Sedimentation and fouling of optical surfaces at the ANTARES site

被引:54
作者
Amram, P
Anghinolfi, M
Anvar, C
Ardellier-Desages, FE
Aslanides, E
Aubert, JJ
Azoulay, R
Bailey, D
Basa, S
Battaglieri, M
Belloti, R
Beltramelli, J
Benhammou, Y
Berthier, R
Bertin, V
Billault, M
Blaes, R
Bland, RW
Blondeau, F
de Botton, N
Boulesteix, J
Brooks, CB
Brunner, J
Cafagna, F
Calzas, A
Capone, A
Caponetto, L
Cârloganu, C
Carmona, E
Carr, J
Cartwright, SL
Cecchini, S
Ciacio, F
Circella, M
Compère, C
Cooper, S
Coyle, P
Cuneo, S
Danilov, M
van Dantzig, R
De Marzo, C
Destelle, JJ
De Vita, R
Dispau, G
Druillole, F
Engelen, J
Feinstein, F
Ferdi, C
Festy, D
Fopma, J
机构
[1] CEA Saclay, DSM, DAPNIA, F-91191 Gif Sur Yvette, France
[2] Univ Aix Marseille 1, LAM, CNRS, INSU, F-13012 Marseille 12, France
[3] Univ Genoa, Dept Fis, I-16146 Genoa, Italy
[4] Sezione Ist Nazl Fis Nucl, I-16146 Genoa, Italy
[5] Univ Aix Marseille 2, CPPM, CNRS, IN2P3, F-13288 Marseille 9, France
[6] Univ Oxford, Nucl & Astrophys Lab, Dept Phys, Oxford OX1 3RH, England
[7] Dipartimento Interateneo Fis, I-70126 Bari, Italy
[8] Sezione Ist Nazl Fis Nucl, I-70126 Bari, Italy
[9] Univ Haute Alsace, GRPHE, F-68093 Mulhouse, France
[10] Univ Roma La Sapienza, Dipartimento Fis, I-00185 Rome, Italy
[11] Sezione Ist Nazl Fis Nucl, I-00185 Rome, Italy
[12] Univ Catania, Dipartimento Fis & Astron, I-95129 Catania, Italy
[13] Sezione Ist Nazl Fis Nucl, I-95129 Catania, Italy
[14] NIKHEF H, NL-1009 SJ Amsterdam, Netherlands
[15] Univ Valencia, CSIC, IFIC, Inst Fis Corpuscular Edificios Invest Paterna, Valencia 46071, Spain
[16] Univ Sheffield, Dept Phys & Astron, Sheffield S3 7RH, S Yorkshire, England
[17] Univ Bologna, Dipartmento Fis, I-40127 Bologna, Italy
[18] Sezione Ist Nazl Fis Nucl, I-40127 Bologna, Italy
[19] CNR, TESRE, I-40129 Bologna, Italy
[20] IFREMER, Ctr Toulon La Seyne Sur Mer, F-83500 La Seyne Sur Mer, France
[21] IFREMER, Ctr Brest, F-29280 Plouzane, France
[22] Inst Theoret & Expt Phys, Moscow 117259, Russia
[23] Univ Louis Pasteur Strasbourg 1, Inst Rech Subatom, CNRS, IN2P3, F-67037 Strasbourg 2, France
[24] Univ Aix Marseille 2, CNRS, INSU, COM,Stn Marine Endoume Luminy, F-13007 Marseille, France
[25] LNS, Ist Nazl Fis Nucl, I-95123 Catania, Italy
[26] CNRS, Ctr Phys Theor, F-13288 Marseille 09, France
[27] Univ Perpignan, CEFREM, F-66860 Perpignan, France
基金
俄罗斯基础研究基金会;
关键词
neutrino telescope; undersea Cherenkov detectors; sea water properties; fouling; sedimentation;
D O I
10.1016/S0927-6505(02)00202-5
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
ANTARES is a project leading towards the construction and deployment of a neutrino telescope in the deep Mediterranean Sea. The telescope will use an array of photomultiplier tubes to detect the Cherenkov light emitted by muons resulting from the interaction with matter of high energy neutrinos. In the vicinity of the deployment site the ANTARES Collaboration has performed a series of in situ measurements to study the change in light transmission through glass surfaces during immersions of several months. The average loss of light transmission is estimated to be only similar to2% at the equator of a glass sphere one year after deployment. It decreases with increasing zenith angle, and tends to saturate with time. The transmission loss, therefore, is expected to remain small for the several year lifetime of the ANTARES detector whose optical modules are oriented downwards. The measurements were complemented by the analysis of the (210)Pb activity profile in sediment cores and the study of biofouling on glass plates. Despite a significant sedimentation rate at the site, in the 0.02-0.05 cm yr(-1) range, the sediments adhere loosely to the glass surfaces and can be washed off by water currents. Further, fouling by deposits of light-absorbing particulates is only significant for surfaces facing upwards. (C) 2002 Elsevier Science B.V. All rights reserved.
引用
收藏
页码:253 / 267
页数:15
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