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Committee for cooperation of the Czech Republic with Joint Institute for Nuclear Research Login
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COMMITTEE
The main task of the Committee is organization of scientific cooperation between czech research and academic institutions and JINR.

Members of the Committee:

Bartova Eva (IBP ASCR)
Burdik Cestmir (FNSPE CTU)
Davidkova Marie (INP ASCR)
Dobes Jan (INP ASCR, Chairman of the Committee for cooperation of the Czech Republic with JINR)
Hedbavny Pavel (Czech Vacuum Society)
Chudoba Vratislav (Head of the national group of the CR in JINR)
Jancik Petr (FMST VSB-TUO)
Janosec Jiri (TC ASCR)
Jirak Zdenek (IP ASCR)
Katovsky Karel (FEEC BUT)
Kvasil Jan (FMP CU)
Leitner Rupert (MFF CUNI,Chairman of the Committee for cooperation of the Czech Republic with CERN)
Lidl Vaclav (MPO CR)
Maslan Miroslav (FoS UP)
Pospisil Stanislav (IEAP CTU, Member of the JINR Scientific Council)
Prasil Jan (MPO CR)
Rod Frantisek (MF CR)
Skoda Radek (FEE UWB)
Stekl Ivan (IEAP CTU, Vice-chairman of the Committee for cooperation of the Czech Republic with JINR)
Tursunov Arman (FPS SUO)
Vratislav Stanislav (FNSPE CTU)
Vysinka Marek (Plenipotentiary of the Government of the Czech Republic in JINR)
Wagner Vladimir (INP ASCR)
Wilhelm Ivan (Member of the JINR Scientific Council)
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HOW TO GET THERE
Tram 3, 10, 24 - Bulovka stop
Bus 201 - Vychovatelna stop
Bus 166 - Nemocnice Bulovka gynekologie stop

MAP
Peoples More...
Čuba Václav doc. Ing. Ph.D.
Fiala Lukáš
Chudoba Vratislav Ing. Ph.D.
Robenková Jitka Ing.
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MINISTR ŠKOLSTVÍ KE SPOLUPRÁCI ČR S SÚJV
Ministr školství ke spolupráci ČR s SÚJV
Grants More...
Air Pollution Mathematical Modelling: Integration, Verification and Utilization of CALPUFF in ADMOSS
Air Pollution Mathematical Modelling: Integration, Verification and Utilization of CALPUFF in ADMOSS
Publications More...
Status of the NICA project at JINR
4th International Conference on New Frontiers in Physics (ICNFP), Crete, Greece

The project NICA (Nuclotron-based Ion Collider fAcility) is aimed to study hot and dense baryonic matter in heavy ion collisions in the energy range up to root s(NN)=11 GeV