Abstract
It is impossible to make a direct measurement of the coronal magnetic field from the ground. The coronal magnetic field is, then, usually inferred by extrapolation of the observed photospheric magnetic field. The so-called ‘potential model’ has been used for this extrapolation. We have to solve the Laplacian equation of the magnetic scalar potential. This magnetic scalar potential can be expanded into a spherical harmonic series. In this paper, new simple recursion formulae are proposed to solve the Laplacian equation; that is, to determine the spherical harmonic coefficients.
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References
Altschuler, M. D. and Newkirk, G., Jr.: 1969,Solar Phys. 9, 131.
Altschuler, M. D., Levine, R., Stix, M., and Harvey, J.: 1977,Solar Phys. 51, 345.
Bruno, R., Burlaga, L. F., and Hundhausen, A. J.: 1984,J. Geophys. Res. 89, 5381.
Burlaga, L. F., Hundhausen, A. J., and Zhao, X.-P.: 1981,J. Geophys. Res. 86, 8893.
Chapman, S. and Bartels, J.: 1940,Geomagnetism, Oxford University Press, London.
Hakamada, K.: 1987,J. Geophys. Res. 92, 4339.
Hakamada, K. and Kojima, M.: 1994,Solar Phys. 153, 419.
Hakamada, K., Kojima, M., and Kakinuma, T.: 1991,J. Geophys. Res. 96, 5397.
Hoeksema, J. T. and Scherrer, P. H.: 1986,Rep. UAG-94, NOAA, Boulder, Colorado.
Hoeksema, J. T., Wilcox, J. M., and Scherrer, P. H.: 1982,J. Geophys. Res. 87, 10331.
Levine, R. H.: 1977,Astrophys. J. 218, 291.
Levine, R. H.: 1979,Solar Phys. 62, 277.
Levine, R. H.: 1982,Solar Phys. 79, 203.
Levine, R. H., Altschuler, M. D., and Harvey, J. W.: 1977,J. Geophys. Res. 82, 1061.
Newkirk, G., Jr. and Altschuler, M. D.: 1970,Solar Phys. 13, 131.
Riesebieter, W. and Neubauer, F. M.: 1979,Solar Phys. 63, 127.
Schatten, K. H., Wilcox, J. M., and Ness, N. F.: 1969,Solar Phys. 9, 442.
Suess, S. T., Wilcox, J. M., Hoeksema, J. T., Henning, H., and Dryer, M.: 1984,J. Geophys. Res. 89, 3957.
Wang, Y.-M. and Sheeley, N. R., Jr.: 1992,Astrophys. J. 392, 310.
Wilcox, J. M. and Hundhausen, A. J.: 1983,J. Geophys. Res. 88, 8095.
Wilcox, J. M. and Svalgaard, L.: 1974,Solar Phys. 34, 461.
Wilcox, J. M., Hoeksema, J. T., and Scherrer, P. H.: 1980,Science 209, 603.
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Hakamada, K. A simple method to compute spherical harmonic coefficients for the potential model of the coronal magnetic field. Sol Phys 159, 89–96 (1995). https://doi.org/10.1007/BF00733033
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DOI: https://doi.org/10.1007/BF00733033