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):

Material type: Text

TextSeries: Lecture notes in physics ; 380.Publication details: Berlin ; New York : Springer-Verlag, 1991.Description: 1 online resource (x, 530 pages) : illustrationsContent type:

text

Media type:

computer

Carrier type:

online resource

ISBN:

9783540464839
3540464832

Subject(s): Genre/Form:

Additional physical formats: Print version:: Sun and cool stars.DDC classification:

523.7 20

LOC classification:

QB524 .I59 1990

Other classification:

39.40
UD 8220

Online resources:

Click here to access online

Action note:

digitized 2010 HathiTrust Digital Library committed to preserve

Summary: 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.

Holdings ( 1 )
Title notes ( 8 )

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Item type	Current library	Collection	Call number	Status	Date due	Barcode	Item holds
eBook	e-Library	eBook LN Physics		Available

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Includes bibliographical references.

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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