书目名称 | Solar Photosphere: Structure, Convection, and Magnetic Fields | 副标题 | Proceedings of the 1 | 编辑 | J. O. Stenflo | 视频video | | 丛书名称 | International Astronomical Union Symposia | 图书封面 |  | 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 | 关键词 | Main sequence; Photosphere; Sunspot; helioseismology; solar | 版次 | 1 | doi | https://doi.org/10.1007/978-94-009-1061-4 | isbn_softcover | 978-0-7923-0530-9 | isbn_ebook | 978-94-009-1061-4Series ISSN 1743-9213 Series E-ISSN 2352-2186 | issn_series | 1743-9213 | copyright | International Astronomical Union 1990 |
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书目名称Solar Photosphere: Structure, Convection, and Magnetic Fields被引频次 
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