Simulation of Solar Wind Charged Particle Energy Deposited and Particle Identification by $Δ$E-E Discrimination in the SNAPPY Cubesat Detector
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arXiv
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| Format: | Preprint |
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2024
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| _version_ | 1866913578571792384 |
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| author | Reichart, Daniel Solomey, Nickolas |
| author_facet | Reichart, Daniel Solomey, Nickolas |
| contents | The Solar Neutrino and Astro-Particle PhYsics (SNAPPY) Cubesat is expected to launch in 2025 and it will carry into a polar orbit a prototype test detector for solar neutrino background studies while over the Earth's poles for the neutrino Solar Orbiting Laboratory future project ($ν$SOL). During this flight it is possible to do other science measurements. One of these is an improved study of the solar wind particles through better particle identification and energy measurements. This study aimed to understand how well could the solar wind particles be identified using the planned detector but instead of using the veto array as an anti-coincidence it would be used as a $Δ$E energy sampling of a phoswich particle ID system. |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2411_08170 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Simulation of Solar Wind Charged Particle Energy Deposited and Particle Identification by $Δ$E-E Discrimination in the SNAPPY Cubesat Detector Reichart, Daniel Solomey, Nickolas Solar and Stellar Astrophysics Instrumentation and Methods for Astrophysics Instrumentation and Detectors Plasma Physics Space Physics The Solar Neutrino and Astro-Particle PhYsics (SNAPPY) Cubesat is expected to launch in 2025 and it will carry into a polar orbit a prototype test detector for solar neutrino background studies while over the Earth's poles for the neutrino Solar Orbiting Laboratory future project ($ν$SOL). During this flight it is possible to do other science measurements. One of these is an improved study of the solar wind particles through better particle identification and energy measurements. This study aimed to understand how well could the solar wind particles be identified using the planned detector but instead of using the veto array as an anti-coincidence it would be used as a $Δ$E energy sampling of a phoswich particle ID system. |
| title | Simulation of Solar Wind Charged Particle Energy Deposited and Particle Identification by $Δ$E-E Discrimination in the SNAPPY Cubesat Detector |
| topic | Solar and Stellar Astrophysics Instrumentation and Methods for Astrophysics Instrumentation and Detectors Plasma Physics Space Physics |
| url | https://arxiv.org/abs/2411.08170 |