Magnetohydrodynamic simulation of the interaction between two interplanetary magnetic clouds and its consequent geoeffectiveness: 2. Oblique collision
- Author
- MING XIONG1 ; HUINAN ZHENG1 ; SHUI WANG1
[1] Chinese Academy of Sciences Key Laboratory for Basic Plasma Physics, School of Earth and Space Sciences, University of Science and Technology of China, Hefei, China - Source
Journal of geophysical research. 2009, Vol 114, Num A11 ; A11101.1-A11101.14 ; ref : 1 p.1/4
- ISSN
- 0148-0227
- Scientific domain
- Astronomy earth cosmic environment; Geology; Geophysics; Climatology, meteorology; Oceanography
- Publisher
- American Geophysical Union, Washington, DC
- Publication country
- United States
- Document type
- Article
- Language
- English
- Keyword (fr)
- Compression Couplage Cours eau Déflexion Ejection masse coronale Elasticité Eruption Espace interplanétaire Front choc Hélicité Héliosphère Latitude Magnétohydrodynamique Modèle MHD Nuage magnétique Orientation Propagation Simulation numérique Système convectif mésoéchelle Tampon
- Keyword (en)
- compression coupling streams Deflection Coronal mass ejection elasticity eruptions interplanetary space Shock front Helicity Heliosphere latitude magnetohydrodynamics MHD model Magnetic cloud orientation propagation digital simulation Mesoscale convective system buffers
- Keyword (es)
- Compresión Curso agua Deflección Eyección masa coronal Elasticidad Erupción Helicidad Heliosfera Magnetohidrodinámica Modelo MHD Nube magnetica Orientación Propagación Simulación numérica Sistema convectiva mesoescala Tampón
- Classification
- Discipline
- Earth sciences
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 22323684
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:150:\"Magnetohydrodynamic simulation of the interaction between two interplanetary magnetic clouds and its consequent geoeffectiveness: 2. Oblique collision\";s:9:\"\u0000*\u0000jtitle\";s:31:\"Journal of geophysical research\";s:9:\"\u0000*\u0000stitle\";s:15:\"J. geophys. res\";s:7:\"\u0000*\u0000date\";s:4:\"2009\";s:9:\"\u0000*\u0000volume\";s:3:\"114\";s:8:\"\u0000*\u0000issue\";s:3:\"A11\";s:8:\"\u0000*\u0000spage\";s:0:\"\";s:8:\"\u0000*\u0000epage\";s:0:\"\";s:8:\"\u0000*\u0000pages\";s:18:\"A11101.1-A11101.14\";s:7:\"\u0000*\u0000issn\";s:9:\"0148-0227\";s:8:\"\u0000*\u0000eissn\";s:0:\"\";s:9:\"\u0000*\u0000aulast\";s:10:\"MING XIONG\";s:10:\"\u0000*\u0000aufirst\";s:0:\"\";s:9:\"\u0000*\u0000auinit\";s:0:\"\";s:10:\"\u0000*\u0000auinitm\";s:0:\"\";s:5:\"\u0000*\u0000au\";a:2:{i:0;s:12:\"HUINAN ZHENG\";i:1;s:9:\"SHUI WANG\";}s:9:\"\u0000*\u0000aucorp\";s:0:\"\";s:7:\"\u0000*\u0000isbn\";s:0:\"\";s:8:\"\u0000*\u0000coden\";s:0:\"\";s:8:\"\u0000*\u0000genre\";s:7:\"article\";s:7:\"\u0000*\u0000part\";s:0:\"\";s:9:\"\u0000*\u0000btitle\";s:0:\"\";s:8:\"\u0000*\u0000title\";s:150:\"Magnetohydrodynamic simulation of the interaction between two interplanetary magnetic clouds and its consequent geoeffectiveness: 2. Oblique collision\";s:8:\"\u0000*\u0000place\";s:14:\"Washington, DC\";s:6:\"\u0000*\u0000pub\";s:26:\"American