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Titlebook: Solar and Stellar Physics; Proceedings of the 5 Egon-Horst Schröter,Manfred Schüssler Conference proceedings 1987 Springer-Verlag Berlin He

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书目名称Solar and Stellar Physics
副标题Proceedings of the 5
编辑Egon-Horst Schröter,Manfred Schüssler
视频videohttp://file.papertrans.cn/872/871463/871463.mp4
丛书名称Lecture Notes in Physics
图书封面Titlebook: Solar and Stellar Physics; Proceedings of the 5 Egon-Horst Schröter,Manfred Schüssler Conference proceedings 1987 Springer-Verlag Berlin He
描述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.)
出版日期Conference proceedings 1987
关键词Granulation; LOPES; astrophysics; solar activity; solar physics; solar wind
版次1
doihttps://doi.org/10.1007/BFb0032307
isbn_softcover978-3-662-13631-7
isbn_ebook978-3-540-48053-2Series ISSN 0075-8450 Series E-ISSN 1616-6361
issn_series 0075-8450
copyrightSpringer-Verlag Berlin Heidelberg 1987
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Observations from space vs. ground based observations: Advantages and disadvantages,ve, either directly or indirectly, access to:.Instrumentation and observing modes have to comply with the scientific needs. With the aid of a few examples we discuss advantages and disadvantages of observations from space and from the ground.
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Solar and Stellar Physics978-3-540-48053-2Series ISSN 0075-8450 Series E-ISSN 1616-6361
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Lecture Notes in Physicshttp://image.papertrans.cn/s/image/871463.jpg
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Stellar activity and rotation,the aim of indicating which are the most significant data that are required to constrain possible models of stellar activity. The sporadic and cyclic variability aspect is, particularly stressed, firstly, because it is a crucial activity parameter and, secondly, because of its possible effects. on t
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Solar and stellar chromospheres,spheres and their variation among the stars, and the underlying fine structure that affects or determines these global properties. After an introductory discussion of the gross vertical structure of a stellar chromosphere, attention is given to the chromospheric geometric extent and its dependence o
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