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Volumn 471, Issue 1, 2007, Pages 295-299

Large amplitude oscillatory motion along a solar filament

Author keywords

Magnetohydrodynamics (MHD); Sun: filaments

Indexed keywords

FUNCTION EVALUATION; INVERSE KINEMATICS; MAGNETOHYDRODYNAMICS; PARAMETER ESTIMATION; VELOCITY MEASUREMENT;

EID: 34547960699     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20077668     Document Type: Article
Times cited : (100)

References (31)
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    • Aschwanden, M. J. 2003, in Turbulence, Waves, and Instabilities in the Solar Plasma, ed. R. von Fay-Siebenburgen, K. Petrovay, B. Roberts, & M. J. Aschwanden, NATO Science Ser. (Kluwer Academic Publishers), 215
    • (2003) NATO Science Ser , pp. 215
    • Aschwanden, M.J.1
  • 3
    • 34547942537 scopus 로고    scopus 로고
    • Hyder, C. L. 1966, ZAp, 63, 78
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  • 8
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    • (1978) ApJ , vol.220 , pp. 1133
    • Jockers, K.1
  • 22
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    • Tsubaki, T. 1988, in Solar and Stellar Coronal Structures and Dynamics, ed. R. C. Altrock, National Solar Observatory, 140, Fluid Dynam., 3, 89
    • Tsubaki, T. 1988, in Solar and Stellar Coronal Structures and Dynamics, ed. R. C. Altrock, National Solar Observatory, 140, Fluid Dynam., 3, 89


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.