Measurement of South Pole ice transparency with the IceCube LED calibration system

IceCube Collaboration

Measurement of South Pole ice transparency with the IceCube LED calibration system

IceCube Collaboration

Natuurkunde

Onderzoeksoutput: Article › peer review

181 Citaten (Scopus)

Samenvatting

The IceCube Neutrino Observatory, approximately 1 km^3 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.
The IceCube Neutrino Observatory, approximately 1km^3 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.

Originele taal-2	English
Pagina's (van-tot)	73-89
Aantal pagina's	16
Tijdschrift	Nuclear Instruments and Methods in Physics Research Section A
Volume	711
Status	Published - 21 mei 2013

SRP8: SRP (Zwaartepunt): Hoge-Energiefysica
D'Hondt, J., Van Eijndhoven, N., Craps, B. & Buitink, S.
1/11/12 → 31/10/24
Project: Fundamenteel

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@article{4f3a379f30114c849e1ce85513423330,

title = "Measurement of South Pole ice transparency with the IceCube LED calibration system",

abstract = "The IceCube Neutrino Observatory, approximately 1 km^3 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. The IceCube Neutrino Observatory, approximately 1km^3 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.",

keywords = "IceCube, South Pole Ice, Optical properties, Photon progagation",

author = "{IceCube Collaboration} and Lionel Brayeur and Martin Casier and {De Clercq}, Catherine and Golup, {Geraldina Tamara} and {Van Eijndhoven}, Nicolaas and Jan Kunnen and Giuliano Maggi and {De Vries}, Krijn",

year = "2013",

month = may,

day = "21",

language = "English",

volume = "711",

pages = "73--89",

journal = "Nuclear Instruments and Methods in Physics Research Section A",

issn = "0168-9002",

publisher = "Elsevier",

}

TY - JOUR

T1 - Measurement of South Pole ice transparency with the IceCube LED calibration system

AU - IceCube Collaboration

AU - Brayeur, Lionel

AU - Casier, Martin

AU - De Clercq, Catherine

AU - Golup, Geraldina Tamara

AU - Van Eijndhoven, Nicolaas

AU - Kunnen, Jan

AU - Maggi, Giuliano

AU - De Vries, Krijn

PY - 2013/5/21

Y1 - 2013/5/21

N2 - The IceCube Neutrino Observatory, approximately 1 km^3 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. The IceCube Neutrino Observatory, approximately 1km^3 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 km^3 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. The IceCube Neutrino Observatory, approximately 1km^3 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 - South Pole Ice

KW - Optical properties

KW - Photon progagation

M3 - Article

VL - 711

SP - 73

EP - 89

JO - Nuclear Instruments and Methods in Physics Research Section A

JF - Nuclear Instruments and Methods in Physics Research Section A

SN - 0168-9002

ER -

Measurement of South Pole ice transparency with the IceCube LED calibration system

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SRP8: SRP (Zwaartepunt): Hoge-Energiefysica

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