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Penetrating particle ANalyzer (PAN)

PAN is a scientific instrument suitable for deep space and interplanetary missions. It can precisely measure and monitor the flux, composition, and direction of highly penetrating particles ( >∼ 100 MeV/nucleon) in deep space, over at least one full solar cycle (11 years). The science program of...

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Detalles Bibliográficos
Autores principales: Wu, X., Ambrosi, G., Azzarello, P., Bergmann, B., Bertucci, B., Cadoux, F., Campbell, M., Duranti, M., Ionica, M., Kole, M., Krucker, S., Maehlum, G., Meier, D., Paniccia, M., Pinsky, L., Plainaki, C., Pospisil, S., Stein, T., Thonet, P.A., Tomassetti, N., Tykhonov, A.
Lenguaje:eng
Publicado: 2019
Materias:
Acceso en línea:https://dx.doi.org/10.1016/j.asr.2019.01.012
http://cds.cern.ch/record/2688108
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author Wu, X.
Ambrosi, G.
Azzarello, P.
Bergmann, B.
Bertucci, B.
Cadoux, F.
Campbell, M.
Duranti, M.
Ionica, M.
Kole, M.
Krucker, S.
Maehlum, G.
Meier, D.
Paniccia, M.
Pinsky, L.
Plainaki, C.
Pospisil, S.
Stein, T.
Thonet, P.A.
Tomassetti, N.
Tykhonov, A.
author_facet Wu, X.
Ambrosi, G.
Azzarello, P.
Bergmann, B.
Bertucci, B.
Cadoux, F.
Campbell, M.
Duranti, M.
Ionica, M.
Kole, M.
Krucker, S.
Maehlum, G.
Meier, D.
Paniccia, M.
Pinsky, L.
Plainaki, C.
Pospisil, S.
Stein, T.
Thonet, P.A.
Tomassetti, N.
Tykhonov, A.
author_sort Wu, X.
collection CERN
description PAN is a scientific instrument suitable for deep space and interplanetary missions. It can precisely measure and monitor the flux, composition, and direction of highly penetrating particles ( >∼ 100 MeV/nucleon) in deep space, over at least one full solar cycle (11 years). The science program of PAN is multi- and cross-disciplinary, covering cosmic ray physics, solar physics, space weather and space travel. PAN will fill an observation gap of galactic cosmic rays in the GeV region, and provide precise information of the spectrum, composition and emission time of energetic particle originated from the Sun. The precise measurement and monitoring of the energetic particles is also a unique contribution to space weather studies. PAN will map the flux and composition of penetrating particles, which cannot be shielded effectively, precisely and continuously, providing valuable input for the assessment of the related health risk, and for the development of an adequate mitigation strategy. PAN has the potential to become a standard on-board instrument for deep space human travel. PAN is based on the proven detection principle of a magnetic spectrometer, but with novel layout and detection concept. It will adopt advanced particle detection technologies and industrial processes optimized for deep space application. The device will require limited mass (20 kg) and power (20 W) budget. Dipole magnet sectors built from high field permanent magnet Halbach arrays, instrumented in a modular fashion with high resolution silicon strip detectors, allow to reach an energy resolution better than 10% for nuclei from H to Fe at 1 GeV/n. The charge of the particle, from 1 (proton) to 26 (Iron), can be determined by scintillating detectors and silicon strip detectors, with readout ASICs of large dynamic range. Silicon pixel detectors used in a low power setting will maintain the detection capabilities for even the strongest solar events. A fast scintillator with silicon photomultiplier (SiPM) readout will provide timing information to determine the entering direction of the particle, as well as a high rate particle counter. Low noise, low power and high density ASIC will be developed to satisfy the stringent requirement of the position resolution and the power consumption of the tracker.
