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Titlebook: Solar Flare Magnetic Fields and Plasmas; Yuhong Fan,George Fisher Book 2012 Springer Science+Business Media New York 2012 Coronal Mass Eje

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書目名稱Solar Flare Magnetic Fields and Plasmas
編輯Yuhong Fan,George Fisher
視頻videohttp://file.papertrans.cn/872/871386/871386.mp4
概述Presents new and unique applications of vector magnetogram observations for understanding energy transport and transient forces that occur during solar flares.Includes unique new observations of stell
圖書封面Titlebook: Solar Flare Magnetic Fields and Plasmas; Yuhong Fan,George Fisher Book 2012 Springer Science+Business Media New York 2012 Coronal Mass Eje
描述This volume is devoted to the dynamics and diagnostics of solar magnetic fields and plasmas in the Sun’s atmosphere. Five broad areas of current research in Solar Physics are presented: (1) New techniques for incorporating radiation transfer effects into three-dimensional magnetohydrodynamic models of the solar interior and atmosphere, (2) The connection between observed radiation processes occurring during flares and the underlying flare energy release and transport mechanisms, (3) The global balance of forces and momenta that occur during flares, (4) The data-analysis and theoretical tools needed to understand and assimilate vector magnetogram observations and (5) Connecting flare and CME phenomena to the topological properties of the magnetic field in the Solar Atmosphere. The role of the Sun’s magnetic field is a major emphasis of this book, which was inspired by a workshop honoring Richard C. (Dick) Canfield.? Dick has been making profound contributions to these areas of research over a long and productive scientific career.? Many of the articles in this topical issue were first presented as talks during this workshop and represent substantial original work.? The workshop was
出版日期Book 2012
關(guān)鍵詞Coronal Mass Ejections; Dick Canfield Research; Magneto-Hydrodynamics; Solar Flares Research; Solar Magn
版次1
doihttps://doi.org/10.1007/978-1-4614-3761-1
isbn_softcover978-1-4899-9915-3
isbn_ebook978-1-4614-3761-1
copyrightSpringer Science+Business Media New York 2012
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Modeling and Interpreting the Effects of Spatial Resolution on Solar Magnetic Field Maps,closer to the line of sight. Further-derived quantities such as vertical current density show variations even in areas of high average magnetic fill fraction. In short, unresolved maps fail to represent the distribution of the underlying unresolved fields, and the “post-facto” methods generally do n
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