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010   $a1-283-84954-2
010   $a3-642-32093-7
024 7 $a10.1007/978-3-642-32093-4
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035   $a(EBL)1030210
035   $a(OCoLC)820204661
035   $a(SSID)ssj0000797462
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035   $a(PQKBTitleCode)TC0000797462
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035   $a(DE-He213)978-3-642-32093-4
035   $a(MiAaPQ)EBC1030210
035   $a(PPN)168320975
035   $a(EXLCZ)992670000000279876
100   $a20121126d2013      uy         0
101 0 $aeng
135   $aur|n|---|||||
181   $ctxt
182   $cc
183   $acr
200 10$aSolar and stellar dynamos /$fPaul Charbonneau
205   $a1st ed. 2013.
210   $aBerlin $cSpringer$d2013
215   $a1 online resource (245 p.)
225 1 $aSaas-Fee advanced course,$x1861-7980 ;$v39
300   $aDescription based upon print version of record.
311   $a3-642-43047-3 
311   $a3-642-32092-9 
320   $aIncludes bibliographical references and index.
327   $a1 Magnetohydrodynamics -- 2 Decay and Amplification of Magnetic Fields -- 3 Dynamo Models of the Solar Cycle -- 4 Fluctuations, Intermittency and Predictivity -- 5 Stellar Dynamos -- A Useful Identities and Theorems from Vector Calculus -- B Coordinate Systems and the Fluid Equations -- C Physical and Astronomical Constants -- D Maxwell?s Equations and Physical Units -- Index.
330   $aAstrophysical dynamos are at the heart of cosmic magnetic fields of a wide range of scales, from planets and stars to entire galaxies. This book presents a thorough, step-by-step introduction to solar and stellar dynamos. Looking first at the ultimate origin of cosmic seed magnetic fields, the antagonists of field amplification are next considered: resistive decay, flux expulsion, and flows ruled out by anti-dynamo theorems. Two kinematic flows that can act as dynamos are then studied: the Roberts cell and the CP-flow. Mean-field electrodynamics and derivation of the mean-field dynamo equations lead to the alpha Omega-dynamo, the flux transport dynamo, and dynamos based on the Babcock-Leighton mechanism. Alternatives to the mean-field theory are also presented, as are global MHD dynamo simulations. Fluctuations and grand minima in the solar cycle are discussed in terms of dynamo modulations through stochastic forcing and nonlinear effects. The book concludes with an overview of the major challenges in understanding stellar magnetic fields and their evolution in terms of various dynamo models, global MHD simulations, and fossil fields. Each chapter is accompanied by an annotated bibliography, guiding the readers to the relevant technical literature, which may lead them to carry out their own research in the field of dynamo theory.
410  0$aSaas-Fee advanced course ... lecture notes ;$v39.
606   $aStars$xMagnetic fields
606   $aSolar oscillations
606   $aStellar oscillations
607   $aSun
615  0$aStars$xMagnetic fields.
615  0$aSolar oscillations.
615  0$aStellar oscillations.
676   $a538.72
700   $aCharbonneau$b Paul$0943541
712 02$aSchweizerische Gesellschaft fu?r Astrophysik und Astronomie.
801  0$bMiAaPQ
801  1$bMiAaPQ
801  2$bMiAaPQ
906   $aBOOK
912   $a9910438120603321
996   $aSolar and Stellar Dynamos$92129460
997   $aUNINA