US / RUSSIA collaboration in plasma astrophysics

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Support

The collaboration was started in 1990 and was supported by 

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ATP NASA grant NNX08AH25G (2009-2011)
"3D MHD Simulations of QPOs in LMXBs and Cataclysmic Variables"

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NSF grant AST-0807129 (2009-2011)
"Variability of Accreting Magnetized Stars Studied with 3D MHD
Simulations and 3D Radiative Transfer"

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NSF grant AST-0607135 (2006-2009)
"Accretion and Outflows of Rotating Magnetized Stars"

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NASA grant NNG05GL49G (2005-2008)
"Magnetic Effects on the Giant Planets"

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NASA grant NAG5-13220 (2003-2006)
"Dynamics of Protoplanetary Disks Around Magnetized Stars"

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NASA LTSA grant (2003-2007)
"Probing of Accretion and Outflow in Classical T Tauri Stars: Comparison of HST and FUSE UV Spectra with 3D Simulations" ,

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NSF grant  (2003-2005)
"Disk and Wind Accretion to Magnetized Stars",

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NASA grant:  NAG5 - 9735 (2000 - 2003), 
"Magnetohydrodynamics and Plasma Phenomena in Protostellar Systems" 

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ATP NASA grant: NAG5 - 9047 (1999 - 2002), 
"Accretion to Magnetized Rotating Neutron Stars" 

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NSF grant: NSF AST - 9986936 (1999 - 2002), 
"Disk and Wind Accretion to Magnetized Neutron Stars" 

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NSF POWRE grant (to Dr. Romanova): NSF AST - 9973366 (1999 - 2000), 
"POWRE: Accretion to Rotating Magnetized Stars" 

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The CRDF grant  RP1-173 (1996 - 1998) 
"Magneto-Rotational Phenomena in Astrophysics",

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An NSF grant (1994 - 1998), 

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The Soros Foundation (1991 - 1992), 

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An ESO grant (1990 - 1991), 

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The Russian program RFFI:  99-02-18180 (1999 - 2001), 

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The Russian Ministry of Science grants (Astronomy program).

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NASA High-End Computing (HEC)
Program through the NASA Advanced Supercomputing (NAS) Division at Ames Research Center and the NASA Center for Computational Sciences (NCCS) at Goddard Space Flight Center.

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Hewitt Undergraduate Computing and Visualization Laboratory

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Velocity Cluster of the Cornell Theory Center


created by O. Toropina, 2000-2004 Your comments are welcome
2000-2011, last updated on 19.03.11