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Titlebook: Magneto-Fluid Dynamics; Fundamentals and Cas Paul Lorrain,Fran?ois Lorrain,Stéphane Houle Book 20061st edition Springer-Verlag New York 200

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書目名稱Magneto-Fluid Dynamics
副標(biāo)題Fundamentals and Cas
編輯Paul Lorrain,Fran?ois Lorrain,Stéphane Houle
視頻videohttp://file.papertrans.cn/622/621408/621408.mp4
概述Provides an understanding of the physics at work in sunspots and solar coronal loops.This book provides a new approach to Magneto-Fluid-Dynamics (or Magneto-Hydro-Dynamics), mainly in two different wa
叢書名稱Astronomy and Astrophysics Library
圖書封面Titlebook: Magneto-Fluid Dynamics; Fundamentals and Cas Paul Lorrain,Fran?ois Lorrain,Stéphane Houle Book 20061st edition Springer-Verlag New York 200
描述Magnetohydrodynamics (MHD) concerns the interaction between magnetic fields and conducting fluids. We are concerned here with macroscopic inter- actions and, when the conducting fluid is a plasma, time scales are very much longer than the plasma period. Plasma periods vary widely, but are short, say 10~^^ second. We prefer the term Magneto-F/i^Z(i-Dynamics (MFD) because the disci- pline concerns mostly plasmas, various liquid conductors, and the liquid part of the Earth‘s core. It seems that the only applications of MFD to water are the induction of electric currents in the oceans by the Earth‘s magnetic field, and ship propulsion. But even MFD is not quite appropriate because that term also includes solid conductors that move in magnetic fields. This book is meant for graduate and upper-division undergraduate stu- dents in Physics, Geophysics, and Astrophysics, as well as for practicing sci- entists in these fields. This book is no more than a brief introduction to MFD because this vast subject is closely related to many others, namely Astrophysics, Elec- trodynamics, Fluid Dynamics, Geophysics, Oceanography, Plasma Physics, Thermonuclear Fusion, etc. We sketch the fundamentals, a
出版日期Book 20061st edition
關(guān)鍵詞CERN; Case; Dynamics; Fluid; Magneto Fluid Dynamics; Magneto Hydro Dynamics; Maxwell‘s equations; electric
版次1
doihttps://doi.org/10.1007/978-0-387-47290-4
isbn_softcover978-1-4419-2213-7
isbn_ebook978-0-387-47290-4Series ISSN 0941-7834 Series E-ISSN 2196-9698
issn_series 0941-7834
copyrightSpringer-Verlag New York 2006
The information of publication is updating

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Ohm’s Law for Moving Conductorslds sitting down with the conductor moving in front of you, or do you ride on the conductor with your measuring instruments? It is important to tell between the two points of view because the fields can be radically different. As a rule it is best to stand still, but not always. Chapters 6, 7, and 8
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Case Study: Sunspots spot of a given polarity is accompanied by one or more spots of the opposite polarity. But there are major differences: a) sunspots are larger than magnetic elements by an order of magnitude or more; b) sunspots are dark, while magnetic elements are bright; and c) the dark region of sunspots, calle
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Case Study: Solar Spiculesy? They seem to follow magnetic field lines, but they do not diverge on emerging from, or plunging into, the surface, where the magnetic field lines diverge rapidly. Also, they have a uniform diameter of about 150 to 200 kilometers, despite large changes in the ambient .. That does not make sense. A
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