LEADER 04417nam 22006495 450 001 9910254630403321 005 20200706155721.0 010 $a1-4939-3164-4 024 7 $a10.1007/978-1-4939-3164-4 035 $a(CKB)3710000000718056 035 $a(DE-He213)978-1-4939-3164-4 035 $a(MiAaPQ)EBC6315393 035 $a(MiAaPQ)EBC5596365 035 $a(Au-PeEL)EBL5596365 035 $a(OCoLC)949903013 035 $a(PPN)194074129 035 $a(EXLCZ)993710000000718056 100 $a20160511d2016 u| 0 101 0 $aeng 135 $aurnn|008mamaa 181 $ctxt$2rdacontent 182 $cc$2rdamedia 183 $acr$2rdacarrier 200 10$aModern Fluid Dynamics for Physics and Astrophysics /$fby Oded Regev, Orkan M. Umurhan, Philip A. Yecko 205 $a1st ed. 2016. 210 1$aNew York, NY :$cSpringer New York :$cImprint: Springer,$d2016. 215 $a1 online resource (XXIII, 680 p. 111 illus., 16 illus. in color.) 225 1 $aGraduate Texts in Physics,$x1868-4513 311 08$a1-4939-3163-6 327 $aFundamentals -- Special flows and their properties -- Rotating flows -- Shallow water theory and incompressible waves -- Effects of compressibility sound and shock waves -- Stability and transition -- Rudiments of turbulence -- Equations of magnetohydrodynamics -- Magnetohydrodynamical Phenomena -- Numerical methods and caveats. . 330 $aThis book grew out of the need to provide students with a solid introduction to modern fluid dynamics. It offers a broad grounding in the underlying principles and techniques used, with some emphasis on applications in astrophysics and planetary science. The book comprehensively covers recent developments, methods and techniques, including, for example, new ideas on transitions to turbulence (via transiently growing stable linear modes), new approaches to turbulence (which remains the enigma of fluid dynamics), and the use of asymptotic approximation methods, which can give analytical or semi-analytical results and complement fully numerical treatments. The authors also briefly discuss some important considerations to be taken into account when developing a numerical code for computer simulation of fluid flows. Although the text is populated throughout with examples and problems from the field of astrophysics and planetary science, the text is eminently suitable as a general introduction to fluid dynamics. It is assumed that the readers are mathematically equipped with a reasonable knowledge in analysis, including basics of ordinary and partial differential equations and a good command of vector calculus and linear algebra. Each chapter concludes with bibliographical notes in which the authors briefly discuss the chapter's essential literature and give recommendations for further, deeper reading. Included in each chapter are a number of problems, some of them relevant to astrophysics and planetary science. The book is written for advanced undergraduate and graduate students, but will also prove a valuable source of reference for established researchers. . 410 0$aGraduate Texts in Physics,$x1868-4513 606 $aAstronomy 606 $aAstrophysics 606 $aMechanics 606 $aMathematical physics 606 $aAstronomy, Astrophysics and Cosmology$3https://scigraph.springernature.com/ontologies/product-market-codes/P22006 606 $aClassical Mechanics$3https://scigraph.springernature.com/ontologies/product-market-codes/P21018 606 $aTheoretical, Mathematical and Computational Physics$3https://scigraph.springernature.com/ontologies/product-market-codes/P19005 615 0$aAstronomy. 615 0$aAstrophysics. 615 0$aMechanics. 615 0$aMathematical physics. 615 14$aAstronomy, Astrophysics and Cosmology. 615 24$aClassical Mechanics. 615 24$aTheoretical, Mathematical and Computational Physics. 676 $a532.05 700 $aRegev$b Oded$4aut$4http://id.loc.gov/vocabulary/relators/aut$0815573 702 $aUmurhan$b Orkan M$4aut$4http://id.loc.gov/vocabulary/relators/aut 702 $aYecko$b Philip A$4aut$4http://id.loc.gov/vocabulary/relators/aut 801 0$bMiAaPQ 801 1$bMiAaPQ 801 2$bMiAaPQ 906 $aBOOK 912 $a9910254630403321 996 $aModern Fluid Dynamics for Physics and Astrophysics$92523009 997 $aUNINA