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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.

Information

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

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