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dc.contributor.authorAartsen, M.
dc.contributor.authorAbbasi, R.
dc.contributor.authorAbdou, Y.
dc.contributor.authorAckermann, M.
dc.contributor.authorAdams, J.
dc.contributor.authorAguilar, J.
dc.contributor.authorAhlers, M.
dc.contributor.authorAltmann, D.
dc.contributor.authorAuffenberg, J.
dc.contributor.authorBai, X.
dc.contributor.authorBaker, M.
dc.contributor.authorBarwick, S.
dc.contributor.authorBaum, V.
dc.contributor.authorBay, R.
dc.contributor.authorBeatty, J.
dc.contributor.authorBechet, S.
dc.contributor.authorBecker Tjus, J.
dc.contributor.authorBecker, K.
dc.contributor.authorBell, M.
dc.contributor.authorBenabderrahmane, M.
dc.contributor.authorBenzvi, S.
dc.contributor.authorBerdermann, J.
dc.contributor.authorBerghaus, P.
dc.contributor.authorBerley, D.
dc.contributor.authorBernardini, E.
dc.contributor.authorBernhard, A.
dc.contributor.authorBertrand, D.
dc.contributor.authorBesson, D.
dc.contributor.authorBinder, G.
dc.contributor.authorBindig, D.
dc.contributor.authorBissok, M.
dc.contributor.authorBlaufuss, E.
dc.contributor.authorBlumenthal, J.
dc.contributor.authorBoersma, D.
dc.contributor.authorBohaichuk, S.
dc.contributor.authorBohm, C.
dc.contributor.authorBose, D.
dc.contributor.authorBöser, S.
dc.contributor.authorBotner, O.
dc.contributor.authorBrayeur, L.
dc.contributor.authorBrown, A.
dc.contributor.authorBruijn, R.
dc.contributor.authorBrunner, J.
dc.contributor.authorBuitink, S.
dc.contributor.authorCarson, Michael
dc.contributor.authorCasey, J.
dc.contributor.authorCasier, M.
dc.contributor.authorChirkin, D.
dc.contributor.authorChristy, B.
dc.contributor.authorClark, K.
dc.contributor.authorClevermann, F.
dc.contributor.authorCohen, S.
dc.contributor.authorCowen, D.
dc.contributor.authorCruz Silva, A.
dc.contributor.authorDanninger, M.
dc.contributor.authorDaughhetee, J.
dc.contributor.authorDavis, J.
dc.contributor.authorDe Clercq, C.
dc.contributor.authorDe Ridder, S.
dc.contributor.authorDesiati, P.
dc.contributor.authorDe With, M.
dc.contributor.authorDeyoung, T.
dc.contributor.authorDíaz-Vélez, J.
dc.contributor.authorDunkman, M.
dc.contributor.authorEagan, R.
dc.contributor.authorEberhardt, B.
dc.contributor.authorEisch, J.
dc.contributor.authorEllsworth, R.
dc.contributor.authorEuler, S.
dc.contributor.authorEvenson, P.
dc.contributor.authorFadiran, O.
dc.contributor.authorFazely, A.
dc.contributor.authorFedynitch, A.
dc.contributor.authorFeintzeig, J.
dc.contributor.authorFeusels, T.
dc.contributor.authorFilimonov, K.
dc.contributor.authorFinley, C.
dc.contributor.authorFischer-Wasels, T.
dc.contributor.authorFlis, S.
dc.contributor.authorFranckowiak, A.
dc.contributor.authorFranke, R.
dc.contributor.authorFrantzen, K.
dc.contributor.authorFuchs, T.
dc.contributor.authorGaisser, T.
dc.contributor.authorGallagher, J.
dc.contributor.authorGerhardt, L.
dc.contributor.authorGladstone, L.
dc.contributor.authorGlüsenkamp, T.
dc.contributor.authorGoldschmidt, A.
dc.contributor.authorGolup, G.
dc.contributor.authorGoodman, J.
dc.contributor.authorGóra, D.
dc.contributor.authorGrant, D.
dc.contributor.authorGroß, A.
dc.contributor.authorGurtner, M.
dc.contributor.authorHa, C.
dc.date.accessioned2017-01-30T13:06:05Z
dc.date.available2017-01-30T13:06:05Z
dc.date.created2016-01-18T20:00:43Z
dc.date.issued2013
dc.identifier.citationAartsen, M. and Abbasi, R. and Abdou, Y. and Ackermann, M. and Adams, J. and Aguilar, J. and Ahlers, M. et al. 2013. Measurement of South Pole ice transparency with the IceCube LED calibration system. Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment. 711: pp. 73-89.
dc.identifier.urihttp://hdl.handle.net/20.500.11937/28617
dc.identifier.doi10.1016/j.nima.2013.01.054
dc.description.abstract

The IceCube Neutrino Observatory, approximately 1 km3 in size, is now complete with 86 strings deployed in the Antarctic ice. IceCube detects the Cherenkov radiation emitted by charged particles passing through or created in the ice. To realize the full potential of the detector, the properties of light propagation in the ice in and around the detector must be well understood. This report presents a new method of fitting the model of light propagation in the ice to a data set of in situ light source events collected with IceCube. The resulting set of derived parameters, namely the measured values of scattering and absorption coefficients vs. depth, is presented and a comparison of IceCube data with simulations based on the new model is shown.

dc.titleMeasurement of South Pole ice transparency with the IceCube LED calibration system
dc.typeJournal Article
dcterms.source.volume711
dcterms.source.startPage73
dcterms.source.endPage89
dcterms.source.issn0168-9002
dcterms.source.titleNuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
curtin.departmentDepartment of Exploration Geophysics
curtin.accessStatusFulltext not available


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