The propagation effects in the solar corona on visible characteristics of type III radio bursts
- Author
- ITKINA, M. A; YASHNOV, V. A
Nauchno-issled. radiofizicheskij inst., Ussr - Source
Astronomičeskij žurnal. = Russian astronomical journal. 1989, Vol 66, Num 5, pp 1061-1068, 8 p ; ref : 15 ref
- CODEN
- ASZHA2
- ISSN
- 0004-6299
- Scientific domain
- Astronomy earth cosmic environment
- Publisher
- Nauka, Moskva
- Publication country
- Russian Federation
- Document type
- Article
- Language
- Russian
- Keyword (fr)
- Couronne solaire Modèle théorique Propagation onde Simulation numérique Soleil Sursaut solaire type III
- Keyword (en)
- Solar corona Theoretical model Wave propagation Digital simulation Sun Type III burst
- Keyword (es)
- Corona solar Modelo teórico Propagación onda Simulación numérica Sol Arrebato solar tipo III
- Classification
- Pascal
- 001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03B Solar system / 001E03B60 Solar physics / 001E03B60R Flares, bursts, and related phenomena
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 19387444
Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS
Install on your browser
"O:13:\"PanistOpenUrl\":36:{s:10:\"\u0000*\u0000openUrl\";N;s:6:\"\u0000*\u0000idc\";N;s:6:\"\u0000*\u0000fmt\";s:7:\"journal\";s:6:\"\u0000*\u0000doi\";s:0:\"\";s:6:\"\u0000*\u0000pii\";s:0:\"\";s:7:\"\u0000*\u0000pmid\";s:0:\"\";s:9:\"\u0000*\u0000atitle\";s:95:\"The propagation effects in the solar corona on visible characteristics of type III radio bursts\";s:9:\"\u0000*\u0000jtitle\";s:24:\"Astronomi\u010deskij \u017eurnal\";s:9:\"\u0000*\u0000stitle\";s:9:\"Astron. z\";s:7:\"\u0000*\u0000date\";s:4:\"1989\";s:9:\"\u0000*\u0000volume\";s:2:\"66\";s:8:\"\u0000*\u0000issue\";s:1:\"5\";s:8:\"\u0000*\u0000spage\";s:4:\"1061\";s:8:\"\u0000*\u0000epage\";s:4:\"1068\";s:8:\"\u0000*\u0000pages\";s:0:\"\";s:7:\"\u0000*\u0000issn\";s:9:\"0004-6299\";s:8:\"\u0000*\u0000eissn\";s:0:\"\";s:9:\"\u0000*\u0000aulast\";s:6:\"ITKINA\";s:10:\"\u0000*\u0000aufirst\";s:4:\"M. A\";s:9:\"\u0000*\u0000auinit\";s:0:\"\";s:10:\"\u0000*\u0000auinitm\";s:0:\"\";s:5:\"\u0000*\u0000au\";a:1:{i:0;s:13:\"YASHNOV, V. A\";}s:9:\"\u0000*\u0000aucorp\";s:0:\"\";s:7:\"\u0000*\u0000isbn\";s:0:\"\";s:8:\"\u0000*\u0000coden\";s:6:\"ASZHA2\";s:8:\"\u0000*\u0000genre\";s:7:\"article\";s:7:\"\u0000*\u0000part\";s:0:\"\";s:9:\"\u0000*\u0000btitle\";s:0:\"\";s:8:\"\u0000*\u0000title\";s:95:\"The