QUASI-PERIODIC FAST-MODE WAVE TRAINS WITHIN A GLOBAL EUV WAVE AND SEQUENTIAL TRANSVERSE OSCILLATIONS DETECTED BY SDO/AIA
- Author
- WEI LIU1 2 ; OFMAN, Leon3 4 ; NITTA, Nariaki V1 ; ASCHWANDEN, Markus J1 ; SCHRIJVER, Carolus J1 ; TITLE, Alan M1 ; TARBELL, Theodore D1
[1] Lockheed Martin Solar and Astrophysics Laboratory, 3251 Hanover Street, Palo Alto, CA 94304, United States
[2] W. W. Hansen Experimental Physics Laboratory. Stanford University, Stanford. CA 94305, United States
[3] Department of Physics, Catholic University of America, Washingtom, DC 20064, United States
[4] NASA Goddard Space Flight Center, Code 671, Greenbelt, MD 20771, United States - Source
The Astrophysical journal. 2012, Vol 753, Num 1 ; 52.1-52.17 ; 1 ; ref : 3/4 p
- CODEN
- ASJOAB
- ISSN
- 0004-637X
- Scientific domain
- Astronomy earth cosmic environment
- Publisher
- IOP, Bristol
- Publication country
- United Kingdom
- Document type
- Article
- Language
- English
- Author keyword
- Sun: activity Sun: corona Sun: coronal mass ejections (CMEs) Sun: flares Sun: oscillations waves
- Keyword (fr)
- Composante primaire Composante secondaire Corde flux Durée trajet Déflexion Ejection masse coronale Filament Front onde Kink Mode oscillation Onde MHD Pulsation RX Périodicité Reconfiguration Soleil
- Keyword (en)
- Primary component Secondary component Flux rope Travel time Deflection Coronal mass ejection Filaments Wave front Kinks Oscillation modes MHD waves X ray pulsation Periodicity Reconfiguration Sun
- Keyword (es)
- Componente primario Componente secundaria Cuerda flujo Eyección masa coronal Pulsación rayos X Periodicidad Reconfiguración
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 26821737
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
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