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.
Original language | English (US) |
---|---|
Pages (from-to) | 73-89 |
Number of pages | 17 |
Journal | Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment |
Volume | 711 |
DOIs | |
State | Published - 2013 |
Keywords
- IceCube
- Optical properties
- Photon propagation
- South Pole ice
ASJC Scopus subject areas
- Nuclear and High Energy Physics
- Instrumentation
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In: Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, Vol. 711, 2013, p. 73-89.
Research output: Contribution to journal › Article › peer-review
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TY - JOUR
T1 - Measurement of South Pole ice transparency with the IceCube LED calibration system
AU - Aartsen, M. G.
AU - Abbasi, R.
AU - Abdou, Y.
AU - Ackermann, M.
AU - Adams, J.
AU - Aguilar, J. A.
AU - Ahlers, M.
AU - Altmann, D.
AU - Auffenberg, J.
AU - Bai, X.
AU - Baker, M.
AU - Barwick, S. W.
AU - Baum, V.
AU - Bay, R.
AU - Beatty, J. J.
AU - Bechet, S.
AU - Becker Tjus, J.
AU - Becker, K. H.
AU - Bell, M.
AU - Benabderrahmane, M. L.
AU - Benzvi, S.
AU - Berdermann, J.
AU - Berghaus, P.
AU - Berley, D.
AU - Bernardini, E.
AU - Bernhard, A.
AU - Bertrand, D.
AU - Besson, D. Z.
AU - Binder, G.
AU - Bindig, D.
AU - Bissok, M.
AU - Blaufuss, E.
AU - Blumenthal, J.
AU - Boersma, D. J.
AU - Bohaichuk, S.
AU - Bohm, C.
AU - Bose, D.
AU - Böser, S.
AU - Botner, O.
AU - Brayeur, L.
AU - Brown, A. M.
AU - Bruijn, R.
AU - Brunner, J.
AU - Buitink, S.
AU - Carson, M.
AU - Casey, J.
AU - Casier, M.
AU - Chirkin, D.
AU - Christy, B.
AU - Clark, K.
AU - Clevermann, F.
AU - Cohen, S.
AU - Cowen, D. F.
AU - Cruz Silva, A. H.
AU - Danninger, M.
AU - Daughhetee, J.
AU - Davis, J. C.
AU - De Clercq, C.
AU - De Ridder, S.
AU - Desiati, P.
AU - De With, M.
AU - Deyoung, T.
AU - Díaz-Vélez, J. C.
AU - Dunkman, M.
AU - Eagan, R.
AU - Eberhardt, B.
AU - Eisch, J.
AU - Ellsworth, R. W.
AU - Euler, S.
AU - Evenson, P. A.
AU - Fadiran, O.
AU - Fazely, A. R.
AU - Fedynitch, A.
AU - Feintzeig, J.
AU - Feusels, T.
AU - Filimonov, K.
AU - Finley, C.
AU - Fischer-Wasels, T.
AU - Flis, S.
AU - Franckowiak, A.
AU - Franke, R.
AU - Frantzen, K.
AU - Fuchs, T.
AU - Gaisser, T. K.
AU - Gallagher, J.
AU - Gerhardt, L.
AU - Gladstone, L.
AU - Glüsenkamp, T.
AU - Goldschmidt, A.
AU - Golup, G.
AU - Goodman, J. A.
AU - Góra, D.
AU - Grant, D.
AU - Groß, A.
AU - Gurtner, M.
AU - Ha, C.
AU - Haj Ismail, A.
AU - Hallgren, A.
AU - Halzen, F.
AU - Hanson, K.
AU - Heereman, D.
AU - Heimann, P.
AU - Heinen, D.
AU - Helbing, K.
AU - Hellauer, R.
AU - Hickford, S.
AU - Hill, G. C.
AU - Hoffman, K. D.
AU - Hoffmann, R.
AU - Homeier, A.
AU - Hoshina, K.
AU - Huelsnitz, W.
AU - Hulth, P. O.
AU - Hultqvist, K.
AU - Hussain, S.
AU - Ishihara, A.
AU - Jacobi, E.
AU - Jacobsen, J.
AU - Japaridze, G. S.
AU - Jero, K.
AU - Jlelati, O.
AU - Kaminsky, B.
AU - Kappes, A.
AU - Karg, T.
AU - Karle, A.
AU - Kelley, J. L.
AU - Kiryluk, J.
AU - Kislat, F.
AU - Kläs, J.
AU - Klein, S. R.
AU - Köhne, J. H.
AU - Kohnen, G.
AU - Kolanoski, H.
AU - Köpke, L.
AU - Kopper, C.
AU - Kopper, S.
AU - Koskinen, D. J.
AU - Kowalski, M.
AU - Krasberg, M.
AU - Kroll, G.
AU - Kunnen, J.
AU - Kurahashi, N.
AU - Kuwabara, T.
AU - Labare, M.
AU - Landsman, H.
AU - Larson, M. J.
AU - Lesiak-Bzdak, M.
AU - Leute, J.
AU - Lünemann, J.
AU - Madsen, J.
AU - Maruyama, R.
AU - Mase, K.
AU - Matis, H. S.
AU - McNally, F.
AU - Meagher, K.
AU - Merck, M.
AU - Mészáros, P.
AU - Meures, T.
AU - Miarecki, S.
AU - Middell, E.
