NEVOD
The term NEVOD experimental complex is used of the experimental complex built around the original water Cherenkov detector for the study of cosmic rays; as of 2018, the experimental complex consists of: the Cherenkov water detector (the eponymous NEVOD detector), a coordinate-tracking detector DECOR, an array of scintillation detectors forming the calibration telescopes system CTS, and PRISMA array of thermal neutron detectors. As of 2018, the experimental complex is being expanded by three new cosmic ray detectors: NEVOD-EAS (for determination of cosmic ray air shower parameters), URAN (neutron detector) and TREK (drift chamber detector). Part of the new detectors are under operation (in 2018).
The experimental complex used to also have a muon hodoscope URAGAN which was operational in 2016 and years prior. Current (2019) status of URAGAN is unknown.
Description
As described by its inventors, NEVOD consists of a water reservoir measuring 9 m x 9 m x 26 m into which is placed a spatial lattice of quasi-spherical detector modules (QSMs) to record Cherenkov radiation from any direction. The dimensions of reservoir make it possible to arrange up to 241 QSMs.
The quasi-spherical modules are, in fact, not spherical, but consist of an array of 6 photomultiplier tubes arranged along the primary axes of the device. The arrangement of the PMTs is such that the response of the PMT is dependent only on the intensity of the incident radiation, but not on its angle of incidence (over the limitation of angles viewable by the device), rendering the entire detector "quasi-spherical".
History
NEVOD started operations in 1994 and was described in a journal in 1995, and has since been used both for primary research and for educational purposes. Since the start of NEVOD experiment's operation, many detectors have been added to the original Cherenkov detector, becoming the NEVOD experimental complex. Also the Cherenkov detector has been upgraded many times. One upgrade of the experimental complex was discussed in 2015-2016.
As of 2018, the NEVOD experimental complex is operational.
References
- ^ "TeVPA 2018 (27-August 31, 2018)".
- ^ Yashin, I. I.; Barbashina, N. S.; Borisov, A. A.; Chiavassa, A.; Fakhrutdinov, R. M.; Gromushkin, D. M.; Khokhlov, S. S.; Kokoulin, R. P.; Kozhin, A. S.; Petrukhin, A. A.; Shulzhenko, I. A.; Stenkin, Yu. V.; Zadeba, E. A. (2016). "New detectors of the Experimental complex NEVOD for multicomponent EAS detection". arXiv:1612.09450 [astro-ph.IM].
- ^
Aynutdinov, V.M.; Kindin, V.V.; Kompaniets, K.G.; Petrukhin, A.A.; Tkachenko, P.V.; Shutenko, V.V.; Yashin1, I.I. (1997). "Neutrino Water Detector on the Earth's Surface". Astrophysics and Space Science. 58 (1–2): 105. Bibcode:1997Ap&SS.258..105A. doi:10.1023/A:1001779122430. S2CID 115885167.
{{cite journal}}: CS1 maint: numeric names: authors list (link) - ^ "Experimental Complex NEVOD". NEVOD MEPhI. 2006. Retrieved 2010-06-18.
- ^ Kindin, V.V.; Amelchakov, M.B.; Barbashina, N.S.; Burtsev, V.D.; Khokhlov, S.S.; Kokoulin, R.P.; Kompaniets, K.G.; Ovchinnikov, V.V.; Petrukhin, A.A.; Shulzhenko, I.A.; Shutenko, V.V.; Yashin, I.I.; Zadeba, E.A. (2015). "Cherenkov Water Detector NEVOD: A New Stage of Development". Physics Procedia. 74: 435–441. Bibcode:2015PhPro..74..435K. doi:10.1016/j.phpro.2015.09.221.
- ^ Yashin, I. I.; Barbashina, N. S.; Borisov, A. A.; Chiavassa, A.; Fakhrutdinov, R. M.; Gromushkin, D. M.; Khokhlov, S. S.; Kokoulin, R. P.; Kozhin, A. S.; Petrukhin, A. A.; Shulzhenko, I. A.; Stenkin, Yu. V.; Zadeba, E. A. (2016). "New detectors of the Experimental complex NEVOD for multicomponent EAS detection". arXiv:1612.09450 [astro-ph.IM].
- ^ "TeVPA 2018 (27-August 31, 2018)".
External links
NEVOD experiment record on INSPIRE-HEP