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Titlebook: Solar Photosphere: Structure, Convection, and Magnetic Fields; Proceedings of the 1 J. O. Stenflo Conference proceedings 1990 International

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書目名稱Solar Photosphere: Structure, Convection, and Magnetic Fields
副標題Proceedings of the 1
編輯J. O. Stenflo
視頻videohttp://file.papertrans.cn/872/871408/871408.mp4
叢書名稱International Astronomical Union Symposia
圖書封面Titlebook: Solar Photosphere: Structure, Convection, and Magnetic Fields; Proceedings of the 1 J. O. Stenflo Conference proceedings 1990 International
描述Solar and stellar photospheres constitute the layers most accessible to observations, forming the interface between the interior and the outside of the stars. The solar atmosphere is a rich physics laboratory, in which the whole spectrum of radiative, dynamical, and magnetic processes that tranfer energy into space can be observed. As the fundamental processes take place on very small spatial scales, we need high· resolution observations to explore them. On the other hand the small-scale processes act together to form global properties of the sun, which have their origins in the solar interior. The rapid advances in observational techniques and theoreticallllodelling over the past decade made it very timely to bring together scientists from east and west to the first lAU Symposium on this topic. The physics of the photosphere involves complicated interactions between magnetic fields, convection, waves, and radiation. During the past decade our understanding of these gener- ally small-scale structures and processes has been dramatically advanced. New instrumen- tations, on ground and in space, have given us new means to study the granular convection. Diagnostic methods in Stokes pol
出版日期Conference proceedings 1990
關鍵詞Main sequence; Photosphere; Sunspot; helioseismology; solar
版次1
doihttps://doi.org/10.1007/978-94-009-1061-4
isbn_softcover978-0-7923-0530-9
isbn_ebook978-94-009-1061-4Series ISSN 1743-9213 Series E-ISSN 2352-2186
issn_series 1743-9213
copyrightInternational Astronomical Union 1990
The information of publication is updating

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Temperature Diagnostics of the Upper Photospherethe upper photosphere, in the context of Avrett’s NLTE recovery of the LTE Holweger-Müller model below the temperature minimum and Ayres’ bifurcation into hot and cool components above the temperature minimum.
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Thermal Bifurcation Of the Outer PhotosphereThe degree of thermal heterogeneity at the base of the solar chromosphere is substantially beyond that simulated in the best-available multicomponent models; casting serious doubts on inferences drawn from them.
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Solar Photosphere: Structure, Convection, and Magnetic Fields978-94-009-1061-4Series ISSN 1743-9213 Series E-ISSN 2352-2186
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