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Volumn 202, Issue 1, 2001, Pages 11-26

Does the poleward migration rate of the magnetic fields depend on the strength of the solar cycle?

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EID: 0035647636     PISSN: 00380938     EISSN: None     Source Type: Journal    
DOI: 10.1023/A:1011855103278     Document Type: Article
Times cited : (36)

References (44)
  • 25
    • 0002339767 scopus 로고
    • Solar Photosphere: Structure, Convection, and Magnetic fields
    • J. O. Stenflo (ed.)
    • Makarov, V. I. and Sivaraman, K. R.: 1990, in J. O. Stenflo (ed.), Solar Photosphere: Structure, Convection, and Magnetic fields, IAU Symp. 138, 281.
    • (1990) IAU Symp. , vol.138 , pp. 281
    • Makarov, V.I.1    Sivaraman, K.R.2
  • 33
    • 0042498909 scopus 로고
    • Solar Magnetic Fields
    • M. Schüssler and W. Schmidt (eds.), June 29 - July 2, 1993, Cambridge University Press, Cambridge
    • Parker, E. N.: 1994, in M. Schüssler and W. Schmidt (eds.), Solar Magnetic Fields, Proc. Int. Conf. Freiburg, Germany, June 29 - July 2, 1993, Cambridge University Press, Cambridge, p. 94.
    • (1994) Proc. Int. Conf. Freiburg, Germany , pp. 94
    • Parker, E.N.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.