| Date | Name | Institute | Reason
|
| 6/28/16 | Huchi Li <hcli@mail.sdu.edu.cn> | Shandong University | Study MHD
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| 6/28/16 | Gang Li <en-super@hotmail.com> | Peking University | Learn computational MHD
|
| 3/22/16 | Miguel Avillez <mavillez@uevora.pt> | University of Evora, Portugal | I would like to use learn the ASTROBEAR code and try to implement time-dependent ionisation structure following my previous work. I also would like to use the code in teaching courses on computational astrophysics.
|
| 2/23/16 | Gustavo <grsilva@princeton.edu> | Princeton University | Comparison between different codes
|
| 12/6/15 | Dominik Schleicher <dschleicher@astro-udec.cl> | Department of Astronomy, Universidad de Concepcion | Modeling of circumbinary disk formation (Master student project)
|
| 11/24/15 | WeiGang Zeng <cengwg14@mails.tsinghua.edu.cn> | Tsinghua University | For Fluid Dynamic simulation
|
| 10/30/15 | Dinh van Trung; dvtrung@iop.vast.ac.vn | Institute of Physics, Vietnam Academy of Science and Technology | I plan to simulate star and planet interaction
|
| 10/23/15 | Mariana Cecere | Instituto de Astronomía Teórica y Experimental CONICET-UNC Argentina | I am studying resistive MHD and would like to try to work with this code
|
| 6/1/15 | Carmen Tornow | Inst. of Planetary Research | protoplanetary disk evolution
|
disk formation from collapsing cloud core
| 2/2/15 | Frank Otto | The Chinese University of Hong Kong | Investigate star formation in molecular clouds
|
| 2/2/15 | Gustavo Salgado Enriquez | Universidad Complutense de Madrid | Study of wave structures and transport scheme
|
| 9/18/14 | Manuel | University of Birmingham | Research
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| 9/18/14 | Roberto Toscano-Fletes | Dep. Fisica UdeG, Universidad de Guadalajara, México | We try to use astrobear to model magnetohydrodynamic fluids in geophysical environments
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| 6/10/14 | Derek Mariscal | UCSD | Plasma jet calculations
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| 5/31/14 | Patrick Adams | University of Cape Town | MHD simulation of magnetic fields in astrophysical and cosmological contexts
|
| 5/30/14 | Bo Chai | Polar Research Institute of China | simulate jet in AGN
|
| 5/23/14 | Ruslan Gabb | Mexico, UAEH | teaching
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| 5/23/14 | Julio Valenzuela | UCSD | 2D counter-propagating plasma flows
|
| 5/23/14 | Dipanjan Mukherjee | Inter-University Centre for Astronomy and Astrophysics | AMR simulations of supernova driven outflows from galactic disks.
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| 5/13/14 | Shashi Kanbur | SUNY Oswego |
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| 5/8/14 | Laurence Sabin | Institute of Astronomy and Meteorology, University of Guadalajara | MHD modelling of evolved stars and comparison to observational data to understand the role played by magnetic fields (e.g. magnetic launching, Alfvén radius…etc).
|
| 5/6/14 | Lee Youngjun | Chung-Ang University | Plasma Theory and Nonlinear Dynamics Lab., Chung-Ang University, Seoul, Korea. I'm researching on hydrodynamics instability, especially occurs on 'fast ignition scheme'. (more specially, inertial confinement fusion) Although AstroBEAR used on astrophysical area, I think it is suitable on our researching area, studying on Rayleigh-Taylor instability, Kelvin-Helmholtz instability, so on. In this reason, we request AstroBEAR code to improve our researching.
|
| 5/6/14 | Laura Chajet | York University, Toronto | Modelling of outflows from quasar accretion disc
|
