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Volumn 25, Issue 1, 2007, Pages 293-302

Effects of a moving X-line in a time-dependent reconnection model

Author keywords

[No Author keywords available]

Indexed keywords

MAGNETIC FIELD; MAGNETOTAIL; MODEL; PLASMA; STEADY-STATE EQUILIBRIUM; TIME DEPENDENT BEHAVIOR; TOPOLOGY;

EID: 33846876288     PISSN: 09927689     EISSN: 14320576     Source Type: Journal    
DOI: 10.5194/angeo-25-293-2007     Document Type: Article
Times cited : (2)

References (21)
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    • Alexeev, I.V.1    Semenov, V.S.2    Biernat, H.K.3
  • 10
    • 38249035257 scopus 로고    scopus 로고
    • Owen, C J. and Cowley, S W H.: Simple models of time-dependent reconnection in a collision-free plasma with an application to substorms in the geomagnetic tail, Planet. Space Sci., 35, 451–466, 1987.
    • Owen, C J. and Cowley, S W H.: Simple models of time-dependent reconnection in a collision-free plasma with an application to substorms in the geomagnetic tail, Planet. Space Sci., 35, 451–466, 1987.
  • 11
    • 0000056210 scopus 로고
    • Magnetic field annihilation
    • edited by: Hess, W. N, NASA Spec. Publ. 50, –
    • Petschek, H E.: Magnetic field annihilation, in: Physics of Solar Flares, edited by: Hess, W. N., NASA Spec. Publ. 50, 425–439, 1964.
    • (1964) Physics of Solar Flares , pp. 425-439
    • Petschek, H.E.1
  • 12
    • 0002679116 scopus 로고
    • Magnetic field reconnection theory and the solar wind-magnetosphere interaction: A review
    • Pudovkin, M I. and Semenov, V S.: Magnetic field reconnection theory and the solar wind-magnetosphere interaction: A review, Space Sci. Rev., 41, 1–89, 1985.
    • (1985) Space Sci. Rev , vol.41 , pp. 1-89
    • Pudovkin, M.I.1    Semenov, V.S.2
  • 14
    • 85039218063 scopus 로고    scopus 로고
    • Rijnbeek, R P. and Semenov, V S.: Features of a Petschek-type reconnection model, Trends in Geophys. Res., 2, 247–268, 1993.
    • Rijnbeek, R P. and Semenov, V S.: Features of a Petschek-type reconnection model, Trends in Geophys. Res., 2, 247–268, 1993.
  • 18
    • 33845809882 scopus 로고    scopus 로고
    • Reconstruction of the reconnection rate from magnetic field disturbances in an incompressible plasma
    • edited by: Biernat, H K, Lammer, H, Vogl, D. F, and Muhlbachler, S, Research Signpost, Trivandrum, India, –
    • Semenov, V S., Penz, T., Heyn, M F., Ivanov, I B., Kubyshkin, I V., Biernat, H K., and Ivanova, V V.: Reconstruction of the reconnection rate from magnetic field disturbances in an incompressible plasma, in: Solar-planetary relations, edited by: Biernat, H K., Lammer, H., Vogl, D. F., and Muhlbachler, S., Research Signpost, Trivandrum, India, 261–302, 2005a.
    • (2005) Solar-planetary relations , pp. 261-302
    • Semenov, V.S.1    Penz, T.2    Heyn, M.F.3    Ivanov, I.B.4    Kubyshkin, I.V.5    Biernat, H.K.6    Ivanova, V.V.7
  • 20
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    • Magnetic field reconnection in highly conducting incompressible fluid
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    • Sonnerup, B.U.O.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.