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Télécharger JPG | Télécharger EPS |
The Computing for Science (CS) group supports ILL scientists, students and visitors in a number of activities including data analysis, instrument simulation and sample simulation.

The ILL Reactor Simulations Data BaseComputed by E. Farhi (ILL/DS/CS), P.A. Harraud (ILL/DS/CS) and S. Fuard (ILL/DPT/BPC) in Nov 2006. Updated in 2011.
This site gathers a comprehensive study of all beam tubes exiting the ILL heavy water reactor vessel (except the inclined tubes). Each simulation comes with its description file for MCNP and/or Tripoli, as well as spectrum, XY and angular distributions to be used for further shielding computations and propagation to the instruments, often through the guides. Interface from MNCP PTRAC and Tripoli BATCH files are available in McStas. Beam tubes (hot, thermal, cold) simulated at 5.2 mMethodology:
The Vanne de Securite (VS) is situated at L=5.2 m distance from the core center ('Bouchon'). The capture flux measurements on beam tubes are performed there, at about 6 m from the doigt-de-gant nose. ILL BrillianceFrom the flux estimates obtained with both MCNP and Tripoli events propagated with McStas, we extract the brilliance of a number of tubes, using the divergence measured with the McStas histograms (usually about +/-1 deg at 5.2 m). The Brilliance of cold sources is 2 1013 at maximum, and thermal tubes reach about 5-8 1013 [n/s/cm2/st/Angs] but this depends a lot on the beam tube (H10 and H11 are more intense by e.g. a factor 2). [fig in EPS][PNG]. This Data has been updated by Farhi and Calzavara on Feb 21st, 2011 [ pdf ]. Overview of measured and computed flux at beam tube
Table 1: Flux measured and simulated with MCNP and Tripoli at 5.2 m from the core (bouchon). Data in italic is to be taken with caution (old or geometry was changed since then).
CONCLUSION: Both MCNP and Tripoli neutrons propagated using McStas agree (nearly) perfectly with measurements. Geometry description and other relevant information
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