Zobrazeno 1 - 10
of 200
pro vyhledávání: '"A. Löw-Baselli"'
A Hybrid Approach to Model the Drag-Flow Capacity of Co-Rotating Twin-Screw Extruder Kneading Blocks
Autor:
Roland, Wolfgang *, Stritzinger, Ursula, Albrecht, Hanny, Löw-Baselli, Bernhard, Berger-Weber, Gerald
Publikováno v:
In IFAC PapersOnLine 2022 55(20):121-126
Publikováno v:
New Astron. 34: 278-293, 2015
We have implemented open boundary conditions into the ANTARES code to increase the realism of our simulations of stellar surface convection. Even though we greatly benefit from the high accuracy of our fifth order numerical scheme (WENO5), the broade
Externí odkaz:
http://arxiv.org/abs/1305.0743
Autor:
Roland, Wolfgang, Marschik, Christian, Krieger, Michael, Löw-Baselli, Bernhard, Miethlinger, Jürgen
Publikováno v:
In Journal of Non-Newtonian Fluid Mechanics June 2019 268:12-29
Autor:
Luger, Hans-Jürgen, Löw-Baselli, Bernhard, Neunhäuserer, Andreas, Friesenbichler, Walter, Miethlinger, Jürgen
Publikováno v:
In Polymer Testing February 2019 73:104-114
Autor:
Happenhofer, Natalie, Grimm-Strele, Hannes, Kupka, Friedrich, Löw-Baselli, Bernhard, Muthsam, Herbert
Publikováno v:
Journal of Computational Physics, vol 236, 96-118 (2013)
In astrophysics and meteorology there exist numerous situations where flows exhibit small velocities compared to the sound speed. To overcome the stringent timestep restrictions posed by the predominantly used explicit methods for integration in time
Externí odkaz:
http://arxiv.org/abs/1112.3507
Publikováno v:
New Astron.15:460-475,2010
We discuss the general design of the ANTARES code which is intended for simulations in stellar hydrodynamics with radiative transfer and realistic microphysics in 1D, 2D and 3D. We then compare the quality of various numerical methods. We have applie
Externí odkaz:
http://arxiv.org/abs/0905.0177
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Using grid refinement, we have simulated solar granulation in 2D. The refined region measures 1.97*2.58 Mm (vertical*horizontal). Grid spacing there is 1.82*2.84 km. The downflows exhibit strong Kelvin-Helmholtz instabilities. Below the photosphere,
Externí odkaz:
http://arxiv.org/abs/0706.3349
Publikováno v:
In Journal of Non-Newtonian Fluid Mechanics October 2017 248:27-39
Autor:
Zacher, Maximilian, Roland, Wolfgang, Löw-Baselli, Bernhard, Berger-Weber, Gerald, Steinbichler, Georg
Publikováno v:
AIP Conference Proceedings; 2023, Vol. 2884 Issue 1, p1-5, 5p