It is aim of this work to develop, implement, and apply a new numerical scheme for modeling turbulent, multiphase astrophysical flows such as galaxy cluster cores and star forming regions. The method combines the capabilities of adaptive mesh refinement (AMR) and large-eddy simulations (LES) to capture localized features and to represent unresolved turbulence, respectively; it will be referred to as Fluid mEchanics with Adaptively Refined Large-Eddy SimulationS or FEARLESS. / Ziel dieser Arbeit war, ein neues numerisches Modell zu entwickeln, welches es ermöglicht Grobstruktursimulationen auch mit adaptiven Gittercodes auszuführen, um Turbulenz über große Längenskalenbereiche konsistent zu simulieren.
| Identifer | oai:union.ndltd.org:uni-wuerzburg.de/oai:opus.bibliothek.uni-wuerzburg.de:2643 |
| Date | January 2008 |
| Creators | Maier, Andreas |
| Source Sets | University of Würzburg |
| Language | English |
| Detected Language | English |
| Type | doctoralthesis, doc-type:doctoralThesis |
| Format | application/pdf |
| Rights | info:eu-repo/semantics/openAccess |
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