propagation effects in the solar corona on visible characteristics of type III radio bursts\";s:8:\"\u0000*\u0000place\";s:6:\"Moskva\";s:6:\"\u0000*\u0000pub\";s:5:\"Nauka\";s:10:\"\u0000*\u0000edition\";s:0:\"\";s:9:\"\u0000*\u0000tpages\";s:1:\"8\";s:9:\"\u0000*\u0000series\";s:0:\"\";s:8:\"\u0000*\u0000proxy\";s:30:\"http:\/\/proxyout.inist.fr:8080\/\";s:12:\"\u0000*\u0000integrite\";b:1;}"
Panist access
"O:12:\"IstexOpenUrl\":35:{s:10:\"\u0000*\u0000openUrl\";N;s:6:\"\u0000*\u0000fmt\";s:7:\"journal\";s:6:\"\u0000*\u0000doi\";s:0:\"\";s:6:\"\u0000*\u0000pii\";s:0:\"\";s:7:\"\u0000*\u0000pmid\";s:0:\"\";s:9:\"\u0000*\u0000atitle\";s:95:\"The propagation effects in the solar corona on visible characteristics of type III radio bursts\";s:9:\"\u0000*\u0000jtitle\";s:24:\"Astronomi\u010deskij \u017eurnal\";s:9:\"\u0000*\u0000stitle\";s:9:\"Astron. z\";s:7:\"\u0000*\u0000date\";s:4:\"1989\";s:9:\"\u0000*\u0000volume\";s:2:\"66\";s:8:\"\u0000*\u0000issue\";s:1:\"5\";s:8:\"\u0000*\u0000spage\";s:4:\"1061\";s:8:\"\u0000*\u0000epage\";s:4:\"1068\";s:8:\"\u0000*\u0000pages\";s:0:\"\";s:7:\"\u0000*\u0000issn\";s:9:\"0004-6299\";s:8:\"\u0000*\u0000eissn\";s:0:\"\";s:9:\"\u0000*\u0000aulast\";s:6:\"ITKINA\";s:10:\"\u0000*\u0000aufirst\";s:4:\"M. A\";s:9:\"\u0000*\u0000auinit\";s:0:\"\";s:10:\"\u0000*\u0000auinitm\";s:0:\"\";s:5:\"\u0000*\u0000au\";a:1:{i:0;s:13:\"YASHNOV, V. A\";}s:9:\"\u0000*\u0000aucorp\";s:0:\"\";s:7:\"\u0000*\u0000isbn\";s:0:\"\";s:8:\"\u0000*\u0000coden\";s:6:\"ASZHA2\";s:8:\"\u0000*\u0000genre\";s:7:\"article\";s:7:\"\u0000*\u0000part\";s:0:\"\";s:9:\"\u0000*\u0000btitle\";s:0:\"\";s:8:\"\u0000*\u0000title\";s:95:\"The propagation effects in the solar corona on visible characteristics of type III radio bursts\";s:8:\"\u0000*\u0000place\";s:6:\"Moskva\";s:6:\"\u0000*\u0000pub\";s:5:\"Nauka\";s:10:\"\u0000*\u0000edition\";s:0:\"\";s:9:\"\u0000*\u0000tpages\";s:1:\"8\";s:9:\"\u0000*\u0000series\";s:0:\"\";s:8:\"\u0000*\u0000proxy\";s:30:\"http:\/\/proxyout.inist.fr:8080\/\";s:12:\"\u0000*\u0000integrite\";b:1;}"
Istex access
