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Manifestations of Solar Magnetic Fields

Published online by Cambridge University Press:  14 August 2015

S.K. Solanki
S.K. Solanki*
Affiliation:
Institute of Astronomy, ETH, CH-8092 Zurich, Switzerland

Abstract

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The magnetism of the Sun manifests itself in innumerable ways, many of which constitute what is referred to as solar magnetic activity, while others are counted among the phenomena of the quiet Sun. After a brief overview of the structure of the solar magnetic field, a few examples of its manifestations are pointed out.

Type
II. Joint Discussions
Information
Highlights of Astronomy , Volume 11 , Issue 2: Highlights of Astronomy. As presented at the XXIIIrd General Assembly of the IAU (Part B), 1997 , 1998 , pp. 857 - 860
Copyright
Copyright © Kluwer 1998

References

Alissandrakis, C.E., Kundu, M.R., Lantos, P., 1980, Aatron. Astrophyl. 82, 30–40.Google Scholar
Bogdan, T.J., Brown, T.M., Lites, B.W., Thomas, J.H., 1993, Astrophys. J. 406, 723–734.Google Scholar
Bommier, V., Leroy, J.L., 1997, in New Perspectives on Solar Prominences, Webb, D., Schmieder, B., Rust, D. (Eds.), IA U Coll. 167 in pressGoogle Scholar
Braun, D.C., Duvall, T.L. Jr., La Bonte, B.J., Jefferies, S.M., Harvey, J.W., Pomerantz, M.A., 1992, Astrophys. J. 391, L113–L116.Google Scholar
Carlsson, M., Stein, R.F., 1995, Astrophys. J. 440, L29–L32.CrossRefGoogle Scholar
Degenhardt, D., Wiehr, E., 1991, Astron. Astrophys. 252, 821–826.Google Scholar
Dere, K.P., Bartoe, J.-D.F., Brueckner, G.E., 1989, Solar Phys. 123, 41–68.Google Scholar
Dere, K.P., Bartoe, J.-D.F., Brueckner, G.E., Ewing, J., Lund, P., 1991, J. Geophys. Res. 96, 9399 Google Scholar
Elsworth, Y., Howe, R., Isaak, G.R., McLeod, C.P., Miller, B.A., New, R., Speake, C.C., Wheeler, S.J., 1994, Astrophys. J. 434, 801–806.Google Scholar
Fontenla, J.M., Avrett, E.H., Loeser, R., 1993, Astrophys. J. 406, 319–345.CrossRefGoogle Scholar
Foukal, P., Lean, J., 1988, Astrophys. J. 328, 347–357.Google Scholar
Harvey, K.L., 1985, Australian J. Phys. 38, 875 Google Scholar
Harvey, K.L., Harvey, J.W., Martin, S.F., 1975, Solar Phys. 40, 87–102.Google Scholar
Innes, D.E., Inhester, B., Axford, W.I., Wilhelm, K., 1997, Nature 386, 811–813.Google Scholar
Keller, C.U., Deubner, F.-L., Egger, U., Fleck, B., Povel, P., 1994, Astron. Astrophys. 286, 626–634.Google Scholar
Klein, L., 1992, in Methods of Solar and Stellar Magnetic Field Determination, Faurobert-Scholl, M., Mein, N., Frisch, H. (Eds.), Obs. de Paris, Meudon, p. 113–130.Google Scholar
Lee, J.W., Hurford, G.J., Gary, D.E., 1993, in The Magnetic and Velocity Fields of Solar Active Regions, Zirin, H., Ai, G., Wang, H. (Eds.), Astron. Soc. Pacific Conf. Series, IAU Coll. 141, 287–290.Google Scholar
Lee, J.W., White, S.M., Gopalswamy, N., Kundu, M.R., 1997, Solar Phys. submittedGoogle Scholar
Libbrecht, K.G., Woodard, M.F., 1990, Nature 345, 779–782 Google Scholar
Lin, H., 1995, Astrophys. J. 446, 421–430 Google Scholar
Leroy, J.L., 1985, in Measurements of Solar Vector Magnetic Fields, Hagyard, M.J. (Ed.), NASA Conf. Publ. 2374, p. 121–140.Google Scholar
Martin, S.F., 1988, Solar Phys. 117, 243–259.Google Scholar
Parker, E.N., 1988, Astrophys. J. 330, 474–479.CrossRefGoogle Scholar
Priest, E.R., Parnell, C.E., Martin, S.F., 1994, Astrophys. J. 427, 459–474.CrossRefGoogle Scholar
Schmelz, J.T., Holman, G.D., Brosius, J.W., Willson, R.F., 1994, Astrophys. J. 434, 786–794.Google Scholar
Schrijver, C.J., Coté, J., Zwaan, C., Saar, S.H., 1989, Astrophys. J. 337, 964–976.Google Scholar
Shibata, K.: 1982, Solar Phys. 81, 9–17.Google Scholar
Solanki, S.K., Schmidt, H.U., 1993, Astron. Astrophys. 267, 287–291.Google Scholar
Solanki, S.K., Unruh, Y., 1997, Astron. Astrophys. in pressGoogle Scholar
Solanki, S.K., Livingston, W., Ayres, T., 1994, Science 263, 64–66.CrossRefGoogle Scholar
Solanki, S.K., Zuffrey, D., Lin, H., Rüedi, I., Kuhn, J., 1996, Astron. Astrophys. 310, L33–L36.Google Scholar
Spruit, H.C., 1982, Astron. Astrophys. 108, 348–355.Google Scholar
Sterling, A.C., Hollweg, J.V., 1988, Astrophys. J. 327, 950–963.Google Scholar
Tarbell, T., Peri, M., Frank, Z., Shine, R., Title, A., 1988, Seismology of the Sun and Sun-like Stars, ESA SP-286, p. 315–319.Google Scholar
Title, A., 1997, in Cool Stars, Stellar Systems and the Sun, X, Bookbinder, J.A., Donahue, R. (Eds.), Harvard Smithsonian Center for Astrophysics, Cambridge, MA, in pressGoogle Scholar
Title, A.M., Frank, Z.A., Shine, R.A., Tarbell, T.D., Topka, K.P., Scharmer, G., Schmidt, W., 1993, Astrophys. J. 403, 780–796.CrossRefGoogle Scholar
Venkatakriehnan, P., 1986, Nature 322, 156–157.Google Scholar
Willson, R.C., Hudson, H.S., 1991, Nature 351, 42–44.CrossRefGoogle Scholar
Yokoyama, T., Shibata, K., 1995, Nature 375, 42–44.Google Scholar
Zirin, H., 1987, Solar Phys. 110, 101–107.CrossRefGoogle Scholar