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Titlebook: Solar Prominences; Jean-Claude Vial,Oddbj?rn Engvold Book 2015 Springer International Publishing Switzerland 2015 Coronagraphy.Images Sola

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發(fā)表于 2025-3-21 16:16:46 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書目名稱Solar Prominences
編輯Jean-Claude Vial,Oddbj?rn Engvold
視頻videohttp://file.papertrans.cn/872/871417/871417.mp4
概述Provides the latest research results on solar prominences, including discussions on chirality, fine structure and solar plasma physics.Presents a historical description of the developments in spectros
叢書名稱Astrophysics and Space Science Library
圖書封面Titlebook: Solar Prominences;  Jean-Claude Vial,Oddbj?rn Engvold Book 2015 Springer International Publishing Switzerland 2015 Coronagraphy.Images Sola
描述.This volume presents the latest research results on solar prominences, including new developments on e.g. chirality, fine structure, magnetism, diagnostic tools and relevant solar plasma physics..In 1875 solar prominences, as seen out of the solar limb, were described by P.A. Secchi in his book .Le Soleil. as "gigantic pink or peach-flower coloured flames". The development of spectroscopy, coronagraphy and polarimetry brought tremendous observational advances in the twentieth century. The authors present and discuss exciting new challenges (resulting from observations made by space and ground-based telescopes in the 1990s and the first decade of the 21.st. century) concerning the diagnostics of prominences, their formation, their life time and their eruption along with their impact in the heliosphere (including the Earth)..The book starts with a general introduction of the prominence “object” with some historical background on observations and instrumentation. In the next chapter, the various forms of prominences are described with a thorough attempt of classification. Their thermodynamic (and velocity) properties are then derived with emphasis on the methods (and their limits) us
出版日期Book 2015
關(guān)鍵詞Coronagraphy; Images Solar Eruptions; SDO Telescope; SOHO Telescope; STEREO Telescope; Solar Corona; Solar
版次1
doihttps://doi.org/10.1007/978-3-319-10416-4
isbn_softcover978-3-319-35703-4
isbn_ebook978-3-319-10416-4Series ISSN 0067-0057 Series E-ISSN 2214-7985
issn_series 0067-0057
copyrightSpringer International Publishing Switzerland 2015
The information of publication is updating

書目名稱Solar Prominences影響因子(影響力)




書目名稱Solar Prominences影響因子(影響力)學(xué)科排名




書目名稱Solar Prominences網(wǎng)絡(luò)公開度




書目名稱Solar Prominences網(wǎng)絡(luò)公開度學(xué)科排名




書目名稱Solar Prominences被引頻次




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發(fā)表于 2025-3-21 21:26:23 | 只看該作者
Description and Classification of Prominences,laments when seen against the solar disk. The aims of prominence classifications were from the start to establish references and frameworks for understanding the physical conditions for their formation and development through interplay with the solar magnetic environment. The multi-thermal nature of
板凳
發(fā)表于 2025-3-22 03:30:27 | 只看該作者
地板
發(fā)表于 2025-3-22 08:39:13 | 只看該作者
Derivations and Observations of Prominence Bulk Motions and Mass,essential to development and testing of models discussed throughout this book. Prominence flows are complex and various, ranging from the relatively linear flows along prominence spines to the complex, turbulent patterns exhibited by hedgerow prominences. Techniques for measuring flows include time
5#
發(fā)表于 2025-3-22 12:19:39 | 只看該作者
Radiative Transfer in Solar Prominences,. Solar prominences are low-density structures and, therefore, the non-equilibrium (NLTE) spectroscopy tools have to be used. We describe the basics of the NLTE radiative-transfer theory applied to typical prominence conditions and demonstrate why the NLTE approach is necessary. Starting from the si
6#
發(fā)表于 2025-3-22 13:32:36 | 只看該作者
Derivation of the Major Properties of Prominences Using NLTE Modelling,he prominences and their fine-structures are presented. Modelling the radiative transfer processes out of local thermodynamic equilibrium allows one to retrieve the prominence plasma parameters (temperature, density, pressure, ionisation degree) as well as the prominence’s mass.
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發(fā)表于 2025-3-22 20:08:48 | 只看該作者
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發(fā)表于 2025-3-22 23:46:46 | 只看該作者
Magnetometry of Prominences,ization emitted by He atoms in the presence of magnetic fields. The relatively weak magnetic fields expected in prominences require taking into consideration a long series of quantum coherences between the atomic levels of the He atom, coherences that are critical for the sensitivity of the emitted
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發(fā)表于 2025-3-23 01:34:33 | 只看該作者
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