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Titlebook: Coronal Magnetometry; Steven Tomczyk,Jie Zhang,Timothy Bastian Book 2014 Springer Science+Business Media New York 2014 Embedded Systems.Ha

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發(fā)表于 2025-3-21 16:05:49 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書(shū)目名稱(chēng)Coronal Magnetometry
編輯Steven Tomczyk,Jie Zhang,Timothy Bastian
視頻videohttp://file.papertrans.cn/239/238293/238293.mp4
概述Captures advances being made in the field of coronal magnetism, from theory to observations and instrumentation.Includes a collection of papers on coronal magnetism from the Workshop: Coronal Magnetis
圖書(shū)封面Titlebook: Coronal Magnetometry;  Steven Tomczyk,Jie Zhang,Timothy Bastian Book 2014 Springer Science+Business Media New York 2014 Embedded Systems.Ha
描述.Captures advances being made in the field of coronal magnetism, from theory to observations and instrumentation..This volume is a collection of research articles on the subject of the solar corona, and particularly, coronal magnetism. The book was motivated by the Workshop on Coronal Magnetism: Connecting Models to Data and the Corona to the Earth, which was held 21 - 23 May 2012 in Boulder, Colorado, USA. This workshop was attended by approximately 60 researchers. Articles from this meeting are contained in this topical issue, but the topical issue also contains contributions from researchers not present at the workshop..This volume is aimed at researchers and graduate students active in solar physics..Originally published in .Solar Physics., Vol. 288, Issue 2, 2013 and Vol. 289, Issue 8, 2014..
出版日期Book 2014
關(guān)鍵詞Embedded Systems; Hardware Security and Trust; Integrated Circuit Design; Secure Embedded Systems; Secur
版次1
doihttps://doi.org/10.1007/978-1-4939-2038-9
isbn_softcover978-1-4939-4983-0
isbn_ebook978-1-4939-2038-9
copyrightSpringer Science+Business Media New York 2014
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978-1-4939-4983-0Springer Science+Business Media New York 2014
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發(fā)表于 2025-3-22 01:14:18 | 只看該作者
Transactional Aspects of Workflows, in both the global magnetic-field evolution over a solar cycle, and the local storage of magnetic free energy within coronal plasmas. We address commonly held skepticisms concerning angular ambiguities and line-of-sight confusion. We argue that ambiguities are, in principle, no worse than more fami
地板
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Micronutrients and Other Trace Elements,r atmosphere has been an important task over the past decades. This task has been made complicated by the difficulties to measure the magnetic field in the corona, while it is currently known with a good accuracy in the photosphere and/or chromosphere. Thus, to determine the coronal magnetic field,
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Pseudospectral and Galerkin Methodsty to probe the plasma parameters of the solar atmosphere. Here, high-cadence observations of two “EIT wave” events taken using the . (AIA) instrument onboard the . (SDO) are combined with spectroscopic measurements from the . (EIS) onboard the . spacecraft and used to examine the variability of the
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Mathematics and Its Applications. onboard the .. Three minutes after the start of a C2.0 flare, wave trains were first observed along an open divergent loop system in 171?? observations at a distance of 150 Mm from the footpoint of the guiding loop system and with a speed of 689?km?s., then they appeared in 193?? observations afte
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International Regulatory Environment, cavities are elliptical regions of rarefied density lying above and around prominences. They can be long-lived (weeks to months) but are often observed to eventually erupt as part of a coronal mass ejection (CME). We determine morphological properties of the cavities both by qualitatively assessing
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