| HAL : in2p3-00372131, version 1 |
| DOI : 10.1016/j.nuclphysbps.2009.02.047 |
| Fiche détaillée | Récupérer au format |
|
|
| Neutrino Oscillation Workshop - NOW 2008, Conca Specchiulla, Oranto : Italie (2008) |
|
|
|
|
| The CNGS neutrino beam: status |
|
|
| D. Autiero1I. EfthymiopoulosA. FerrariE. GschwendtnerA. GuglielmiJ. LettryA. PardonsF. PietropaoloP.R. SalaL. SarchiaponeH. Vincke |
|
|
| (2009) |
|
|
| The first months of 2008 were a busy and productive period for the CNGS facility. An ambitious and demanding project aimed to the protection of electronics against radiation has been devised and carried out in a very short time. Meanwhile, the Earth magnetic field has been singled out as the responsible of the asymmetry observed in the muon pits profiles when switching from neutrino to anti-neutrino mode. The facility ran smoothly from June 18th to November 3rd 2008 delivering almost 2.0dot operator1019 protons on target (p.o.t.) |
|
|
|
|
|
|
|
|
|
|
| 1 : | IPNL - Institut de Physique Nucléaire de Lyon |
|
|
|
|
|
|
|
|
| Thème(s) | : | Physique/Astrophysique/Phénomènes cosmiques de haute energie Planète et Univers/Astrophysique/Phénomènes cosmiques de haute energie |
| in2p3-00372131, version 1 | |
| http://hal.in2p3.fr/in2p3-00372131 | |
| oai:hal.in2p3.fr:in2p3-00372131 | |
| Contributeur : Dominique Girod | |
| Soumis le : Mardi 31 Mars 2009, 13:07:08 | |
| Dernière modification le : Mardi 4 Août 2009, 10:12:54 | |