id oai-inspirehep.net-1725457
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2019
record_format invenio
spelling oai-inspirehep.net-17254572022-01-15T03:03:32Zdoi:10.1016/j.asr.2019.01.012http://cds.cern.ch/record/2688108engWu, X.Ambrosi, G.Azzarello, P.Bergmann, B.Bertucci, B.Cadoux, F.Campbell, M.Duranti, M.Ionica, M.Kole, M.Krucker, S.Maehlum, G.Meier, D.Paniccia, M.Pinsky, L.Plainaki, C.Pospisil, S.Stein, T.Thonet, P.A.Tomassetti, N.Tykhonov, A.Penetrating particle ANalyzer (PAN)astro-ph.IMAstrophysics and Astronomyphysics.space-phOther Fields of PhysicsPAN is a scientific instrument suitable for deep space and interplanetary missions. It can precisely measure and monitor the flux, composition, and direction of highly penetrating particles ( >∼ 100 MeV/nucleon) in deep space, over at least one full solar cycle (11 years). The science program of PAN is multi- and cross-disciplinary, covering cosmic ray physics, solar physics, space weather and space travel. PAN will fill an observation gap of galactic cosmic rays in the GeV region, and provide precise information of the spectrum, composition and emission time of energetic particle originated from the Sun. The precise measurement and monitoring of the energetic particles is also a unique contribution to space weather studies. PAN will map the flux and composition of penetrating particles, which cannot be shielded effectively, precisely and continuously, providing valuable input for the assessment of the related health risk, and for the development of an adequate mitigation strategy. PAN has the potential to become a standard on-board instrument for deep space human travel. PAN is based on the proven detection principle of a magnetic spectrometer, but with novel layout and detection concept. It will adopt advanced particle detection technologies and industrial processes optimized for deep space application. The device will require limited mass (20 kg) and power (20 W) budget. Dipole magnet sectors built from high field permanent magnet Halbach arrays, instrumented in a modular fashion with high resolution silicon strip detectors, allow to reach an energy resolution better than 10% for nuclei from H to Fe at 1 GeV/n. The charge of the particle, from 1 (proton) to 26 (Iron), can be determined by scintillating detectors and silicon strip detectors, with readout ASICs of large dynamic range. Silicon pixel detectors used in a low power setting will maintain the detection capabilities for even the strongest solar events. A fast scintillator with silicon photomultiplier (SiPM) readout will provide timing information to determine the entering direction of the particle, as well as a high rate particle counter. Low noise, low power and high density ASIC will be developed to satisfy the stringent requirement of the position resolution and the power consumption of the tracker.PAN is a scientific instrument suitable for deep space and interplanetary missions. It can precisely measure and monitor the flux, composition, and direction of highly penetrating particles ($> \sim$100 MeV/nucleon) in deep space, over at least one full solar cycle (~11 years). The science program of PAN is multi- and cross-disciplinary, covering cosmic ray physics, solar physics, space weather and space travel. PAN will fill an observation gap of galactic cosmic rays in the GeV region, and provide precise information of the spectrum, composition and emission time of energetic particle originated from the Sun. The precise measurement and monitoring of the energetic particles is also a unique contribution to space weather studies. PAN will map the flux and composition of penetrating particles, which cannot be shielded effectively, precisely and continuously, providing valuable input for the assessment of the related health risk, and for the development of an adequate mitigation strategy. PAN has the potential to become a standard on-board instrument for deep space human travel. PAN is based on the proven detection principle of a magnetic spectrometer, but with novel layout and detection concept. It will adopt advanced particle detection technologies and industrial processes optimized for deep space application. The device will require limited mass (~20 kg) and power (~20 W) budget. Dipole magnet sectors built from high field permanent magnet Halbach arrays, instrumented in a modular fashion with high resolution silicon strip detectors, allow to reach an energy resolution better than 10\% for nuclei from H to Fe at 1 GeV/n.arXiv:1901.04351oai:inspirehep.net:17254572019-01-14
spellingShingle astro-ph.IM
Astrophysics and Astronomy
physics.space-ph
Other Fields of Physics
Wu, X.
Ambrosi, G.
Azzarello, P.
Bergmann, B.
Bertucci, B.
Cadoux, F.
Campbell, M.
Duranti, M.
Ionica, M.
Kole, M.
Krucker, S.
Maehlum, G.
Meier, D.
Paniccia, M.
Pinsky, L.
Plainaki, C.
Pospisil, S.
Stein, T.
Thonet, P.A.
Tomassetti, N.
Tykhonov, A.
Penetrating particle ANalyzer (PAN)
title Penetrating particle ANalyzer (PAN)
title_full Penetrating particle ANalyzer (PAN)
title_fullStr Penetrating particle ANalyzer (PAN)
title_full_unstemmed Penetrating particle ANalyzer (PAN)
title_short Penetrating particle ANalyzer (PAN)
title_sort penetrating particle analyzer (pan)
topic astro-ph.IM
Astrophysics and Astronomy
physics.space-ph
Other Fields of Physics
url https://dx.doi.org/10.1016/j.asr.2019.01.012
http://cds.cern.ch/record/2688108
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