scholarly journals Benchmark numerical simulations of rarefied non-reacting gas flows using an open-source DSMC code

2015 ◽  
Vol 120 ◽  
pp. 140-157 ◽  
Author(s):  
Rodrigo C. Palharini ◽  
Craig White ◽  
Thomas J. Scanlon ◽  
Richard E. Brown ◽  
Matthew K. Borg ◽  
...  
Keyword(s):  
Numerical Simulations ◽  
Open Source ◽  
Gas Flows

scholarly journals An open source, parallel DSMC code for rarefied gas flows in arbitrary geometries

2010 ◽  
Vol 39 (10) ◽  
pp. 2078-2089 ◽  
Author(s):  
T.J. Scanlon ◽  
E. Roohi ◽  
C. White ◽  
M. Darbandi ◽  
J.M. Reese
Keyword(s):  
Open Source ◽  
Rarefied Gas ◽  
Gas Flows ◽  
Rarefied Gas Flows ◽  
Arbitrary Geometries

Numerical simulations of gas flows through an open, non-contact cell for LA-ICP-MS

2011 ◽  
Vol 26 (3) ◽  
pp. 631-634 ◽  
Author(s):  
Dhinesh Asogan ◽  
Barry L. Sharp ◽  
Ciaran J. P. O'Connor ◽  
Damon A. Green ◽  
Jay Wilkins
Keyword(s):  
Numerical Simulations ◽  
Gas Flows ◽  
Icp Ms

scholarly journals Numerical Simulations of Galactic Outflow and Inflow Phenomena

1991 ◽  
Vol 144 ◽  
pp. 407-416
Author(s):  
Kohji Tomisaka
Keyword(s):  
Numerical Simulations ◽  
Galactic Disk ◽  
Gas Flows ◽  
Polar Cap ◽  
Hot Gas ◽  
Numerical Studies ◽  
Dynamical Time ◽  
Density Scale ◽  
Velocity Cloud ◽  
High Velocity Cloud

The recent progress of numerical studies on outflow phenomena from the galactic disk to the halo is summarized. Firstly, a galactic-scale outflow is considered. If the high-velocity cloud is formed from the radiatively cooled gas, which was originally ejected from the disk as a hot gas, the temperature and density at the base of the halo should be ~ 106 K and 10–3 cm–3. Next, recent results of numerical simulations of the evolution of superbubbles, through which hot gas flows out to the halo, are reviewed. In the case of a thin disk whose density scale height is H ≃ 100 pc, the shell begins to be accelerated upwardly after several dynamical time scales. After that, the polar cap of the shell is broken and the hot gas flows away into the halo. In the case of a thick disk (H ≃ 500 pc) or a magnetized disk with a magnetic field parallel to the disk (B ≃ 5μG), the shell is not accelerated and never shows blow-out.

Numerical simulations of paper‐based electrophoretic separations with open‐source tools

2021 ◽  
Author(s):  
Gabriel S. Gerlero ◽  
Santiago Márquez Damián ◽  
Federico Schaumburg ◽  
Nicolás Franck ◽  
Pablo A. Kler
Keyword(s):  
Numerical Simulations ◽  
Open Source ◽  
Electrophoretic Separations
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