Abstract
The long-term evolution of the polar magnetic field at the coronal base induced by the first Rossby mode demonstrates the reversal of the line-of-sight magnetic field component in polar caps and what is more the same line-of-sight magnetic polarities in both caps (“the line-of-sight solar magnetic monopole”) at the moment of reversal.
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References
Altschuler, M. D. and Newkirk, G., Jr.:1969, Solar Phvs. 9, 131.
Babcock, H. D.: 1959, Astrophys. J. 130, 364.
Balogh, A. and Forsyth, R. J.: 1998, in E. R. Priest, F. Moreno-Insertis, and R. A. Harris (eds.), A Crossroads for European Solar and Heliospheric Physics,ESA SP-417, p. 45.
Burlaga, L. F. and Ness, N. F.:1993, J. Geophys. Res. 98, 17451.
Cowling, T. G.: 1981, Ann. Rev. Astron. Astrophys. 19, 115.
Hoeksema, J. T.: 1991, Tech. Rep. CSSA-ASTRO-91–01, Stanford Univ., CA.
Hoeksema, J. T.: 1992, in E. Marsch, and R. Schwenn (eds.), Solar Wind Seven, Vol. 3, Pergamon Press, London, p. 191.
Howard, R. and Harvey, J.: 1970, Solar Phys. 12, 23.
Hundhausen, A. J.: 1997, in J. B. Zirker (eds.), Coronal Holes and High Speed Wind Streams, Colorado Associated University Press, Boulder, Ch. 7, p. 224.
Layzer, D., Rosner, R. and Doyle, H. T.: 1979, Astrophys. J. 229, 1126.
Piddington, J. H.: 1970, Aust. J. Phvs. 23, 791.
Parker, E. N.: 1979, Cosmical Magnetic Fields (Their Origin and Their Activity), Clarendon Press, Oxford.
Pisanko, Yu. V., Tritakis, V. P. and Paliatsos, A. G.: 1997, in O. Kjeldseth-Moe, and A. Wilson (eds.), The Corona and Solar Wind Near Minimum Activity,ESA SP-404, p. 609.
Pisanko, Yu. V.: 1999, in J.-C. Vial, and B. Kaldeich-Schurmann (eds.), Plasma Dynamics and Diagnostics in the Solar Transition Region and Corona,ESA SP-446, p. 543.
Schatten, K. H., Wilcox, J. M., and Ness N. F., Solar Phvs. 6, 442.
Smith, E. J., Neugebauer, M., Balogh, A., Bame, S. J., Erdos, G., Forsyth, R. J., Goldstein, B. E., Phillips, J. L. and Tsurutani, B. T.: 1993, Geophys. Res. Lett. 20, 2327.
Trellis, M. M.: 1960, Compt. Rend. Acad. Sci. 250, 58.
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Pisanko, Y.V. (2001). A Model of the Magnetic Field Long-Term Evolution at the Coronal Base and Polar Heliospheric Regions. In: Marsden, R.G. (eds) The 3-D Heliosphere at Solar Maximum. Springer, Dordrecht. https://doi.org/10.1007/978-94-017-3230-7_27
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DOI: https://doi.org/10.1007/978-94-017-3230-7_27
Publisher Name: Springer, Dordrecht
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