Solar and Stellar Physics
Proceedings of the 5th European Solar Meeting Held in Titisee/Schwarzwald, Germany, April 27-30, 1987
Published on 20. November 2013
Book
Paperback/Softback
V, 234 pages
978-3-662-13631-7 (ISBN)
Description
These proceedings bring together ideas from solar and stellar physics. The sun is near enough for rather detailed observations and one chapter is devoted to the more recent experimental data from observations from space. On the other hand the multitude of stars provides a wide range of physical parameters to test hypotheses in solar and stellar astrophysics. The reader will find an illuminating overview of these fields ranging from the dynamo in the convection zone to the stellar envelopes and winds in the outer regions. In particular the importance of small-scale magnetohydrodynamic processes for the activity phenomena plays an important role in the contributions to this volume. For both students and researchers the general introduction by N. O. Weiss makes an excellent guide to this very active field of research. (See also Lecture Notes in Physics Vol. 291.)
More details
Series
Edition
Softcover reprint of the original 1st ed. 1987
Language
English
Place of publication
Berlin
Germany
Publishing group
Springer Berlin
Target group
Professional and scholarly
Research
Illustrations
20 s/w Abbildungen
V, 234 p. 20 illus.
Dimensions
Height: 244 mm
Width: 170 mm
Thickness: 14 mm
Weight
429 gr
ISBN-13
978-3-662-13631-7 (9783662136317)
DOI
10.1007/BFb0032307
Schweitzer Classification
Other editions
Additional editions
Egon-Horst Schröter | Manfred Schüssler
Solar and Stellar Physics
Proceedings of the 5th European Solar Meeting Held in Titisee/Schwarzwald, Germany, April 27-30, 1987
Book
12/1987
Springer
€85.59
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Content
What can the sun tell us about stellar activity?.- On the origin of stellar magnetism.- Stellar activity and rotation.- Solar and stellar convection.- Photospheric structure in solar-type stars.- Solar and stellar chromospheres.- Solar an stellar coronae.- Stellar vs. solar activity: The case of pre-main sequence stars.- Winds in late type stars and the solar wind.- Observations from space vs. ground based observations: Advantages and disadvantages.- New ideas about granulation based on data from the solar optical universal polarimeter instrument on spacelab 2 and magnetic data from big bear solar observatory.- Future prospects of stellar and solar physics from space.