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Future Research Directions: Theoretical Approach and Perspective

Published online by Cambridge University Press:  12 April 2016

N.O. Weiss
N.O. Weiss*
Affiliation:
Dept. of Applied Mathematics and Theoretical Physics, University of Cambridge, England

Abstract

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It is difficult to provide a comprehensive theoretical explanation for the activity of red dwarf stars. Among particular problems that are ripe for further investigation are: the production of steady, cyclic or irregular patterns of activity by nonlinear dynamo action in stars; the effect of magnetic buoyancy in producing photospheric magnetic fields; the formation of isolated flux tubes and their interaction with convection. These topics are discussed and some future lines of research are suggested.

Type
Session V: Future Research Direction and Conclusion
Information
International Astronomical Union Colloquium , Volume 71: Activity in Red-Dwarf Stars , 1983 , pp. 639 - 650
Copyright
Copyright © Reidel 1983

References

REFERENCES

Acheson, D.J.: 1978, Phil. Trans. Roy. Soc. A 289, pp.459–500.Google Scholar
Acheson, D.J.: 1979, Solar Phys. 62, pp.23–50.Google Scholar
Arter, W.: 1983, in “Solar and Stellar Magnetic Fields” (IAU Symp. No.102), ed. Stenflo, J.O., Reidel, Dordrecht.Google Scholar
Arter, W., Galloway, D.J. and Proctor, M.R.E.: 1982, Mon. Not. Roy. Astr. Soc., in press.Google Scholar
Belvedere, G.: 1983, in these Proceedings.Google Scholar
Cattaneo, F.: 1982, in preparation.Google Scholar
Cattaneo, F., Jones, C.A. and Weiss, N.O.: 1983, in “Solar and Stellar Magnetic Fields” (IAU Symp. No.102), ed. Stenflo, J.O., Reidel, Dordrecht.Google Scholar
Claverie, A., Isaak, G.R., McLeod, C.P. and van der Raay, H.B.: 1981, Nature 293, pp.443–445.Google Scholar
Deinzer, W., Hensler, G., Schmitt, D., Schussler, M. and Weisshaar, E.: 1983, in “Solar and Stellar Magnetic Fields” (IAU Symp. No. 102), ed. Stenflo, J.O., Reidel, Dordrecht.Google Scholar
Galloway, D.J. and Proctor, M.R.E.: 1982, in “Planetary and Stellar Magnetism”, ed. Soward, A.M., Gordon and Breach, London.Google Scholar
Galloway, D.J. and Weiss, N.O.: 1981, Astrophys. J. 243, pp.945–953.CrossRefGoogle Scholar
Gilman, P.A.: 1983, in “Solar and Stellar Magnetic Fields” (IAU Symp. No. 102), ed. Stenflo, J.O., Reidel, Dordrecht.Google Scholar
Gilman, P.A. and Miller, J. : 1981, Astrophys. J. Supp. 46, pp.211–238.Google Scholar
Gough, D.O.: 1982, Nature 298, pp.334–339.Google Scholar
Hughes, D.W.: 1982, in preparation.Google Scholar
Knobloch, E. and Spruit, H.C.: 1982, Astron. Astrophys., in press.Google Scholar
Meneguzzi, M., Frisch, U. and Pouquet, A.: 1981, Phys. Rev. Lett. 47, pp.1060–1064.CrossRefGoogle Scholar
Moffatt, H.K.: 1978, “Magnetic Field Generation in Electrically Conducting Fluids”, Cambridge University Press.Google Scholar
Nordlund, A.: 1981, Astron. Astrophys. 107, pp.1–10.Google Scholar
Nordlund, A.: 1983, in “Solar and Stellar Magnetic Fields” (IAU Symp. No. 102), ed. Stenflo, J.O., Reidel, Dordrecht.Google Scholar
Parker, E.N.: 1979, “Cosmical Magnetic Fields”, Clarendon Press, Oxford.Google Scholar
Proctor, M.R.E. and Weiss, N.O.: 1982, Rep. Prog. Phys., in press.Google Scholar
Schmitt, J. and Rosner, R.: 1982, Astrophys. J., in press.Google Scholar
Schüssler, M.: 1983, in “Solar and Stellar Magnetic Fields” (IAU Symp. No. 102), ed. Stenflo, J.O., Reidel, Dordrecht.Google Scholar
Spiegel, E.A. and Weiss, N.O.: 1980, Nature 287, pp.616–617.Google Scholar
Spiegel, E.A. and Weiss, N.O.: 1982, Geophys. Astrophys. Fluid Dyn., in press.Google Scholar
Spruit, H.C.: 1981, in “The Sun as a Star”, ed. Jordan, S.D., pp.385–412, NASA SP-450, Washington.Google Scholar