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Design, performance...
Design, performance, and analysis of a measurement of optical properties of antarctic ice below 400 nm
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- Abbasi, R. (författare)
- Loyola Univ Chicago, Dept Phys, Chicago, IL 60660 USA
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- Botner, Olga (författare)
- Uppsala universitet,Högenergifysik
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- Burgman, Alexander (författare)
- Uppsala universitet,Högenergifysik,FREIA
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- Glaser, Christian (författare)
- Uppsala universitet,Högenergifysik
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- Hallgren, Allan, 1951- (författare)
- Uppsala universitet,Högenergifysik
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- O'Sullivan, Erin (författare)
- Uppsala universitet,Högenergifysik
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- Pérez de los Heros, Carlos (författare)
- Uppsala universitet,Högenergifysik
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- Sharma, Ankur (författare)
- Uppsala universitet,Högenergifysik
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- Valtonen-Mattila, Nora (författare)
- Uppsala universitet,Högenergifysik
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- Zhang, Z. (författare)
- SUNY Stony Brook, Dept Phys & Astron, Stony Brook, NY 11794 USA
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(creator_code:org_t)
- Trieste, Italy : Sissa Medialab Srl, 2022
- 2022
- Engelska.
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Ingår i: 37th International Cosmic Ray Conference (ICRC 2021). - Trieste, Italy : Sissa Medialab Srl.
- Relaterad länk:
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https://doi.org/10.2...
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https://uu.diva-port... (primary) (Raw object)
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https://pos.sissa.it...
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https://urn.kb.se/re...
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https://doi.org/10.2...
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Abstract
Ämnesord
Stäng
- The IceCubeNeutrino Observatory, located at the geographic South Pole, is theworld's largest neutrino telescope, instrumenting 1 km(3) of Antarctic ice with 5160 photosensors to detect Cherenkov light. For the IceCube Upgrade, to be deployed during the 2022-23 polar field season, and the enlarged detector IceCube-Gen2 several new optical sensor designs are under development. One of these optical sensors, the Wavelength-shifting Optical Module (WOM), uses wavelength-shifting and light-guiding techniques to measure Cherenkov photons in the UV range from 250 nm to 380 nm. In order to understand the potential gains from this new technology, a measurement of the scattering and absorption lengths of UV light was performed in the SPICEcore borehole at the South Pole during the winter seasons of 2018/2019 and 2019/2020. For this purpose, a calibration device with a UV light source and a detector using the wavelength shifting technology was developed. We present the design of the developed calibration device, its performance during the measurement campaigns, and the comparison of data to a Monte Carlo simulation.
Ämnesord
- NATURVETENSKAP -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
- NATURAL SCIENCES -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)
Publikations- och innehållstyp
- ref (ämneskategori)
- kon (ämneskategori)