The Cosmic Ray Energetics And Mass (CREAM) instrument is a balloon-borne experiment designed to measure the composition and energy spectra of cosmic rays up to similar to 10(15) eV. The instrument consists of, from top to bottom, an 8-paddle Timing Charge Detector (TCD), a 512-tube Transition Radiation Detector (TRD), a 2912-pixel Silicon Charge Detector (SCD), 2035 scintillating fibers in 3 hodoscopes interleaved with a pair of graphite targets, and a 20-layer tungsten/scintillating-fiber sampling calorimeter with 1000 fiber ribbons. We have developed the CREAM Data Processing System (CDPS), an object-oriented data processing program based on ROOT. In this paper we describe the data processing scheme used to handle flight data.

H. S., A., P., A., M. G., B., J. J., B., Bigongiari, G., P., B., et al. (2005). CREAM flight data processing. In Proceedings of the 29th International Cosmic Ray Conference (pp.389-392). Pune : Tata Inst Fundamental Research.

CREAM flight data processing

BIGONGIARI, GABRIELE;MAESTRO, PAOLO;MARROCCHESI, PIER SIMONE;
2005-01-01

Abstract

The Cosmic Ray Energetics And Mass (CREAM) instrument is a balloon-borne experiment designed to measure the composition and energy spectra of cosmic rays up to similar to 10(15) eV. The instrument consists of, from top to bottom, an 8-paddle Timing Charge Detector (TCD), a 512-tube Transition Radiation Detector (TRD), a 2912-pixel Silicon Charge Detector (SCD), 2035 scintillating fibers in 3 hodoscopes interleaved with a pair of graphite targets, and a 20-layer tungsten/scintillating-fiber sampling calorimeter with 1000 fiber ribbons. We have developed the CREAM Data Processing System (CDPS), an object-oriented data processing program based on ROOT. In this paper we describe the data processing scheme used to handle flight data.
2005
H. S., A., P., A., M. G., B., J. J., B., Bigongiari, G., P., B., et al. (2005). CREAM flight data processing. In Proceedings of the 29th International Cosmic Ray Conference (pp.389-392). Pune : Tata Inst Fundamental Research.
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11365/44358
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