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Titlebook: New Millennium Solar Physics; Markus J. Aschwanden Book 2019 Springer Nature Switzerland AG 2019 Data Processing Methods.Models of Physica

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發(fā)表于 2025-3-21 18:31:25 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書(shū)目名稱(chēng)New Millennium Solar Physics
編輯Markus J. Aschwanden
視頻videohttp://file.papertrans.cn/666/665503/665503.mp4
概述Presents an update of solar research in the new millennium during 2000-2018, complementing the previous successful solar corona textbook in theory and observations.Describes new research results in so
叢書(shū)名稱(chēng)Astrophysics and Space Science Library
圖書(shū)封面Titlebook: New Millennium Solar Physics; Markus J. Aschwanden Book 2019 Springer Nature Switzerland AG 2019 Data Processing Methods.Models of Physica
描述.This is a follow-on book to the introductory textbook "Physics of the Solar Corona" previously published in 2004 by the same author, which provided a systematic introduction and covered mostly scientific results from the pre-2000 era. Using a similar structure as the previous book the second volume provides a seamless continuation of numerous novel research results in solar physics that emerged in the new millennium (after 2000) from the new solar missions of RHESSI, STEREO, Hinode, CORONAS, and the Solar Dynamics Observatory (SDO) during the era of 2000-2018. The new solar space missions are characterized by unprecedented high-resolution imaging, time resolution, spectral capabilities, stereoscopy and tomography, which reveal the intricate dynamics of magneto-hydrodynamic processes in the solar corona down to scales of 100 km. The enormous amount of data streaming down from SDO in Terabytes per day requires advanced automated data processing methods. The book focuses exclusively onnew research results after 2000, which are reviewed in a comprehensive manner, documented by over 3600 literature references, covering theory, observations, and numerical modeling of basic physical proc
出版日期Book 2019
關(guān)鍵詞Data Processing Methods; Models of Physical Processes in High-temperature Plasmas; RHESSI, STEREO, Hin
版次1
doihttps://doi.org/10.1007/978-3-030-13956-8
isbn_ebook978-3-030-13956-8Series ISSN 0067-0057 Series E-ISSN 2214-7985
issn_series 0067-0057
copyrightSpringer Nature Switzerland AG 2019
The information of publication is updating

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The Photosphere and Sunspots,lio et al. .), which amounts to a relative accuracy of ..∕.?≈?0.0007. Space-based observations are considered to be more accurate than ground-based measurements, which are impacted by the seeing through the Earth atmosphere.
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發(fā)表于 2025-3-22 00:41:55 | 只看該作者
The Quiet-Sun Corona,plore the electron density, temperature, thermodynamics, and related fundamental physics (Habbal et al. ., ., .). In the past, solar eclipse observations were leading to fundamental tests of Einstein’s theory of special relativity, by Sir Arthur Eddington in 1919, and to the discovery of coronal hol
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Coronal Loops,nifestations of closed magnetic field lines. The magnetic field is not directly visible in any wavelength, but our knowledge of its topology and geometry is based on our understanding that some field-aligned coronal structures become filled with hot plasma that radiates in EUV and soft X-rays, and t
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發(fā)表于 2025-3-22 18:57:47 | 只看該作者
Coronal Loop Oscillations and Waves,ast kink-mode waves (Aschwanden et al. .; Nakariakov et al. .), although the theoretical framework of MHD waves (including fast kink modes, fast sausage modes, and slow magneto-acoustic waves) has been developed and applied to solar (non-imaging) data at least two decades earlier (see reviews in Rob
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發(fā)表于 2025-3-22 21:23:48 | 只看該作者
Filaments and Prominences,l line in active regions and often represent progenitors of CMEs. What mainly distinguishes filaments from ordinary coronal loops or flux tubes is that their temperature is much cooler, and their density is much higher than the surrounding corona, and thus they are likely to be fed by upflows of hea
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發(fā)表于 2025-3-23 08:29:20 | 只看該作者
fels?ure- oder Salpeters?ureherstellung ) zu unterteilen sind. Bei den hier ausschlie?lich betrachteten Verbrennungsprozessen entstehen aus den Brenn- und Kraftstoffen und der Verbrennungsluft neben der W?rmeenergie feste und gasf?rmige Abfallprodukte. Die Abgase — bei festen und flüssigen Brennstof
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