Space Weather modeling

Density variations over B field lines and contours on the z=-20 plane

Density variations over B field lines during solar wind/Earth magnetosphere interaction (M.S. Yalim). For details on the MHD numerical solver see the JCP article [here] (http://www.sciencedirect.com/science/article/pii/S0021999111002592).

Plasma number density contours in the xz-plane at 3 instants during the 04/06/2000 geomagnetic storm

Plasma number density contours in x-z plane during 04/06/2000 geomagnetic storm (M.S. Yalim). This simulation uses real data from ACE satellite and can run on multiple GPUs (for details see CPC article here).

[WATCH FULL VIDEO here] (https://raw.githubusercontent.com/andrealani/COOLFluiD/master/videos/n.mp4)

The COOLFluiD team is involved and open to new collaborations in Horizon2020, ESA and other research projects dealing with complex multi-disciplinary problems and computational challenges.

Training sessions and consulting services can also be provided on demand.

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