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Published by Springer, Berlin, 2010
ISBN 10: 3540769668ISBN 13: 9783540769668
Seller: Research Ink, Takoma Park, MD, U.S.A.
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Published by Springer, 2008
ISBN 10: 3540769668ISBN 13: 9783540769668
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Published by Routledge, 1998
ISBN 10: 9056996371ISBN 13: 9789056996376
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Published by Kluwer Academic, Dordrecht, 2005
ISBN 10: 1402000928ISBN 13: 9781402000928
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Cloth. Condition: Fine. 269 pp. Tightly bound. Corners not bumped. Text is Free of Markings.
Published by Springer, 2008
ISBN 10: 3540769668ISBN 13: 9783540769668
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Published by Gordon & Breach Science Publishers, Amsterdam, 1998
ISBN 10: 9056996371ISBN 13: 9789056996376
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ISBN 10: 3540769668ISBN 13: 9783540769668
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Published by Springer, 2008
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Published by Springer 8/19/2008, 2008
ISBN 10: 3540769668ISBN 13: 9783540769668
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Hardback or Cased Book. Condition: New. Jets from Young Stars III: Numerical Mhd and Instabilities 0.9. Book.
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ISBN 10: 3540769668ISBN 13: 9783540769668
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Published by Springer, 2008
ISBN 10: 3540769668ISBN 13: 9783540769668
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Published by Springer, 2008
ISBN 10: 3540769668ISBN 13: 9783540769668
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Published by Springer, 2008
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Published by Springer, 2008
ISBN 10: 3540769668ISBN 13: 9783540769668
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Published by Springer Berlin Heidelberg Aug 2008, 2008
ISBN 10: 3540769668ISBN 13: 9783540769668
Seller: BuchWeltWeit Ludwig Meier e.K., Bergisch Gladbach, Germany
Book Print on Demand
Buch. Condition: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -The study of the mechanisms that govern origin and propagation of stellar jets involves the treatment of many concurrent physical processes such as gravitation, hydrodynamics and magnetohydrodynamics, atomic physics and radiation. In the past years, an intensive work has been done looking for so- tions of the ideal MHD equations in the steady state limit as well as studying the stability of out ows in the linear regime. These kind, of approaches have provided a contribution to the understanding of jets that can hardly be ov- estimated. However, the extension of the analyses to the time-dependent and nonlinear regimes could not be avoided, and the MHD numerical simulations were the only mean to achieve this goal. Intherecentyears,considerableprogresseshavebeenmadebythecom- tational uiddynamiccommunityinthedevelopmentofnumericaltechniques, theso-calledhighresolutionshockcapturingschemes,wellsuitedforthetre- ment of supersonic ows with discontinuities. The numerical simulations of astrophysical jets took advantage of these developments; however new physics needed to be incorporated, such as magnetic eld e ects, radiation losses by diluted gases, and proper astrophysics environments. These needs led to the nontrivial extension of the methods devised for the Euler equations of g- dynamics to the magneto-hydrodynamical system. On the other hand, the possibility of carrying out numerical calculations has been greatly facilitated bytheavailability, ononehand,ofpowerfulsupercomputersand,ontheother hand, of fast processors at low cost. Large scale 3D simulations of jets at high resolution are now possible thanks to supercomputers, but also high reso- tion 2D MHD simulations can be performed routinely on desktop computers. 188 pp. Englisch.
Published by Springer Berlin Heidelberg Nov 2010, 2010
ISBN 10: 3642095674ISBN 13: 9783642095672
Seller: BuchWeltWeit Ludwig Meier e.K., Bergisch Gladbach, Germany
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Taschenbuch. Condition: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -The study of the mechanisms that govern origin and propagation of stellar jets involves the treatment of many concurrent physical processes such as gravitation, hydrodynamics and magnetohydrodynamics, atomic physics and radiation. In the past years, an intensive work has been done looking for so- tions of the ideal MHD equations in the steady state limit as well as studying the stability of out ows in the linear regime. These kind, of approaches have provided a contribution to the understanding of jets that can hardly be ov- estimated. However, the extension of the analyses to the time-dependent and nonlinear regimes could not be avoided, and the MHD numerical simulations were the only mean to achieve this goal. Intherecentyears,considerableprogresseshavebeenmadebythecom- tational uiddynamiccommunityinthedevelopmentofnumericaltechniques, theso-calledhighresolutionshockcapturingschemes,wellsuitedforthetre- ment of supersonic ows with discontinuities. The numerical simulations of astrophysical jets took advantage of these developments; however new physics needed to be incorporated, such as magnetic eld e ects, radiation losses by diluted gases, and proper astrophysics environments. These needs led to the nontrivial extension of the methods devised for the Euler equations of g- dynamics to the magneto-hydrodynamical system. On the other hand, the possibility of carrying out numerical calculations has been greatly facilitated bytheavailability, ononehand,ofpowerfulsupercomputersand,ontheother hand, of fast processors at low cost. Large scale 3D simulations of jets at high resolution are now possible thanks to supercomputers, but also high reso- tion 2D MHD simulations can be performed routinely on desktop computers. 188 pp. Englisch.
Published by Kluwer Academic Publishers, 2005
ISBN 10: 1402000928ISBN 13: 9781402000928
Seller: Romtrade Corp., STERLING HEIGHTS, MI, U.S.A.
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Condition: New. Brand New Original US Edition.We Ship to PO BOX Address also. EXPEDITED shipping option also available for faster delivery.This item may ship from the US or other locations in India depending on your location and availability.
Published by Kluwer Academic Publishers, 2005
ISBN 10: 1402000928ISBN 13: 9781402000928
Seller: SMASS Sellers, IRVING, TX, U.S.A.
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Condition: New. Brand New Original US Edition. Customer service! Satisfaction Guaranteed. This item may ship from the US or our Overseas warehouse depending on your location and stock availability. We Ship to PO BOX Location also.
Published by Springer Berlin Heidelberg, 2010
ISBN 10: 3642095674ISBN 13: 9783642095672
Seller: AHA-BUCH GmbH, Einbeck, Germany
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Taschenbuch. Condition: Neu. Druck auf Anfrage Neuware - Printed after ordering - The study of the mechanisms that govern origin and propagation of stellar jets involves the treatment of many concurrent physical processes such as gravitation, hydrodynamics and magnetohydrodynamics, atomic physics and radiation. In the past years, an intensive work has been done looking for so- tions of the ideal MHD equations in the steady state limit as well as studying the stability of out ows in the linear regime. These kind, of approaches have provided a contribution to the understanding of jets that can hardly be ov- estimated. However, the extension of the analyses to the time-dependent and nonlinear regimes could not be avoided, and the MHD numerical simulations were the only mean to achieve this goal. Intherecentyears,considerableprogresseshavebeenmadebythecom- tational uiddynamiccommunityinthedevelopmentofnumericaltechniques, theso-calledhighresolutionshockcapturingschemes,wellsuitedforthetre- ment of supersonic ows with discontinuities. The numerical simulations of astrophysical jets took advantage of these developments; however new physics needed to be incorporated, such as magnetic eld e ects, radiation losses by diluted gases, and proper astrophysics environments. These needs led to the nontrivial extension of the methods devised for the Euler equations of g- dynamics to the magneto-hydrodynamical system. On the other hand, the possibility of carrying out numerical calculations has been greatly facilitated bytheavailability, ononehand,ofpowerfulsupercomputersand,ontheother hand, of fast processors at low cost. Large scale 3D simulations of jets at high resolution are now possible thanks to supercomputers, but also high reso- tion 2D MHD simulations can be performed routinely on desktop computers.