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Volumn 110, Issue A12, 2005, Pages

Solar cycle variation of long-duration radial interplanetary magnetic field events at 1 AU

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EID: 33845795210     PISSN: None     EISSN: 21699402     Source Type: Journal    
DOI: 10.1029/2005JA011165     Document Type: Article
Times cited : (17)

References (9)
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  • 2
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  • 3
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    • Radial heliospheric magnetic fields detected by Ulysses
    • Jones, G. H., A. Balogh, and R. J. Forsyth (1998), Radial heliospheric magnetic fields detected by Ulysses, Geophys. Res. Lett., 25(16), 3109.
    • (1998) Geophys. Res. Lett. , vol.25 , Issue.16 , pp. 3109
    • Jones, G.H.1    Balogh, A.2    Forsyth, R.J.3
  • 4
    • 0037113706 scopus 로고    scopus 로고
    • Strongly underwound magnetic fields in co-rotating rarefaction regions: Observations and implications
    • doi:10.1029/2002GL015164
    • Murphy, N., E. J. Smith, and N. A. Schwadron (2002), Strongly underwound magnetic fields in co-rotating rarefaction regions: Observations and implications, Geophys. Res. Lett., 29(22), 2066, doi:10.1029/2002GL015164.
    • (2002) Geophys. Res. Lett. , vol.29 , Issue.22 , pp. 2066
    • Murphy, N.1    Smith, E.J.2    Schwadron, N.A.3
  • 5
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    • Particle and field signatures of coronal mass ejections in the solar wind
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    • Neugebauer, M., and R. Goldstein (1997), Particle and field signatures of coronal mass ejections in the solar wind, in Coronal Mass Ejections, Geophys. Monogr. Ser., vol. 99, edited by N. Crooker, J. Joselyn, and J. Feynman, p. 245, AGU, Washington, D. C.
    • (1997) Coronal Mass Ejections, Geophys. Monogr. Ser. , vol.99 , pp. 245
    • Neugebauer, M.1    Goldstein, R.2
  • 6
    • 37149007040 scopus 로고    scopus 로고
    • Features observed in the trailing regions of interplanetary clouds from coronal mass ejections
    • Neugebauer, M., R. Goldstein, and B. E. Goldstein (1997), Features observed in the trailing regions of interplanetary clouds from coronal mass ejections, J. Geophys. Res., 102(A9), 19,743.
    • (1997) J. Geophys. Res. , vol.102 , Issue.A9
    • Neugebauer, M.1    Goldstein, R.2    Goldstein, B.E.3
  • 7
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    • Dynamics of the interplanetary gas and magnetic fields
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    • Parker, E.N.1
  • 8
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    • An explanation for strongly underwound magnetic field in co-rotating rarefaction regions and its relationship to footpoint motion on the Sun
    • doi:10.1029/2002GL015028
    • Schwadron, N. A. (2002), An explanation for strongly underwound magnetic field in co-rotating rarefaction regions and its relationship to footpoint motion on the Sun, Geophys. Res. Lett., 29(14), 1663, doi:10.1029/2002GL015028.
    • (2002) Geophys. Res. Lett. , vol.29 , Issue.14 , pp. 1663
    • Schwadron, N.A.1
  • 9
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    • The heliospheric current sheet
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    • Smith, E.J.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.