"O:16:\"EuropePMCOpenUrl\":35:{s:10:\"\u0000*\u0000openUrl\";N;s:6:\"\u0000*\u0000fmt\";s:7:\"journal\";s:6:\"\u0000*\u0000doi\";s:0:\"\";s:6:\"\u0000*\u0000pii\";s:0:\"\";s:7:\"\u0000*\u0000pmid\";s:0:\"\";s:9:\"\u0000*\u0000atitle\";s:95:\"The propagation effects in the solar corona on visible characteristics of type III radio bursts\";s:9:\"\u0000*\u0000jtitle\";s:24:\"Astronomi\u010deskij \u017eurnal\";s:9:\"\u0000*\u0000stitle\";s:9:\"Astron. z\";s:7:\"\u0000*\u0000date\";s:4:\"1989\";s:9:\"\u0000*\u0000volume\";s:2:\"66\";s:8:\"\u0000*\u0000issue\";s:1:\"5\";s:8:\"\u0000*\u0000spage\";s:4:\"1061\";s:8:\"\u0000*\u0000epage\";s:4:\"1068\";s:8:\"\u0000*\u0000pages\";s:0:\"\";s:7:\"\u0000*\u0000issn\";s:9:\"0004-6299\";s:8:\"\u0000*\u0000eissn\";s:0:\"\";s:9:\"\u0000*\u0000aulast\";s:6:\"ITKINA\";s:10:\"\u0000*\u0000aufirst\";s:4:\"M. A\";s:9:\"\u0000*\u0000auinit\";s:0:\"\";s:10:\"\u0000*\u0000auinitm\";s:0:\"\";s:5:\"\u0000*\u0000au\";a:1:{i:0;s:13:\"YASHNOV, V. A\";}s:9:\"\u0000*\u0000aucorp\";s:0:\"\";s:7:\"\u0000*\u0000isbn\";s:0:\"\";s:8:\"\u0000*\u0000coden\";s:6:\"ASZHA2\";s:8:\"\u0000*\u0000genre\";s:7:\"article\";s:7:\"\u0000*\u0000part\";s:0:\"\";s:9:\"\u0000*\u0000btitle\";s:0:\"\";s:8:\"\u0000*\u0000title\";s:95:\"The propagation effects in the solar corona on visible characteristics of type III radio bursts\";s:8:\"\u0000*\u0000place\";s:6:\"Moskva\";s:6:\"\u0000*\u0000pub\";s:5:\"Nauka\";s:10:\"\u0000*\u0000edition\";s:0:\"\";s:9:\"\u0000*\u0000tpages\";s:1:\"8\";s:9:\"\u0000*\u0000series\";s:0:\"\";s:8:\"\u0000*\u0000proxy\";s:30:\"http:\/\/proxyout.inist.fr:8080\/\";s:12:\"\u0000*\u0000integrite\";b:1;}"
Europe PubMed Central access
"O:11:\"BaseOpenUrl\":35:{s:10:\"\u0000*\u0000openUrl\";N;s:6:\"\u0000*\u0000fmt\";s:7:\"journal\";s:6:\"\u0000*\u0000doi\";s:0:\"\";s:6:\"\u0000*\u0000pii\";s:0:\"\";s:7:\"\u0000*\u0000pmid\";s:0:\"\";s:9:\"\u0000*\u0000atitle\";s:95:\"The propagation effects in the solar corona on visible characteristics of type III radio bursts\";s:9:\"\u0000*\u0000jtitle\";s:24:\"Astronomi\u010deskij \u017eurnal\";s:9:\"\u0000*\u0000stitle\";s:9:\"Astron. z\";s:7:\"\u0000*\u0000date\";s:4:\"1989\";s:9:\"\u0000*\u0000volume\";s:2:\"66\";s:8:\"\u0000*\u0000issue\";s:1:\"5\";s:8:\"\u0000*\u0000spage\";s:4:\"1061\";s:8:\"\u0000*\u0000epage\";s:4:\"1068\";s:8:\"\u0000*\u0000pages\";s:0:\"\";s:7:\"\u0000*\u0000issn\";s:9:\"0004-6299\";s:8:\"\u0000*\u0000eissn\";s:0:\"\";s:9:\"\u0000*\u0000aulast\";s:6:\"ITKINA\";s:10:\"\u0000*\u0000aufirst\";s:4:\"M. A\";s:9:\"\u0000*\u0000auinit\";s:0:\"\";s:10:\"\u0000*\u0000auinitm\";s:0:\"\";s:5:\"\u0000*\u0000au\";a:1:{i:0;s:13:\"YASHNOV, V. A\";}s:9:\"\u0000*\u0000aucorp\";s:0:\"\";s:7:\"\u0000*\u0000isbn\";s:0:\"\";s:8:\"\u0000*\u0000coden\";s:6:\"ASZHA2\";s:8:\"\u0000*\u0000genre\";s:7:\"article\";s:7:\"\u0000*\u0000part\";s:0:\"\";s:9:\"\u0000*\u0000btitle\";s:0:\"\";s:8:\"\u0000*\u0000title\";s:95:\"The