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Titlebook: Cool Stars, Stellar Systems, and the Sun; Proceedings of the F Jeffrey L. Linsky,Robert E. Stencel Conference proceedings 1987 Springer-Ver

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書(shū)目名稱(chēng)Cool Stars, Stellar Systems, and the Sun
副標(biāo)題Proceedings of the F
編輯Jeffrey L. Linsky,Robert E. Stencel
視頻videohttp://file.papertrans.cn/238/237888/237888.mp4
叢書(shū)名稱(chēng)Lecture Notes in Physics
圖書(shū)封面Titlebook: Cool Stars, Stellar Systems, and the Sun; Proceedings of the F Jeffrey L. Linsky,Robert E. Stencel Conference proceedings 1987 Springer-Ver
描述Recent research on the solar-stellar system has been triggered by a host of recent observational data, in particular from space based observations. For this conference the major topics selected centered on new measurement capabilities (magnetic fields and infrared, with specific emphasis on the new IRAS results), important classes of stars (F stars, M dwarfs and giants, and pre-main sequence stars), and interesting unanswered questions (the nature of nonthermal phenomena, heating processes, angular momentum evolution, and the existence and cause of the corona/wind dividing line). Each section is opened by two or more invited lectures aimed at a wide audience, including graduate students, and continues with some research papers. The proceedings also record the two general discussions on the role of magnetic fields in cool star atmospheres and the role of monitoring programs for studies of cool stars (see also Lecture Notes in Physics Vol. 292).
出版日期Conference proceedings 1987
關(guān)鍵詞Accretion; Libration; Main sequence; Redshift; Variation; chromosphere; evolution; magnetic field; magnetic
版次1
doihttps://doi.org/10.1007/3-540-18653-0
isbn_softcover978-3-662-14486-2
isbn_ebook978-3-540-48041-9Series ISSN 0075-8450 Series E-ISSN 1616-6361
issn_series 0075-8450
copyrightSpringer-Verlag Berlin Heidelberg 1987
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Control Objectives and Strategies,ds of two close companions may also be important. For evolved binaries the energy probably is mainly gravitational, coming from the transfer of matter onto a compact star..Whatever the basic energy source, some energy appears in the form of fast electrons that are capable of generating intense radio
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The relation between the CA II K line-core flux density and the magnetic flux density on the sun,
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Shifts of the circular zeeman profile in small solar fluxtubes,
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Results of a southern radio survey of active chromosphere stars,
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Control Objectives and Strategies,We derive and discuss relations between magnetic, X-ray, and Ca II H+K flux densities for a sample of G, K, and M dwarfs.
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