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Mechanisms for the rigid rotation of coronal holes

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Abstract

We show that the rotation of coronal holes can be understood in terms of a current-free model of the coronal magnetic field, in which holes are the footpoint locations of open field lines. The coronal field is determined as a function of time by matching its radial component to the photospheric flux distribution, whose evolution is simulated including differential rotation, supergranular diffusion, and meridional flow. We find that ongoing field-line reconnection allows the holes to rotate quasi-rigidly with their outer-coronal extensions, until their boundaries become constrained by the neutral line of the photospheric field as it winds up to form stripes of alternating magnetic polarity. This wind-up may be significantly retarded by a strong axisymmetric field component which forces the neutral line to low latitudes; it is also gradually halted by the cross-latitudinal transport of flux via supergranular diffusion and a poleward bulk flow. We conclude that a strong axisymmetric field component is responsible for the prolonged rigid rotation of large meridional holes during the declining phase of the sunspot cycle, but that diffusion and flow determine the less rigid rotation observed near sunspot maximum, when the holes corotate with their confining polarity stripes.

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References

  • Altschuler, M. D. and Newkirk, G.: 1969, Solar Phys. 9, 131.

    Google Scholar 

  • Axford, W. I.: 1977, in M. A. Shea, D. F. Smart, and S. T. Wu (eds.), Study of Traveling Interplanetary Phenomena, D. Reidel Publ. Co., Dordrecht, Holland, p. 145.

    Google Scholar 

  • Bohlin, J. D.: 1977, Solar Phys. 51, 377.

    Google Scholar 

  • Bohlin, J. D. and Sheeley, N. R., Jr.: 1978, Solar Phys. 56, 125.

    Google Scholar 

  • Broussard, R. M., Sheeley, N. R., Jr., Tousey, R., and Underwood, J. H.: 1978, Solar Phys. 56, 161.

    Google Scholar 

  • Bumba, V. and Howard, R.: 1965, Astrophys. J. 141, 1502.

    Google Scholar 

  • Chapman, G. A. and Sheeley, N. R. Jr.: 1968, in K. O. Kiepenheuer (ed.), ‘Structure and Development of Solar Active Regions’, IAU Symp. 35, 161.

  • DeVore, C. R.: 1987, Solar Phys. 112, 17.

    Google Scholar 

  • DeVore, C. R. and Sheeley, N. R., Jr.: 1987, Solar Phys. 108, 47.

    Google Scholar 

  • DeVore, C. R., Sheeley, N. R., Jr., and Boris, J. P.: 1984, Solar Phys. 92, 1.

    Google Scholar 

  • Duvall, T. R., Jr.: 1979, Solar Phys. 63, 3.

    Google Scholar 

  • Fisher, R. and Sime, D. G.: 1984, Astrophys. J. 287, 959.

    Google Scholar 

  • Gabriel, A. H.: 1976, Phil. Trans. Roy. Soc. A281, 339.

    Google Scholar 

  • Giovanelli, R. G.: 1980, Solar Phys. 68, 49.

    Google Scholar 

  • Hansen, R. T., Hansen, S. F., and Loomis, H. G.: 1969, Solar Phys. 10, 135.

    Google Scholar 

  • Harvey, J. W. and Sheeley, N. R., Jr.: 1979, Space Sci. Rev. 23, 139.

    Google Scholar 

  • Harvey, J. W. and Sheeley, N. R., Jr.: 1987, Bull. Am. Astron. Soc. 19, 935.

    Google Scholar 

  • Harvey, K. L., Harvey, J. W., and Sheeley, N. R. Jr.: 1986, in P. A. Simon, G. Heckman, and M. A. Shea (eds.), Solar-Terrestrial Predictions: Proceedings of a Workshop at Meudon, France, June 18–22, 1984, NOAA/AFGL, p. 198.

  • Hoeksema, J. T.: 1984, Ph.D. Thesis, Stanford University.

  • Hoeksema, J. T. and Scherrer, P. H.: 1987, Astrophys. J. 318, 428.

    Google Scholar 

  • Howard, R. and LaBonte, B. J.: 1981, Solar Phys. 74, 131.

    Google Scholar 

  • Jahnke, E. and Emde, F.: 1945, Tables of Functions, Dover, New York, p. 110.

    Google Scholar 

  • Jones, H. P.: 1985, Australian J. Phys. 38, 919.

    Google Scholar 

  • Leighton, R. B.: 1964, Astrophys. J. 140, 1547.

    Google Scholar 

  • Levine, R. H., Altschuler, M. D., Harvey, J. W., and Jackson, B. V.: 1977, Solar Phys. 25, 636.

    Google Scholar 

  • McIntosh, P. S., Krieger, A. S., Nolte, J. T., and Vaiana, G.: 1976, Solar Phys. 49, 57.

    Google Scholar 

  • Newton, H. W. and Nunn, M. L: 1951, Monthly Notices Roy. Astron. Soc. 111, 413.

    Google Scholar 

  • Parker, G. D.: 1986, Solar Phys. 104, 333.

    Google Scholar 

  • Parker, G. D., Hansen, R. T., and Hansen, S. F.: 1982, Solar Phys. 80, 185.

