Penetrating particle ANalyzer (PAN)
- NázevTitle
- Penetrating particle ANalyzer (PAN)Penetrating particle ANalyzer (PAN)
- Druh výsledkuResult type
- Článek v časopiseJournal article
- AutořiAuthors
- X. Wu, G. Ambrosi, P. Azzarello, B. Bergmann, S. Pospíšil
- DOIDOI
- 10.1016/j.asr.2019.01.012
- Časopis / citaceJournal / citation
- Advances in Space Research. 2019, 63(8), 2672-2682. ISSN 0273-1177.
- RokYear
- 2019
- JazykLanguage
- eng
- WoSWoS
- 000462690600025
- ScopusScopus
- 2-s2.0-85060678738
- RIVRIV
- RIV/68407700:21670/19:00336845!RIV20-MSM-21670___
- ProjektProject
- Institucionální podpora na rozvoj výzkumné org.Institucionální podpora na rozvoj výzkumné org.
AbstraktAbstract
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 (>similar to 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 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 (>similar to 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.