія НАН України |
publishDate |
2012 |
url |
http://dspace.nbuv.gov.ua/handle/123456789/119192 |
citation_txt |
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. |
series |
Advances in Astronomy and Space Physics |
work_keys_str_mv |
AT glubokovask smallscalesolarwinddensityturbulencespectrumfrominterplanetaryscintillationobservations AT chasheiiv smallscalesolarwinddensityturbulencespectrumfrominterplanetaryscintillationobservations AT tyulbashevsa smallscalesolarwinddensityturbulencespectrumfrominterplanetaryscintillationobservations |
first_indexed |
2023-10-18T20:33:58Z |
last_indexed |
2023-10-18T20:33:58Z |
_version_ |
1796150534522011648 |