Abstract
Viscous resistance to differential rotation causes a current whose magnetic field is proportional to the vorticity of the medium. The magnetic fields of stars and galaxies could arise in this manner, provided that the time scale for development of the field is reasonable. The latter condition (assuming Ohmic rather than synchroton dissipation) requires that the scale length for a galactic field be less than 3×1013 cm. It is suggested that there may be continual generation of field within the core of a vortex of this dimension in the galactic nucleus, the field lines then being carried outwards by expanding plasma. The main observational evidence in connection with solar, stellar and galactic magnetic fields is appraised in the context of the above theory.
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References
Angel, J. R. P.: 1978,Ann. Rev. Astron. Astrophys. 16, 487.
Arp, H. C.: 1963,Sci. Am. 208, 71.
Axon, D. J., and Taylor, K.: 1978,Nature 274, 37.
Babcock, H. W.: 1951,Astrophys. J. 114, 1.
Babcock, H. W.: 1958a,Astrophys. J. 128, 228.
Babcock, H. W.: 1958b,Astrophys. J. Suppl. 3, 141.
Babcock, H. W.: 1961,Astrophys. J. 133, 572.
Beckers, J. M.: 1976,Nature 260, 227.
Beckers, J. M., and Schroter, E. H.: 1968,Solar Phys. 4, 165.
Berge, G. L., and Seielstad, G. A.: 1967,Astrophys. J. 148, 367.
Biermann, L.: 1950,Z Naturforsch 5a, 65.
Bjerknes, V.: 1926,Astrophys. J.:64, 93.
Bonsack, W. K., and Wolff, S. C.: 1980,Astron. J. 85, 599.
Borra, E. F., and Landstreet, J. D.: 1980,Astrophys. J. Suppl. 42, 421.
Brinkman, H. C.: 1959,Physica 25, 1063.
Browne, P. F.: 1968a,Astrophys. Letters 2, 217.
Browne, P. F.: 1968b,Nature 220, 1296.
Bruznek, A.: 1967,Solar Phys. 2, 541.
Burbidge, E. M.:Plasma Astrophysics, Proceedings of the International School of Physics Enrico Fermi, No. 39, p. 254.
Cattani, D.: 1967,Nuovo Cimento 52B, 574.
Claverie, A., Isaak, G. R., McLeod, C. P., and van der Raay, H. B.: 1981,Nature 293, 443.
Clube, S. V. M.: 1978,Vistas Astron. 22, 77.
Coles, W. A., Rickett, B. J., Rumsey, V. H., Kaufman, J. J., Turley, D. G., Ananthakrishnan, S., Armstrong, J. W., Harmons, J. K., Scott, S. L. and Sime, D. G.: 1980,Nature 286, 239.
Cowling, T. G.: 1956,Monthly Notices Roy. Astron. Soc. 116, 114.
Dennison, B.: 1980,Astrophys. J. 236, 761.
Dicke, R. H., and Goldenberg, H. M.: 1967,Phys. Rev. Letters 18, 313.
Dicke, R. H., and Goldenber, H. M.: 1974,Astrophys. J. Suppl. 27, 131.
Dunn, R. B., and Zirker, J. B.: 1973,Solar Phys. 33, 281.
Eddy, J. A., Gilman, P. A., and Trotter, D. E.: 1977,Science 198, 824.
El-Raey, M., and Scherrer, P.: 1972,Solar Phys. 26, 15.
Gardner, F. F., and Davies, R. D.: 1966,Australian J. Phys. 19, 129.
Gilman, P. A.: 1974,Ann. Rev. Astron. Astrophys. 12, 47.
Harrison, E. R.: 1968,Astrophys. Letters 3, 133.
Heiles, C., and Chu, Y.-H.: 1980,Astrophys. J. 235, L105.
Howard, R.: 1977a,Ann. Rev. Astron. Astrophys. 15, 153.
Howard, R.: 1977b,Astrophys. J. 210, L159.
Howard, R. and Harvey, J.: 1970,Solar Phys. 12, 23.
Lallemand, A., Duchesne, M., and Walker, M. F.: 1960,Publ. Astron. Soc. Pacific 72, 76.
Landstreet, J. D.: 1979, in H. M. van Horn and V. Weidermann (eds.), ‘White Dwarfs and Variable Degenerate Stars’,IAU Symp. 53, 297.
Landstreet, J. D.: 1980,Astron. J. 85, 611.
Ledoux, P.: 1951,Astrophys. J. 114, 373.
Ledoux, P. and Renson, P.: 1966,Ann. Rev. Astron. Astrophys. 4, 293.
Mathers, C. D., and Cramer, N. F.: 1978,Australian J. Phys. 31, 171.
Mehltretter, J. P.: 1974,Solar Phys. 38, 43.
Meyer, F., Schmidt, H. U., Weiss, N. O., and Wilson, P. R.: 1974,Monthly Notices Roy. Astron. Soc. 169, 35.
Morris, D., and Berge, G. L.: 1964,Astrophys. J. 139, 1388.
Moss, D., and Smith, R. C.: 1981,Report Prog. Phys. 44, 831.
Munch, G.: 1960,Astrophys. J. 131, 250.
Parker, E. N.: 1977,Ann. Rev. Astron. Astrophys. 15, 45.
Parker, E. N.: 1979,Astrophys. J. 230, 905.
Piddington, J. H.: 1975,Astrophys. Space Sci. 34, 347.
Richardson, R. S., and Schwarzschild, M.: 1980, ‘Convegno Volta’,Acad. Naz. Lincei 11, 228.
Schatten, K. H.: 1977,Vistas Astron. 20, 475.
Schmidt, H. U.: 1974, in R. G. Athay (ed.), ‘Chromospheric Fine Structure’,IAU Symp. 56, 95.
Sheeley, N. R.: 1969,Solar Phys. 9, 347.
Simard-Normandin, M., and Kronberg, P. P.: 1979,Nature 279, 115.
Slettebak, A.: 1954,Astrophys. J. 119, 146.
Spitzer, L.: 1956,The Physics of Fully Ionized Gases, Interscience, New York.
Svalgaard, L., and Wilcox, J. M.: 1978,Ann. Rev. Astron. Astrophys. 16, 429.
van Breugel, W. J. M.: 1980a,Astron. Astrophys. 81, 265.
van Breugel, W. J. M.: 1980b,Astron. Astrophys. 88, 248.
van Breugel, W. J. M., and Willis, A. G.: 1981,Astron. Astrophys. 96, 332.
Vrabec, D.: 1974, in R. G. Athay (ed.), ‘Chromospheric Fine Structure’,IAU Symp. 56, 201.
Walker, M. F.: 1962,Astrophys. J. 136, 695.
Wilcox, J., Schatten, K., Tanenbaum, A., and Howard, R.: 1970,Solar Phys. 14, 255.
Willis, A. G., Strom, R. G., Bridle, A. H., and Fomalont, E. B.: 1981,Astron. Astrophys. 95, 250.
Zwaan, C.: 1978,Solar Phys. 60, 213.
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Browne, P.F. Vorticity and astrophysical magnetism. Astrophys Space Sci 87, 407–423 (1982). https://doi.org/10.1007/BF00648933
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DOI: https://doi.org/10.1007/BF00648933