AU - Milke, N.
AU - Miller, J.
AU - Mohrmann, L.
AU - Montaruli, T.
AU - Morse, R.
AU - Nahnhauer, R.
AU - Naumann, U.
AU - Niederhausen, H.
AU - Nowicki, S. C.
AU - Nygren, D. R.
AU - Obertacke, A.
AU - Odrowski, S.
AU - Olivas, A.
AU - Olivo, M.
AU - O'Murchadha, A.
AU - Paul, L.
AU - Pepper, J. A.
AU - Pérez De Los Heros, C.
AU - Pfendner, C.
AU - Pieloth, D.
AU - Pirk, N.
AU - Posselt, J.
AU - Price, P. B.
AU - Przybylski, G. T.
AU - Rädel, L.
AU - Rawlins, K.
AU - Redl, P.
AU - Resconi, E.
AU - Rhode, W.
AU - Ribordy, M.
AU - Richman, M.
AU - Riedel, B.
AU - Rodrigues, J. P.
AU - Rott, C.
AU - Ruhe, T.
AU - Ruzybayev, B.
AU - Ryckbosch, D.
AU - Saba, S. M.
AU - Salameh, T.
AU - Sander, H. G.
AU - Santander, M.
AU - Sarkar, S.
AU - Schatto, K.
AU - Scheel, M.
AU - Scheriau, F.
AU - Schmidt, T.
AU - Schmitz, M.
AU - Schoenen, S.
AU - Schöneberg, S.
AU - Schönherr, L.
AU - Schönwald, A.
AU - Schukraft, A.
AU - Schulte, L.
AU - Schulz, O.
AU - Seckel, D.
AU - Seo, S. H.
AU - Sestayo, Y.
AU - Seunarine, S.
AU - Sheremata, C.
AU - Smith, M. W.E.
AU - Soiron, M.
AU - Soldin, D.
AU - Spiczak, G. M.
AU - Spiering, C.
AU - Stamatikos, M.
AU - Stanev, T.
AU - Stasik, A.
AU - Stezelberger, T.
AU - Stokstad, R. G.
AU - Stößl, A.
AU - Strahler, E. A.
AU - Ström, R.
AU - Sullivan, G. W.
AU - Taavola, H.
AU - Taboada, I.
AU - Tamburro, A.
AU - Ter-Antonyan, S.
AU - Tilav, S.
AU - Toale, P. A.
AU - Toscano, S.
AU - Usner, M.
AU - Van Der Drift, D.
AU - Van Eijndhoven, N.
AU - Van Overloop, A.
AU - Van Santen, J.
AU - Vehring, M.
AU - Voge, M.
AU - Vraeghe, M.
AU - Walck, C.
AU - Waldenmaier, T.
AU - Wallraff, M.
AU - Wasserman, R.
AU - Weaver, Ch
AU - Wellons, M.
AU - Wendt, C.
AU - Westerhoff, S.
AU - Whitehorn, N.
AU - Wiebe, K.
AU - Wiebusch, C. H.
AU - Williams, D. R.
AU - Wissing, H.
AU - Wolf, M.
AU - Wood, T. R.
AU - Xu, C.
AU - Xu, D. L.
AU - Xu, X. W.
AU - Yanez, J. P.
AU - Yodh, G.
AU - Yoshida, S.
AU - Zarzhitsky, P.
AU - Ziemann, J.
AU - Zierke, S.
AU - Zilles, A.
AU - Zoll, M.
N1 - Funding Information: We acknowledge the support from the following agencies: U.S. National Science Foundation-Office of Polar Programs , U.S. National Science Foundation-Physics Division , University of Wisconsin Alumni Research Foundation , the Grid Laboratory Of Wisconsin (GLOW) grid infrastructure at the University of Wisconsin, Madison, the Open Science Grid (OSG) grid infrastructure; U.S. Department of Energy , and National Energy Research Scientific Computing Center , the Louisiana Optical Network Initiative (LONI) grid computing resources; National Science and Engineering Research Council of Canada ; Swedish Research Council , Swedish Polar Research Secretariat , Swedish National Infrastructure for Computing (SNIC) , and Knut and Alice Wallenberg Foundation , Sweden; German Ministry for Education and Research (BMBF) , Deutsche Forschungsgemeinschaft (DFG) , Helmholtz Alliance for Astroparticle Physics (HAP) , Research Department of Plasmas with Complex Interactions (Bochum) , Germany; Fund for Scientific Research (FNRS-FWO) , FWO Odysseus programme, Flanders Institute to encourage scientific and technological research in industry (IWT), Belgian Federal Science Policy Office (Belspo); University of Oxford, United Kingdom; Marsden Fund, New Zealand; Australian Research Council; Japan Society for Promotion of Science (JSPS); the Swiss National Science Foundation (SNSF) , Switzerland.
PY - 2013
Y1 - 2013
N2 - 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.
AB - 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.
KW - IceCube
KW - Optical properties
KW - Photon propagation
KW - South Pole ice
UR - http://www.scopus.com/inward/record.url?scp=84874743378&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=84874743378&partnerID=8YFLogxK
U2 - 10.1016/j.nima.2013.01.054
DO - 10.1016/j.nima.2013.01.054
M3 - Article
AN - SCOPUS:84874743378
SN - 0168-9002
VL - 711
SP - 73
EP - 89
JO - Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
JF - Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
ER -