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Radio observations of active stars: Direct evidence for polarity reversals?

  • 2. Rotation and Activity in Main Sequence Stars
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Part of the book series: Lecture Notes in Physics ((LNP,volume 193))

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References

  • Fisher, P. L. and Gibson, D. M. 1982, in Second Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun (SAO Spec. Rept. 392), eds. M. S. Giampapa and L. Golub, Vol. 2, p. 109.

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  • Gibson, D. M. 1983, Proc. Southwest Reg. Conf. Astron. Astrophys., IX, in press.

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  • Hjellming, R. M. and Gibson, D. M. 1980, in Radio Physics of the Sun, IAU Symp. 86, eds. M. R. Kundu and T. E. Gergely (Dordrecht: Reidel), p. 209.

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  • Melrose, D. B. and Dulk, G. A. 1982, Ap. J., 259, 844.

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  • Owen, F. N., Jones, T. W., and Gibson, D. M. 1976, Ap. J. (Lett.), 210, L27.

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  • Stenflo, J. O. 1968, in Structure and Development of Solar Active Regions, IAU Symp. 3, ed. H. Kiepenheuer (Dordrecht: Reidel), p. 47.

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Sallie L. Baliunas Lee Hartmann

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© 1984 Springer-Verlag

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Gibson, D.M. (1984). Radio observations of active stars: Direct evidence for polarity reversals?. In: Baliunas, S.L., Hartmann, L. (eds) Cool Stars, Stellar Systems, and the Sun. Lecture Notes in Physics, vol 193. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-12907-3_203

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  • DOI: https://doi.org/10.1007/3-540-12907-3_203

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-12907-3

  • Online ISBN: 978-3-540-38785-5

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