메뉴 건너뛰기




Volumn 494, Issue 1 PART II, 1998, Pages

A two-dimensional magnetohydrodynamic simulation of chromospheric evaporation in a solar flare based on a magnetic reconnection model

Author keywords

Conduction; MHD; Plasmas; Sun: flares

Indexed keywords


EID: 25544438679     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/311174     Document Type: Article
Times cited : (147)

References (26)
  • 8
    • 0002032354 scopus 로고
    • Proc. Kofu Symp., New Look at the Sun with Emphasis on Advanced Observations of Coronal Dynamics and Flares, ed. S. Enome & T. Hirayama, Nagano: NRO
    • Hanaoka, Y. 1994, in Proc. Kofu Symp., New Look at the Sun with Emphasis on Advanced Observations of Coronal Dynamics and Flares, ed. S. Enome & T. Hirayama, NRO Rep. 360 (Nagano: NRO), 181
    • (1994) NRO Rep. , vol.360 , pp. 181
    • Hanaoka, Y.1
  • 18
  • 19
    • 0000056210 scopus 로고
    • The Physics of Solar Flares, ed. W. N. Hess (SP-50; Washington, DC: NASA)
    • Petschek, H. E. 1964, in Proc. AAS-NASA Symp., The Physics of Solar Flares, ed. W. N. Hess (SP-50; Washington, DC: NASA), 425
    • (1964) Proc. AAS-NASA Symp. , pp. 425
    • Petschek, H.E.1
  • 20
    • 0007460132 scopus 로고    scopus 로고
    • Magnetic Reconnection in the Solar Atmosphere, ed. R. D. Bentley & J. T. Mariska (San Francisco: ASP)
    • Savy, S. K. 1997, in ASP Conf. Ser. Ill, Magnetic Reconnection in the Solar Atmosphere, ed. R. D. Bentley & J. T. Mariska (San Francisco: ASP), 240
    • (1997) ASP Conf. Ser. Ill , pp. 240
    • Savy, S.K.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.