| 000 | 03074cam a2200649Ma 4500 | ||
|---|---|---|---|
| 001 | ocn859161179 | ||
| 003 | OCoLC | ||
| 005 | 20171106081405.0 | ||
| 006 | m o d | ||
| 007 | cr cn||||||||| | ||
| 008 | 130831s2013 gw ad ob 001 0 eng d | ||
| 020 |
_a9783527648924 _q(electronic bk.) |
||
| 020 |
_a3527648925 _q(electronic bk.) |
||
| 020 |
_a9783527648955 _q(electronic bk.) |
||
| 020 |
_a352764895X _q(electronic bk.) |
||
| 020 |
_a9783527648948 _q(electronic bk.) |
||
| 020 |
_a3527648941 _q(electronic bk.) |
||
| 020 | _a3527410341 | ||
| 020 | _a9783527410347 | ||
| 020 | _z9783527410347 | ||
| 028 | 0 | 1 |
_aEB00229306 _bRecorded Books |
| 029 | 1 |
_aAU@ _b000052185431 |
|
| 029 | 1 |
_aCHBIS _b010441920 |
|
| 029 | 1 |
_aCHVBK _b334089433 |
|
| 029 | 1 |
_aDEBBG _bBV041634208 |
|
| 029 | 1 |
_aDEBBG _bBV041829445 |
|
| 029 | 1 |
_aNLGGC _b370174194 |
|
| 029 | 1 |
_aNZ1 _b15340087 |
|
| 029 | 1 |
_aNZ1 _b15905461 |
|
| 035 |
_a(OCoLC)859161179 _z(OCoLC)883259803 _z(OCoLC)961667236 _z(OCoLC)962583594 |
||
| 040 |
_aE7B _beng _epn _cE7B _dOCLCO _dCUS _dCUI _dDG1 _dN$T _dYDXCP _dOCLCF _dRECBK _dOCLCQ _dCOO _dOCLCQ _dLOA |
||
| 049 | _aMAIN | ||
| 050 | 4 |
_aTK454.4.M3 _bR83 2013eb |
|
| 072 | 7 |
_aSCI _x004000 _2bisacsh |
|
| 082 | 0 | 4 |
_a523.0188 _223 |
| 100 | 1 |
_aRüdiger, G. _q(Günther) |
|
| 245 | 1 | 0 |
_aMagnetic processes in astrophysics : theory, simulations, experiments / _cGünther Rüdiger, Leonid L. Kitchatinov, and Rainer Hollerbach. _h[electronic resource] |
| 260 |
_aWeinheim, Germany : _bWiley-VCH, _c2013. |
||
| 300 |
_a1 online resource (x, 346 pages :) : _billustrations (some color) |
||
| 336 |
_atext _btxt _2rdacontent |
||
| 337 |
_acomputer _bc _2rdamedia |
||
| 338 |
_aonline resource _bcr _2rdacarrier |
||
| 504 | _aIncludes bibliographical references (pages 327-329) and index. | ||
| 520 | _aIn this work the authors draw upon their expertise in geophysical and astrophysical MHD to explore the motion of electrically conducting fluids, the so-called dynamo effect, and describe the similarities and differences between different magnetized objects. They also explain why magnetic fields are crucial to the formation of the stars, and discuss promising experiments currently being designed to investigate some of the relevant physics in the laboratory. This interdisciplinary approach will appeal to a wide audience in physics, astrophysics and geophysics. This second edition covers such additional topics as small-scale dynamos, while also presenting the latest results and experiments. | ||
| 588 | 0 | _aOnline resource; title from PDF title page (Wiley, viewed October 7, 2013). | |
| 650 | 0 | _aMagnetics. | |
| 650 | 0 | _aAstrophysics. | |
| 650 | 7 |
_aSCIENCE _xAstronomy. _2bisacsh |
|
| 650 | 7 |
_aAstrophysics. _2fast _0(OCoLC)fst00819797 |
|
| 650 | 7 |
_aMagnetics. _2fast _0(OCoLC)fst01005823 |
|
| 655 | 4 | _aElectronic books. | |
| 655 | 7 |
_aElectronic books. _2local |
|
| 700 | 1 | _aKitchatinov, Leonid L. | |
| 700 | 1 | _aHollerbach, Rainer. | |
| 856 | 4 | 0 |
_uhttp://onlinelibrary.wiley.com/book/10.1002/9783527648924 _zWiley Online Library |
| 942 |
_2ddc _cBK |
||
| 999 |
_c207007 _d207007 |
||