propagation effects in the solar corona on visible characteristics of type III radio bursts\";s:8:\"\u0000*\u0000place\";s:6:\"Moskva\";s:6:\"\u0000*\u0000pub\";s:5:\"Nauka\";s:10:\"\u0000*\u0000edition\";s:0:\"\";s:9:\"\u0000*\u0000tpages\";s:1:\"8\";s:9:\"\u0000*\u0000series\";s:0:\"\";s:8:\"\u0000*\u0000proxy\";s:30:\"http:\/\/proxyout.inist.fr:8080\/\";s:12:\"\u0000*\u0000integrite\";b:1;}"
Base Search access
"O:12:\"ArXivOpenUrl\":35:{s:10:\"\u0000*\u0000openUrl\";N;s:6:\"\u0000*\u0000fmt\";s:7:\"journal\";s:6:\"\u0000*\u0000doi\";s:0:\"\";s:6:\"\u0000*\u0000pii\";s:0:\"\";s:7:\"\u0000*\u0000pmid\";s:0:\"\";s:9:\"\u0000*\u0000atitle\";s:95:\"The propagation effects in the solar corona on visible characteristics of type III radio bursts\";s:9:\"\u0000*\u0000jtitle\";s:24:\"Astronomi\u010deskij \u017eurnal\";s:9:\"\u0000*\u0000stitle\";s:9:\"Astron. z\";s:7:\"\u0000*\u0000date\";s:4:\"1989\";s:9:\"\u0000*\u0000volume\";s:2:\"66\";s:8:\"\u0000*\u0000issue\";s:1:\"5\";s:8:\"\u0000*\u0000spage\";s:4:\"1061\";s:8:\"\u0000*\u0000epage\";s:4:\"1068\";s:8:\"\u0000*\u0000pages\";s:0:\"\";s:7:\"\u0000*\u0000issn\";s:9:\"0004-6299\";s:8:\"\u0000*\u0000eissn\";s:0:\"\";s:9:\"\u0000*\u0000aulast\";s:6:\"ITKINA\";s:10:\"\u0000*\u0000aufirst\";s:4:\"M. A\";s:9:\"\u0000*\u0000auinit\";s:0:\"\";s:10:\"\u0000*\u0000auinitm\";s:0:\"\";s:5:\"\u0000*\u0000au\";a:1:{i:0;s:13:\"YASHNOV, V. A\";}s:9:\"\u0000*\u0000aucorp\";s:0:\"\";s:7:\"\u0000*\u0000isbn\";s:0:\"\";s:8:\"\u0000*\u0000coden\";s:6:\"ASZHA2\";s:8:\"\u0000*\u0000genre\";s:7:\"article\";s:7:\"\u0000*\u0000part\";s:0:\"\";s:9:\"\u0000*\u0000btitle\";s:0:\"\";s:8:\"\u0000*\u0000title\";s:95:\"The propagation effects in the solar corona on visible characteristics of type III radio bursts\";s:8:\"\u0000*\u0000place\";s:6:\"Moskva\";s:6:\"\u0000*\u0000pub\";s:5:\"Nauka\";s:10:\"\u0000*\u0000edition\";s:0:\"\";s:9:\"\u0000*\u0000tpages\";s:1:\"8\";s:9:\"\u0000*\u0000series\";s:0:\"\";s:8:\"\u0000*\u0000proxy\";s:30:\"http:\/\/proxyout.inist.fr:8080\/\";s:12:\"\u0000*\u0000integrite\";b:1;}"
arXiv access