Geophysical Union\";s:10:\"\u0000*\u0000edition\";s:0:\"\";s:9:\"\u0000*\u0000tpages\";s:0:\"\";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:150:\"Magnetohydrodynamic simulation of the interaction between two interplanetary magnetic clouds and its consequent geoeffectiveness: 2. Oblique collision\";s:9:\"\u0000*\u0000jtitle\";s:31:\"Journal of geophysical research\";s:9:\"\u0000*\u0000stitle\";s:15:\"J. geophys. res\";s:7:\"\u0000*\u0000date\";s:4:\"2009\";s:9:\"\u0000*\u0000volume\";s:3:\"114\";s:8:\"\u0000*\u0000issue\";s:3:\"A11\";s:8:\"\u0000*\u0000spage\";s:0:\"\";s:8:\"\u0000*\u0000epage\";s:0:\"\";s:8:\"\u0000*\u0000pages\";s:18:\"A11101.1-A11101.14\";s:7:\"\u0000*\u0000issn\";s:9:\"0148-0227\";s:8:\"\u0000*\u0000eissn\";s:0:\"\";s:9:\"\u0000*\u0000aulast\";s:10:\"MING XIONG\";s:10:\"\u0000*\u0000aufirst\";s:0:\"\";s:9:\"\u0000*\u0000auinit\";s:0:\"\";s:10:\"\u0000*\u0000auinitm\";s:0:\"\";s:5:\"\u0000*\u0000au\";a:2:{i:0;s:12:\"HUINAN ZHENG\";i:1;s:9:\"SHUI WANG\";}s:9:\"\u0000*\u0000aucorp\";s:0:\"\";s:7:\"\u0000*\u0000isbn\";s:0:\"\";s:8:\"\u0000*\u0000coden\";s:0:\"\";s:8:\"\u0000*\u0000genre\";s:7:\"article\";s:7:\"\u0000*\u0000part\";s:0:\"\";s:9:\"\u0000*\u0000btitle\";s:0:\"\";s:8:\"\u0000*\u0000title\";s:150:\"Magnetohydrodynamic simulation of the interaction between two interplanetary magnetic clouds and its consequent geoeffectiveness: 2. Oblique collision\";s:8:\"\u0000*\u0000place\";s:14:\"Washington, DC\";s:6:\"\u0000*\u0000pub\";s:26:\"American Geophysical Union\";s:10:\"\u0000*\u0000edition\";s:0:\"\";s:9:\"\u0000*\u0000tpages\";s:0:\"\";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:150:\"Magnetohydrodynamic simulation of the interaction between two interplanetary magnetic clouds and its consequent geoeffectiveness: 2. Oblique collision\";s:9:\"\u0000*\u0000jtitle\";s:31:\"Journal of geophysical research\";s:9:\"\u0000*\u0000stitle\";s:15:\"J. geophys. res\";s:7:\"\u0000*\u0000date\";s:4:\"2009\";s:9:\"\u0000*\u0000volume\";s:3:\"114\";s:8:\"\u0000*\u0000issue\";s:3:\"A11\";s:8:\"\u0000*\u0000spage\";s:0:\"\";s:8:\"\u0000*\u0000epage\";s:0:\"\";s:8:\"\u0000*\u0000pages\";s:18:\"A11101.1-A11101.14\";s:7:\"\u0000*\u0000issn\";s:9:\"0148-0227\";s:8:\"\u0000*\u0000eissn\";s:0:\"\";s:9:\"\u0000*\u0000aulast\";s:10:\"MING XIONG\";s:10:\"\u0000*\u0000aufirst\";s:0:\"\";s:9:\"\u0000*\u0000auinit\";s:0:\"\";s:10:\"\u0000*\u0000auinitm\";s:0:\"\";s:5:\"\u0000*\u0000au\";a:2:{i:0;s:12:\"HUINAN ZHENG\";i:1;s:9:\"SHUI WANG\";}s:9:\"\u0000*\u0000aucorp\";s:0:\"\";s:7:\"\u0000*\u0000isbn\";s:0:\"\";s:8:\"\u0000*\u0000coden\";s:0:\"\";s:8:\"\u0000*\u0000genre\";s:7:\"article\";s:7:\"\u0000*\u0000part\";s:0:\"\";s:9:\"\u0000*\u0000btitle\";s:0:\"\";s:8:\"\u0000*\u0000title\";s:150:\"Magnetohydrodynamic simulation of the interaction between two interplanetary magnetic clouds and its consequent geoeffectiveness: 2. Oblique collision\";s:8:\"\u0000*\u0000place\";s:14:\"Washington, DC\";s:6:\"\u0000*\u0000pub\";s:26:\"American Geophysical