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The Hale solar sector boundary

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Abstract

A Hale solar sector boundary is defined as the half (northern hemisphere or southern hemisphere) of a sector boundary in which the change of sector magnetic field polarity is the same as the change of polarity from a preceding spot to a following spot. Above a Hale sector boundary the green corona has maximum brightness, while above a non-Hale boundary the green corona has a minimum brightness. The Hale portion of a photospheric sector boundary tends to have maximum magnetic field strength, while the non-Hale portion has minimum field strength.

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References

  • Antonucci, E. and Duvall, T.: 1974, Solar Phys., 38, 439.

    Google Scholar 

  • Bumba, V. and Howard, R.: 1969, Solar Phys., 7, 28.

    Google Scholar 

  • Hansen, S., Sawyer, C. and Hansen, R. T.: 1974, Geophys. Res. Letters, 1, 13.

    Google Scholar 

  • Howard, R.: 1972, Solar Phys., 25, 5.

    Google Scholar 

  • Howard, R. A. and Kooman, M. J.: 1974, Solar Phys., 37, 469.

    Google Scholar 

  • Schatten, K. H., Ness, N. F. and Wilcox, J. M.: 1968, Solar Phys., 5, 240.

    Google Scholar 

  • Stix, M.: 1974, Astron. Astrophys., 37, 121.

    Google Scholar 

  • Suess, S. T.: 1975, J. Am. Inst. Aeron. Astromautics, 13, 443.

    Google Scholar 

  • Svalgaard, L., Wilcox, J. M. and Duvall, T: 1974a, Solar Phys., 37, 157.

    Google Scholar 

  • Svalgaard, L., Antonucci, E., Duvall, T., Wilcox, J. M. and Dittmer, P. H.: 1974b, Trans. AGU EOS, 55, 556.

    Google Scholar 

  • Svalgaard, L. and Wilcox, J. M.: 1975, Solar Phys., 41, 461.

    Google Scholar 

  • Svalgaard, L., Wilcox, J. M, Scherrer, P. H. and Howard, R: 1975, Solar Phys., 45, 83.

    Google Scholar 

  • Svalgaard, L. and Wilcox, J. M.: 1976, Nature, submitted.

  • Timothy, A. F., Krieger, A. S. and Vaiana, G. S.: 1975, Solar Phys., 42, 135.

    Google Scholar 

  • Waldmeier, M.: 1973, Solar Phys., 28, 389.

    Google Scholar 

  • Wilcox, J. M.: 1968, Space Sci. Rev. 8, 258.

    Google Scholar 

  • Wilcox. J. M.: 1971, Comments on Astrophys. and Space Phys., 3, 133.

    Google Scholar 

  • Wolfer, A.: 1897, Publ. Sternw. Eidg. Polytechn. Zürich, 1, 317.

    Google Scholar 

  • Wolff, C. L.: 1974, Astrophys. J., 194, 489.

    Google Scholar 

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Authors and Affiliations

  1. Institute for Plasma Research, Stanford University, Stanford, California, USA

    Leif Svalgaard & John M. Wilcox

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  1. Leif Svalgaard
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  2. John M. Wilcox
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Svalgaard, L., Wilcox, J.M. The Hale solar sector boundary. Sol Phys 49, 177–185 (1976). https://doi.org/10.1007/BF00221492

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  • DOI: https://doi.org/10.1007/BF00221492

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