Solar and stellar physics : proceedings of the 5th European Solar Meeting, held in Titisee/Schwarzwald, Germany, April 27-30, 1987 / E.-H. Schröter, M. Schüssler, [editors].

By: (5th : European Solar Meeting (5th : 1987 : Titisee, Germany)
Contributor(s): Schröter, E.-H. (Egon-Horst), 1928- | Schüssler, M. (Manfred), 1951-
Material type: TextTextSeries: Lecture notes in physics: 292.Publisher: Berlin ; New York : Springer-Verlag, ©1987Description: 1 online resource (iv, 231 pages) : illustrationsContent type: text Media type: computer Carrier type: online resourceISBN: 9783540480532; 3540480536Subject(s): Sun -- Congresses | Stars -- Congresses | Astrophysics -- Congresses | Étoiles -- Congrès | Astrophysique -- Congrès | Soleil -- Congrès | Astrophysics | Stars | Sun | Étoiles -- Congrès | Astrophysique -- Congrès | Soleil -- Congrès | Astrophysik | SonneGenre/Form: Electronic books. | Conference papers and proceedings. | Kongress. Additional physical formats: Print version:European Solar Meeting (5th : 1987 : Titisee, Germany).: Solar and stellar physics.DDC classification: 523.7 LOC classification: QB520 | .E87 1987Online resources: Click here to access online
Contents:
General Introduction -- Lower Atmospheres, Convection Zones -- Outer Atmospheres, Winds -- Observations from Space -- Poster Contributions -- Participants.
Action note: digitized 2010 committed to preserveSummary: 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.).
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General Introduction -- Lower Atmospheres, Convection Zones -- Outer Atmospheres, Winds -- Observations from Space -- Poster Contributions -- Participants.

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.).

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