Union\";s:10:\"\u0000*\u0000edition\";s:0:\"\";s:9:\"\u0000*\u0000tpages\";s:0:\"\";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:150:\"Magnetohydrodynamic simulation of the interaction between two interplanetary magnetic clouds and its consequent geoeffectiveness: 2. Oblique collision\";s:9:\"\u0000*\u0000jtitle\";s:31:\"Journal of geophysical research\";s:9:\"\u0000*\u0000stitle\";s:15:\"J. geophys. res\";s:7:\"\u0000*\u0000date\";s:4:\"2009\";s:9:\"\u0000*\u0000volume\";s:3:\"114\";s:8:\"\u0000*\u0000issue\";s:3:\"A11\";s:8:\"\u0000*\u0000spage\";s:0:\"\";s:8:\"\u0000*\u0000epage\";s:0:\"\";s:8:\"\u0000*\u0000pages\";s:18:\"A11101.1-A11101.14\";s:7:\"\u0000*\u0000issn\";s:9:\"0148-0227\";s:8:\"\u0000*\u0000eissn\";s:0:\"\";s:9:\"\u0000*\u0000aulast\";s:10:\"MING XIONG\";s:10:\"\u0000*\u0000aufirst\";s:0:\"\";s:9:\"\u0000*\u0000auinit\";s:0:\"\";s:10:\"\u0000*\u0000auinitm\";s:0:\"\";s:5:\"\u0000*\u0000au\";a:2:{i:0;s:12:\"HUINAN ZHENG\";i:1;s:9:\"SHUI WANG\";}s:9:\"\u0000*\u0000aucorp\";s:0:\"\";s:7:\"\u0000*\u0000isbn\";s:0:\"\";s:8:\"\u0000*\u0000coden\";s:0:\"\";s:8:\"\u0000*\u0000genre\";s:7:\"article\";s:7:\"\u0000*\u0000part\";s:0:\"\";s:9:\"\u0000*\u0000btitle\";s:0:\"\";s:8:\"\u0000*\u0000title\";s:150:\"Magnetohydrodynamic simulation of the interaction between two interplanetary magnetic clouds and its consequent geoeffectiveness: 2. Oblique collision\";s:8:\"\u0000*\u0000place\";s:14:\"Washington, DC\";s:6:\"\u0000*\u0000pub\";s:26:\"American Geophysical Union\";s:10:\"\u0000*\u0000edition\";s:0:\"\";s:9:\"\u0000*\u0000tpages\";s:0:\"\";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:150:\"Magnetohydrodynamic simulation of the interaction between two interplanetary magnetic clouds and its consequent geoeffectiveness: 2. Oblique collision\";s:9:\"\u0000*\u0000jtitle\";s:31:\"Journal of geophysical research\";s:9:\"\u0000*\u0000stitle\";s:15:\"J. geophys. res\";s:7:\"\u0000*\u0000date\";s:4:\"2009\";s:9:\"\u0000*\u0000volume\";s:3:\"114\";s:8:\"\u0000*\u0000issue\";s:3:\"A11\";s:8:\"\u0000*\u0000spage\";s:0:\"\";s:8:\"\u0000*\u0000epage\";s:0:\"\";s:8:\"\u0000*\u0000pages\";s:18:\"A11101.1-A11101.14\";s:7:\"\u0000*\u0000issn\";s:9:\"0148-0227\";s:8:\"\u0000*\u0000eissn\";s:0:\"\";s:9:\"\u0000*\u0000aulast\";s:10:\"MING XIONG\";s:10:\"\u0000*\u0000aufirst\";s:0:\"\";s:9:\"\u0000*\u0000auinit\";s:0:\"\";s:10:\"\u0000*\u0000auinitm\";s:0:\"\";s:5:\"\u0000*\u0000au\";a:2:{i:0;s:12:\"HUINAN ZHENG\";i:1;s:9:\"SHUI WANG\";}s:9:\"\u0000*\u0000aucorp\";s:0:\"\";s:7:\"\u0000*\u0000isbn\";s:0:\"\";s:8:\"\u0000*\u0000coden\";s:0:\"\";s:8:\"\u0000*\u0000genre\";s:7:\"article\";s:7:\"\u0000*\u0000part\";s:0:\"\";s:9:\"\u0000*\u0000btitle\";s:0:\"\";s:8:\"\u0000*\u0000title\";s:150:\"Magnetohydrodynamic simulation of the interaction between two interplanetary magnetic clouds and its consequent geoeffectiveness: 2. Oblique collision\";s:8:\"\u0000*\u0000place\";s:14:\"Washington, DC\";s:6:\"\u0000*\u0000pub\";s:26:\"American Geophysical Union\";s:10:\"\u0000*\u0000edition\";s:0:\"\";s:9:\"\u0000*\u0000tpages\";s:0:\"\";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
