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: | , , |
| Format: | Artikel |
| Sprache: | English |
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Головна астрономічна обсерваторія НАН України
2012
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| 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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Glubokova, S.K. Chashei, I.V. Tyul'bashev, S.A. 2017-06-04T19:41:01Z 2017-06-04T19:41:01Z 2012 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 https://nasplib.isofts.kiev.ua/handle/123456789/119192 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. 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. en Головна астрономічна обсерваторія НАН України Advances in Astronomy and Space Physics Small-scale solar wind density turbulence spectrum from interplanetary scintillation observations Article published earlier |
| institution |
Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| collection |
DSpace DC |
| title |
Small-scale solar wind density turbulence spectrum from interplanetary scintillation observations |
| spellingShingle |
Small-scale solar wind density turbulence spectrum from interplanetary scintillation observations Glubokova, S.K. Chashei, I.V. Tyul'bashev, S.A. |
| 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 |
| author |
Glubokova, S.K. Chashei, I.V. Tyul'bashev, S.A. |
| author_facet |
Glubokova, S.K. Chashei, I.V. Tyul'bashev, S.A. |
| publishDate |
2012 |
| language |
English |
| container_title |
Advances in Astronomy and Space Physics |
| publisher |
Головна астрономічна обсерваторія НАН України |
| format |
Article |
| 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.
|
| issn |
2227-1481 |
| url |
https://nasplib.isofts.kiev.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. |
| work_keys_str_mv |
AT glubokovask smallscalesolarwinddensityturbulencespectrumfrominterplanetaryscintillationobservations AT chasheiiv smallscalesolarwinddensityturbulencespectrumfrominterplanetaryscintillationobservations AT tyulbashevsa smallscalesolarwinddensityturbulencespectrumfrominterplanetaryscintillationobservations |
| first_indexed |
2025-12-07T18:44:35Z |
| last_indexed |
2025-12-07T18:44:35Z |
| _version_ |
1850876179824771072 |