Flow around car.

Image Credits:
Renato N. Elias, Associate Researcher at the CFD Group from NACAD/COPPE/UFRJ
Rio de Janeiro, Brazil

The magnetic jet from a young stellar object rams into the magnetized molecular cloud from which the star is born by collapse. Isocontours of log10(density) are shown within an AMR structure. Data simulation by Rolf Walder and Doris Folini with the A-MAZE code.

Image Credits:
Swiss National Supercomputing Centre

Lox

Image Credits:
Kitware, Inc.

...

Image Credits:
Kitware, Inc.

Asteroid colliding with a planet.

Image Credits:
ChomboVis, Lawrence Berkeley Laboratory

Asteroid colliding with a planet.

Image Credits:
ChomboVis, Lawrence Berkeley Laboratory

A DNS simulation of a planar jet, using a 512x512x128 grid. They are Vorticity norm isosurfaces colored by positive Q criterium.

Image Credits:
Ricardo Reis, LASEF/IST
Lisboa, Portugal
www.lasef.ist.utl.pt 

Delta Wing

Image Credits:
Chris Rumsey

A DNS simulation of a planar jet, using a 512x512x128 grid.
They are Vorticity norm isosurfaces colored by positive Q criterium.

Image Credits:
Ricardo Reis, LASEF/IST
Lisboa, Portugal
www.lasef.ist.utl.pt 

Instability

Image Credits:
Renato N. Elias, Associate Researcher at the CFD Group from NACAD/COPPE/UFRJ
Rio de Janeiro, Brazil

Vortex Shedding

Image Credits:
Renato N. Elias, Associate Researcher at the CFD Group from NACAD/COPPE/UFRJ
Rio de Janeiro, Brazil

Dambreak wave interacting with a square cylinder.

Image Credits:
Renato N. Elias, Associate Researcher at the CFD Group from NACAD/COPPE/UFRJ
Rio de Janeiro, Brazil

ZSU23-4 Russian Anti-Aircraft vehicle being hit by a planar wave. 2.5 billion cell calculation.

Image Credits:
Jerry Clarke (US Army Research Laboratory)

2d density (log-scale) in an AMR simulation of colliding winds by Rolf Walder and Doris Folini.

Image Credits:
Visualization by Jean M. Favre