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On the Spottedness, Magnetism and Internal Structure of Stars

  • R.E. Gershberg (a1)

Abstract

It is hypothesized that kinematical structures within stellar interiors that are results of a self-organization of these interiors as thermodynamically open nonlinear systems constitute the physical basis for stellar magnetism.

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Copyright

References

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Appenzeller, I. and Dearborn, D.S.F, 1984 - Astrophys. J. v. 278, p. 689.
Gerenberg, R.E., 1982 - Astron. Nachr. v. 303, p. 251.
Gershberg, R.E., 1983 - in Byrne, P.B. and Rodono, M. (eds)‘Activity in red dwarf stars’. Reidel, Dordrecht, p. 487.
Hartmann, L. and Rosner, R., 1979 - Astrophys. J. v. 230, p. 802.
Howard, R. and LaBonte, B.J., 1983 - in Stenflo, J.O. (ed)‘Solar and stellar magnetic fields: origins and coronal effects’. Reidel. Dordrecht, p. 101.
Roxburgh, I.W., 1983 - in Stenflo, J.O. (ibid), p. 449.
Vaiana, G.S., 1983 - in Stenflo, J.O. (ibid), p. 165.
Vaughan, A.H., 1983 - in Stenflo, J.O. (ibid), p. 113.
Willson, R.C., Gulkis, S., Janssen, M., Hudson, H.S., Chapman, G.A., 198I - Science, v. 211, p. 700.

On the Spottedness, Magnetism and Internal Structure of Stars

  • R.E. Gershberg (a1)

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