6533b860fe1ef96bd12c394b

RESEARCH PRODUCT

Sedimentation and Fouling of Optical Surfaces at the ANTARES Site

P AmramM AnghinolfiC AnvarFe Ardellier-desagesE AslanidesJj AubertR AzoulayD BaileyS BasaM BattaglieriR BellotiJ BeltramelliY BenhammouR BerthierV BertinM BillaultR BlaesRw BlandF BlondeauN De BottonJ BoulesteixCb BrooksJ BrunnerF CafagnaA CalzasA CaponeL CaponettoC CarloganuE CarmonaJ CarrSl CartwrightS CecchiniF CiacioM CircellaC CompereS CooperP CoyleS CuneoM DanilovR Van DantzigC De MarzoJj DestelleR De VitaG DispauF DruilloleJ EngelenF FeinsteinC FerdiD FestyJ FopmaJm GalloneG GiacomelliP GoretJf GournayG HallewellA HeijboerJj Hernandez-reyJr HubbardM JaquetM De JongM KarolakP KellerP KooijmanA KouchnerVa KudryavtsevH LafouxP LagierP LamareJc LanguillatL LaubierJp LaugierB LeildeH Le ProvostAl Van SuuL Lo NigroD Lo PrestiS LoucatosF LouisV LyashukP MagnierM MarcelinA MargiottaR MasulloF MazeasB MazeauA MazureJe McmillanE MignecoC MillotP MolsF MontanetT MontaruliL MoscosoM MusumeciE NezriGj NoorenJej OberskiC OlivettoA Oppelt-pohlN Palanque-delabrouilleR PapaleoP PayreP PerrinM PetruccettiC PettaP PiattelliJ PoinsignonR PotheauY QueinecC RaccaG RaiaN RandazzoF RethoreG RiccobeneJs RicolM RipaniV Roca-blayA RomeyerA RostovstevGv RussoY SacquinE SalustiJp SchullerW SchusterJp SoiratO SouvorovaNjc SpoonerM SpurioT StolarczykD StubertM TaiutiC TaoLf ThompsonS TilavR TriayA UsikP ValdyV ValenteI VarlamovG VaudaineP VerninE VladimirskyM VorobievPd HubertsE De WolfV ZakharovS ZavatarelliJd ZornozaJ ZunigaJc AloisiP KerherveA MonacoAntares CollaborationAntares CollaborationCefrem Collaboration

subject

PhotomultiplierTransmission lossEquatorMineralogyFOS: Physical sciencesAstrophysics[SDU.ASTR] Sciences of the Universe [physics]/Astrophysics [astro-ph]Neutrino telescopeAstrophysics01 natural scienceslaw.inventionTelescope[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]High Energy Physics - Phenomenology (hep-ph)law0103 physical sciencesfouling; neutrino telescope; sea water properties; sedimentation; undersea cherenkov detectors14. Life underwater010306 general physicsCherenkov radiationZenithPhysicsUndersea Cherenkov detectors[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsAstrophysics (astro-ph)Sea water propertieAstronomy and AstrophysicsFoulingSedimentationHigh Energy Physics - Phenomenology[PHYS.ASTR.CO] Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Física nuclearNeutrinoSedimentation

description

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 ~2% 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.

http://hal.in2p3.fr/in2p3-00012411