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110906s2010 ne o 000 0 eng d |
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|a OPELS
|b eng
|e pn
|c OPELS
|d OCLCQ
|d OCLCF
|d OCLCQ
|d U3W
|d WYU
|d LEAUB
|d S2H
|d OCLCO
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|a 9780444528643
|q (electronic bk.)
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|a 0444528644
|q (electronic bk.)
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|a (OCoLC)749875923
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|a QC809.M35
|b H45 2010
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|a 551.514
|2 22
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|a Heikkila, Walter J.
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|a Earth's magnetosphere :
|b created by the low latitude boundary layer /
|c by W.J. Heikkila.
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|a Amsterdam ;
|a London :
|b Elsevier Science,
|c 2010.
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|a 1 online resource
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|a text
|b txt
|2 rdacontent
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|a computer
|b c
|2 rdamedia
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|a online resource
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|2 rdacarrier
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|a The author argues that, after four decades of debate about the interactive of solar wind with the magnetosphere, it is time to get back to basics. Starting with Newton's law, this book also examines Maxwell's equations and subsidiary equations such as continuity, constitutive relations and the Lorentz transformation; Helmholtz' theorem, and Poynting's theorem, among other methods for understanding this interaction. Includes chapters on prompt particle acceleration to high energies, plasma transfer event, and the low latitude boundary layer More than 200 figures illustrate the text Includes a color insert.
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|a Prologue -- 1. Historical Introduction -- 2. Approximate Methods -- 3. Helmholtz's Theorem -- 4. Poynting's Energy Conservation Theorem -- 5. Magnetopause -- 6. High Altitude Cusps -- 7. Low-Latitude Boundary Layer -- 7. Driving The Plasma Sheet -- 9. Magnetospheric Substorms -- 10. Epilogue.
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|a Magnetosphere.
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|a Magn�etosph�ere.
|0 (CaQQLa)201-0012439
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|a Magnetosphere
|2 fast
|0 (OCoLC)fst01005892
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|i Print version:
|a Heikkila, Walter J.
|t Earth's magnetosphere.
|d Amsterdam ; London : Elsevier Science, 2010
|z 9780444528643
|w (OCoLC)424556020
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856 |
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0 |
|u https://sciencedirect.uam.elogim.com/science/book/9780444528643
|z Texto completo
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