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Titlebook: Energy Storage and Release through the Solar Activity Cycle; Models Meet Radio Ob Christophe Marqué,Alexander Nindos Book 2012 Springer Sci

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發(fā)表于 2025-3-21 19:35:52 | 只看該作者 |倒序瀏覽 |閱讀模式
書目名稱Energy Storage and Release through the Solar Activity Cycle
副標題Models Meet Radio Ob
編輯Christophe Marqué,Alexander Nindos
視頻videohttp://file.papertrans.cn/311/310424/310424.mp4
概述Provides an overview of recent research results in observational and theoretical solar radio physics.Focuses on solar eruptions, quiet Sun emission and fundamental radio physics
圖書封面Titlebook: Energy Storage and Release through the Solar Activity Cycle; Models Meet Radio Ob Christophe Marqué,Alexander Nindos Book 2012 Springer Sci
描述For nearly sixty years, radio observations have provided a unique insight into the physics of the active and quiescent solar atmosphere. Thanks to the variety of emission mechanisms and to the large altitude range available to observations, fundamental plasma parameters have been measured from the low chromosphere to the upper corona and interplanetary medium. .This book presents current research in solar radio astronomy and shows how well it fits in the exceptional scientific context brought by the current space solar observatories. It essentially contains contributed research and review papers presented during the 2010 Community of European Solar Radio Astronomers (CESRA) meeting, which took place in Belgium in June 2010. .This book is aimed at graduate students and researchers working in solar physics and space science. .Previously published in Solar Physics journal, Vol. 273/2, 2011.
出版日期Book 2012
關鍵詞CESRA Meeting Results; Coronal Shock Waves; Decimetric Pulsations; Fundamental Radio Physics; Magnetoaco
版次1
doihttps://doi.org/10.1007/978-1-4614-4403-9
isbn_softcover978-1-4899-9309-0
isbn_ebook978-1-4614-4403-9
copyrightSpringer Science+Business Media New York 2012
The information of publication is updating

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Coronal Shock Waves, EUV Waves, and Their Relation to CMEs. II. Modeling MHD Shock Wave Propagationof the modeling of the propagation of shock-associated extreme-ultraviolet (EUV) waves as well as Moreton waves along the solar surface in the simplest solar corona model. The calculations reveal deceleration and lengthening of the waves. In contrast, waves considered in the linear approximation keep their length unchanged and slightly accelerate.
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mission and fundamental radio physicsFor nearly sixty years, radio observations have provided a unique insight into the physics of the active and quiescent solar atmosphere. Thanks to the variety of emission mechanisms and to the large altitude range available to observations, fundamental plasma par
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James K. Whitesell,Mark A. Mintonof the modeling of the propagation of shock-associated extreme-ultraviolet (EUV) waves as well as Moreton waves along the solar surface in the simplest solar corona model. The calculations reveal deceleration and lengthening of the waves. In contrast, waves considered in the linear approximation keep their length unchanged and slightly accelerate.
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發(fā)表于 2025-3-23 01:12:52 | 只看該作者
https://doi.org/10.1007/978-3-662-10051-6nection between the parameters of the radio emission from three different layers of the solar atmosphere and the solar wind velocity near the Earth’s orbit was discovered. Such a connection is suggestive of a common mechanism of solar wind acceleration from chromospheric heights to the upper corona.
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