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PAN

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Development of a demonstrator for the Penetrating Particle Analyser PAN techno...

Development of a demonstrator for the Penetrating Particle Analyser PAN technology The goal of the project is to build a demonstrator for the Penetrating Particle Analyser (PAN), an innovative energetic particle detection technology to precisely measure and monitor the flux and composition of highly penetrating... ver más

31/12/2023

UNIGE

3M€

Presupuesto del proyecto: 3M€

Líder del proyecto

UNIVERSITE DE GENEVE No se ha especificado una descripción o un objeto social para esta compañía.

TRL 4-5

Fecha límite participación Sin fecha límite de participación.

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Financiación concedida El organismo H2020 notifico la concesión del proyecto el día 2023-12-31

FETOPEN-01-2018-2019-2020: FET-Open Challenging Current Thinki... Specific Challenge:to lay the foundations for radically new future technologies of any kind from vis...

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Características del participante

Este proyecto no cuenta con búsquedas de partenariado abiertas en este momento.

Información adicional privada

No hay información privada compartida para este proyecto. Habla con el coordinador.

4 Participantes

UNIGE

1.31M€ | Lider

CVUT

512.50K€ | Participante

UNIPG

125.00K€ | Participante

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Duración del proyecto: 52 meses Fecha Inicio: 2019-08-30
Fecha Fin: 2023-12-31

Líder del proyecto

UNIVERSITE DE GENEVE No se ha especificado una descripción o un objeto social para esta compañía.

TRL 4-5

Presupuesto del proyecto 3M€

Fecha límite de participación Sin fecha límite de participación.

Descripción del proyecto The goal of the project is to build a demonstrator for the Penetrating Particle Analyser (PAN), an innovative energetic particle detection technology to precisely measure and monitor the flux and composition of highly penetrating particles (> ~100 MeV/nucleon) in deep space. The application of PAN is broad and multidisciplinary, covering cosmic ray physics, solar physics, space weather and space travel. PAN will fill an observation gap of galactic cosmic rays in the 100 MeV/nucleon - GeV/nucleon region, which is crucial for improving our still limited understanding of the origin of cosmic rays, and their propagation through the Galaxy and the Solar system. It will provide precise information of the spectrum, composition and timing of energetic particle originated from the Sun, which is essential for studying the physical process of solar activities, in particular the rare but violent solar events that produce intensive flux of energetic particles. The precise measurement and monitoring of the penetrating particles is also a unique contribution to space weather studies, in particular to the development of predictive space weather models in a multi-wavelength and multi-messenger approach, using observations both space and ground based. As indicated by the terminology, penetrating particles cannot be shielded effectively. PAN can monitor the flux and composition of these particles precisely and continuously, thus providing real-time radiation hazard warning and long term radiation health risk for human space travelers. Once developed, PAN can become a standard device for deep space human bases and for deep space exploration and commercial spacecrafts, or as part of a space weather advance warning system permanently deployed in space. It can also be implemented on science missions to perform ground-breaking measurements for cosmic-ray physics, solar physics, planetary science and space radiation dosimetry.

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