Accretion Disks and Magnetic Fields in Astrophysics: by G. Belvedere (auth.), G. Belvedere (eds.)

By G. Belvedere (auth.), G. Belvedere (eds.)

`It is that this element that makes this e-book specific significance to excessive strength astrophysicists.'
Space technological know-how assessment 56, 1991

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Extra resources for Accretion Disks and Magnetic Fields in Astrophysics: Proceedings of the European Physical Society Study Conference, Held in Noto (Sicily), Italy, June 16–21, 1988

Sample text

Then I diseuss nonlinear dynamo waves in Seetion 5. Finally I shall try to summarize our eurrent understanding of nonlinear stellar dynamos in the eonduding seetion. 2. Solar and Stellar Magnetic Activity We shall be eoneerned with magnetic aetivity in lower main-sequenee stars of speetral types G, K and M. In these dwarf stars, which have deep outer eonveetive zones and are typically slow rotators, the eombination of rotation and eonvection produces variable magnetie fields. ) Although solar activity is relatively weak the Sun is the obvious prototype with whieh other cool stars ean be eompared.

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