The sun and cool stars : activity, magnetism, dynamos : proceedings of Colloquium no. 130 of the International Astronomical Union, held in Helsinki, Finland, 17-20 July 1990 / I. Tuominen, D. Moss, G. Rüdiger, eds.

By: International Astronomical Union. Colloquium (130th : 1990 : Helsinki, Finland)
Contributor(s): Tuominen, I. (Ilkka), 1939- | Moss, D, 1943- | Rüdiger, G. (Günther)
Material type: TextTextSeries: Lecture notes in physics: 380.Publisher: Berlin ; New York : Springer-Verlag, 1991Description: 1 online resource (x, 530 pages) : illustrationsContent type: text Media type: computer Carrier type: online resourceISBN: 9783540464839; 3540464832Subject(s): Solar activity -- Congresses | Solar magnetic fields -- Congresses | Cool stars -- Congresses | Dynamo theory (Cosmic physics) -- Congresses | Astrophysics -- Congresses | Astrophysics | Cool stars | Dynamo theory (Cosmic physics) | Solar activity | Solar magnetic fields | Veranderlijke sterren | Magnetische velden | Zon | Dynamotheorie | Aktivität | Dynamotheorie | Kongress | Kühler Stern | Magnetismus | Sonnenaktivität | Soleil -- Activité | Soleil -- Champ magnétique | Étoiles froides | SonneGenre/Form: Electronic books. | Conference papers and proceedings. | Helsinki (1990) Additional physical formats: Print version:: Sun and cool stars.DDC classification: 523.7 LOC classification: QB524 | .I59 1990Other classification: 39.40 | UD 8220 Online resources: Click here to access online Action note: digitized 2010 committed to preserveSummary: The contributions in this volume report recent studies on the sun and late-type stars. Particular emphasis is placed on observations that are relevant to the question of large-scale magnetic activity, and also on the theoretical (dynamo) models for such activity. Experimental papers deal with surface imaging techniques. Explicit computer simulations of hydromagnetic turbulence give insight into the magnetic topology and associated fluid motions, especially near the base of the convection zone. In addition, mean-field dynamo models are presented. The book addresses researchers but should also jbe useful for graduate students.
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The contributions in this volume report recent studies on the sun and late-type stars. Particular emphasis is placed on observations that are relevant to the question of large-scale magnetic activity, and also on the theoretical (dynamo) models for such activity. Experimental papers deal with surface imaging techniques. Explicit computer simulations of hydromagnetic turbulence give insight into the magnetic topology and associated fluid motions, especially near the base of the convection zone. In addition, mean-field dynamo models are presented. The book addresses researchers but should also jbe useful for graduate students.

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