LEADER 03719nam 2200637Ia 450 001 9910140008103321 005 20200520144314.0 010 $a3-642-03370-9 024 7 $a10.1007/978-3-642-03370-4 035 $a(CKB)1000000000812911 035 $a(SSID)ssj0000372764 035 $a(PQKBManifestationID)11249424 035 $a(PQKBTitleCode)TC0000372764 035 $a(PQKBWorkID)10423206 035 $a(PQKB)10921386 035 $a(DE-He213)978-3-642-03370-4 035 $a(MiAaPQ)EBC3064730 035 $a(PPN)139962085 035 $a(EXLCZ)991000000000812911 100 $a20091103d2009 uy 0 101 0 $aeng 135 $aurnn|008mamaa 181 $ctxt 182 $cc 183 $acr 200 10$aJets from young stars V $ehigh performance computing and applications /$fJ. Gracia, F. De Colle, T. Downes (eds.) 210 $aBerlin ;$aLondon $cSpringer$dc2009 215 $a1 online resource (XI, 227 p. 88 illus.) 225 1 $aLecture notes in physics,$x0075-8450 ;$v791 300 $aBibliographic Level Mode of Issuance: Monograph 311 $a3-642-03369-5 320 $aIncludes bibliographical references and index. 327 $aI High Performance Computing -- to Message-Passing Interface -- An Introduction to Grid Computing Using EGEE -- AstroGrid and the Virtual Observatory -- II Applications in Astrophysics -- Three Dimensional Continuum Radiative Transfer -- Large-Scale Jet Simulations -- Modeling Accretion and Ejection Phenomena Around Young Stars: A Numerical Perspective -- Jet Stability: A Computational Survey -- Jets and Outflows from Collapsing Objects. 330 $aStudying the complex physical systems of stellar jets necessitates the incorporation of nonlinear effects which occur on a wide variety of length and timescales. One of the primary methods used to study the physics of jets is numerical simulations that apply high performance computing techniques. Such techniques are also required for analysing the huge modern astrophysical datasets. This book examines those computing techniques. It is a collection of the lectures from the fifth and final school of the JETSET network, "Jets From Young Stars V: High Performance Computing in Astrophysics." It begins with an introduction to parallel programming techniques, with an emphasis on Message Passing Interface (MPI), before it goes on to review grid technology techniques and offer a practical introduction to Virtual Observatory. The second half of the book, then, is devoted to applications of high performance computing techniques, including 3D radiation transfer, to jet and star formation processes. Aimed at graduate students in astrophysics, this book presents state-of-the-art methods, thereby offering interesting new insights to researchers in the field. 410 0$aLecture notes in physics ;$v791. 517 3 $aJets from young stars 5 517 3 $aJets from young stars five 606 $aAstrophysical jets$xMathematical models$vCongresses 606 $aStellar dynamics$vCongresses 606 $aMagnetohydrodynamic instabilities$vCongresses 615 0$aAstrophysical jets$xMathematical models 615 0$aStellar dynamics 615 0$aMagnetohydrodynamic instabilities 676 $a523.82 686 $aUD 8220$2rvk 701 $aGracia$b J$g(Jose)$01061819 701 $aDe Colle$b F$g(Fabio)$01061820 701 $aDownes$b T$g(Turlough)$01061821 712 12$aJETSET School on Jets from Young Stars : High Performance Computing in Astrophysics 801 0$bMiAaPQ 801 1$bMiAaPQ 801 2$bMiAaPQ 906 $aBOOK 912 $a9910140008103321 996 $aJets from young stars V$92520248 997 $aUNINA