Abstract
A next generation of IceCube is under design including the Precision IceCube Next Generation Upgrade (PINGU) for the neutrino mass ordering and an extended array for astrophysical neutrino sources. A new level of precision is needed in order to guarantee improved performance with respect to IceCube. An improved calibration system will enable a better understanding of the ice and will therefore significantly reduce systematic effects. We present a new instrument called the Precision Optical Calibration Module (POCAM). By keeping the outer topology identical to that of the IceCube Digital Optical Module (DOM), cost-effective construction and deployment is ensured. The design of the POCAM is based on the principle of an inverted integrating sphere. An appropriately placed LED in combination with a diffusing layer on the inside of the sphere results in a nearly homogeneous light emission from the apertures in the spherical housing. The output of the LED is monitored in-situ to high precision, ensuring control over the output from the apertures. The POCAM has been simulated and tested in the framework of Geant4. A prototype POCAM is under construction. We report on the status of the POCAM RandD.
| Original language | English |
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| Article number | 1133 |
| Journal | Proceedings of Science |
| Volume | 30-July-2015 |
| State | Published - 2015 |
| Event | 34th International Cosmic Ray Conference, ICRC 2015 - The Hague, Netherlands Duration: 30 Jul 2015 → 6 Aug 2015 |