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Volumn 474, Issue 2 PART I, 1997, Pages 782-789

Three-dimensional simulation study of the magnetohydrodynamic relaxation process in the solar corona. II

Author keywords

Methods: numerical; MHD; Sun: corona; Sun: flares; Sun: magnetic field

Indexed keywords


EID: 21444438538     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/303495     Document Type: Article
Times cited : (4)

References (26)
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    • Hudson, H. 1994, in Proc. Kofu Symposium, New Look at the Sun with Emphasis on Advanced Observations of Coronal Dynamics and Flares, ed. S. Enome & T. Hirayama (NRO Rep. 360), 1
    • (1994) Proc. Kofu Symposium , pp. 1
    • Hudson, H.1
  • 17
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    • Magnetodynamic Phenomena in the Solar Atmosphere, ed. Y. Uchida, T. Kosugi, & S. Hudson (Dordrecht: Kluwer), in press
    • Ohyama, M., & Shibata, K. 1996, in IAU Colloq. 153, Magnetodynamic Phenomena in the Solar Atmosphere, ed. Y. Uchida, T. Kosugi, & S. Hudson (Dordrecht: Kluwer), in press
    • (1996) IAU Colloq. , vol.153
    • Ohyama, M.1    Shibata, K.2
  • 25
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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.