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Volumn 459, Issue 2, 2006, Pages 627-639

Numerical modelling of 3D reconnection II. Comparison between rotational and spinning footpoint motions

Author keywords

Magnetohydrodynamics (MHD); Sun: Activity; Sun: Corona; Sun: Magnetic fields

Indexed keywords

ELECTRONIC STRUCTURE; HEATING; MAGNETIC FIELD EFFECTS; MAGNETIC FLUX; MAGNETOHYDRODYNAMICS; ROTATION;

EID: 33750975916     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20065716     Document Type: Article
Times cited : (30)

References (31)
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    • Green, R. M. 1965, in Solar and Stellar Magnetic Fields, ed. R. Lüst (Amsterdam: North Holland), IAU Symp., 22, 398
    • (1965) IAU Symp. , vol.22 , pp. 398
    • Green, R.M.1
  • 20
    • 0000674588 scopus 로고
    • Parker, E. N. 1972, ApJ, 174, 499
    • (1972) ApJ , vol.174 , pp. 499
    • Parker, E.N.1
  • 23
    • 0000056210 scopus 로고
    • NASA Spec. Publ. SP-50, ed. W. N. Hess
    • Petschek, H. E. 1964, NASA Spec. Publ. SP-50, Physics of Solar Flares, ed. W. N. Hess, 425
    • (1964) Physics of Solar Flares , pp. 425
    • Petschek, H.E.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.