    Google Scholar 

  • Pneuman, G. W. and Kopp, R. A.: 1971, Solar Phys. 18, 258.

    Google Scholar 

  • Pneuman, G. W., Hansen, S. F., and Hansen, R. T.: 1978, Solar Phys. 59, 313.

    Google Scholar 

  • Pope, T. and Mosher, J.: 1975, Solar Phys. 44, 3.

    Google Scholar 

  • Rust, D. M.: 1983, Space Sci. Rev. 48, 381.

    Google Scholar 

  • Schatten, K. H., Wilcox, J. M., and Ness, N. F.: 1969, Solar Phys. 6, 442.

    Google Scholar 

  • Schatten, K. H., Leighton, R. B., Howard, R., and Wilcox, J. M.: 1972, Solar Phys. 26, 283.

    Google Scholar 

  • Sheeley, N. R., Jr.: 1980, Solar Phys. 65, 229.

    Google Scholar 

  • Sheeley, N. R., Jr.: 1981, Astrophys. J. 243, 1040.

    Google Scholar 

  • Sheeley, N. R., Jr. and DeVore, C. R.: 1986, Solar Phys. 103, 203.

    Google Scholar 

  • Sheeley, N. R., Jr. and Harvey, J. W.: 1978, Solar Phys. 59, 159.

    Google Scholar 

  • Sheeley, N. R., Jr. and Harvey, J. W.: 1981, Solar Phys. 70, 237.

    Google Scholar 

  • Sheeley, N. R., Jr., DeVore, C. R., and Boris, J. P.: 1985, Solar Phys. 98, 219.

    Google Scholar 

  • Sheeley, N. R., Jr., Nash, A. G., and Wang, Y.-M.: 1987, Astrophys. J. 319, 481 (Paper I).

    Google Scholar 

  • Sheeley, N. R., Jr., Bohlin, J. D., Brueckner, G. E., Purcell, J. D., Scherrer, V. E., and Tousey, R.: 1975a, Solar Phys. 40, 103.

    Google Scholar 

  • Sheeley, N. R., Jr., Bohlin, J. D., Brueckner, G. E., Purcell, J. D., Scherrer, V. E., and Tousey, R.: 1975b, Astrophys. J. 196, L129.

    Google Scholar 

  • Shelke, R. N. and Pande, M. C.: 1985, Solar Phys. 95, 193.

    Google Scholar 

  • Snodgrass, H.: 1983, Astrophys. J. 270, 288.

    Google Scholar 

  • Solodyna, C. V., Krieger, A. S., and Nolte, J. T.: 1977, Solar Phys. 54, 123.

    Google Scholar 

  • Stenflo, J. O.: 1974, Solar Phys. 36, 495.

    Google Scholar 

  • Stenflo, J. O.: 1977, Astr. Astrophys. 61, 797.

    Google Scholar 

  • Svalgaard, L., Duvall, T. L., Jr., and Scherrer, P. H.: 1978, Solar Phys. 58, 225.

    Google Scholar 

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

    Google Scholar 

  • Veeder, G. J. and Zirin, H.: 1970, Solar Phys. 12, 391.

    Google Scholar 

  • Wagner, W. J.: 1975, Astrophys. J. 198, L141.

    Google Scholar 

  • Waldmeier, M.: 1951, Die Sonnenkorona, Birkhauser Verlag, Basel.

    Google Scholar 

  • Wang, Y.-M., Sheeley, N. R., Jr., Nash, A. G., and Shampine, L. R.: 1988, Astrophys. J. 327, 427 (Paper II).

    Google Scholar 

  • Webb, D. F., McIntosh, P. S., Nolte, J. T., and Solodyna, C. V.: 1978, Solar Phys. 58, 389.

    Google Scholar 

  • Wilcox, J. M. and Howard, R.: 1970, Solar Phys. 13, 251.

    Google Scholar 

  • Wilcox, J. M., Schatten, K. H., Tanenbaum, A. S., and Howard, R.: 1970, Solar Phys. 14, 255.

    Google Scholar 

  • Wilson, R. M.: 1979, Results of Coronal Hole Research: An Update, NASA Technical Memorandum 78237, MSFC, Huntsville, Alabama.

    Google Scholar 

  • Zirker, J. B.: 1977a, Rev. Geophys. and Space Phys. 15, 257.

    Google Scholar 

  • Zirker, J. B.: 1977b, Coronal Holes and High Speed Wind Streams, Colorado Assoc. Univ. Press.

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Authors and Affiliations

  1. E.O. Hulburt Center for Space Research, Naval Research Laboratory, 20375-5000, Washington, D.C., U.S.A.

    A. G. Nash, N. R. Sheeley Jr. & Y. -M. Wang

  2. Applied Research Corporation, 20785, Landover, MD, U.S.A.

    Y. -M. Wang

Authors
  1. A. G. Nash
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  2. N. R. Sheeley Jr.
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  3. Y. -M. Wang
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Nash, A.G., Sheeley, N.R. & Wang, Y.M. Mechanisms for the rigid rotation of coronal holes. Sol Phys 117, 359–389 (1988). https://doi.org/10.1007/BF00147253

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  • DOI: https://doi.org/10.1007/BF00147253

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