Ab dem 31. Januar stellt buchhandel.de die Verkaufsfunktion ein!

Bitte sichern Sie alle notwendigen Daten, wie etwa Rechnungen oder Ihre Wunschliste in Ihrem Kundenprofil.
Weitere Informationen finden Sie hier: https://www.buchhandel.de/info/hilfe.
Suche ›

Jets From Young Stars III

Numerical MHD and Instabilities

Springer Berlin,
74,89 € Lieferbar in 5-7 Tagen
Dieses Produkt ist auch verfügbar als:


This volume contains the lecture notes of the Third JETSET School on Jets from Young Stars focusing on Numerical MHD and Instabilities. The book aims to demonstrate how to use the fundamental tools used in computational astrophysical jet research.


Titel: Jets From Young Stars III
Autoren/Herausgeber: Silvano Massaglia, Gianluigi Bodo, Andrea Mignone, Paola Rossi (Hrsg.)
Aus der Reihe: Lecture Notes in Physics
Ausgabe: Softcover reprint of hardcover 1st ed. 2008

ISBN/EAN: 9783642095672

Seitenzahl: 178
Format: 23,5 x 15,5 cm
Produktform: Taschenbuch/Softcover
Gewicht: 296 g
Sprache: Englisch

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.

buchhandel.de - Newsletter
Möchten Sie sich für den Newsletter anmelden?

Bitte geben Sie eine gültige E-Mail-Adresse ein.
Lieber nicht