Using Hybrid Pixel Radiation Imaging Detectors for Space Radiation Environmental and Dosimetric Applications

1 Jul 2014, 09:00
30m
503/1-001 - Council Chamber (CERN)

503/1-001 - Council Chamber

CERN

503-1-01
162
Show room on map
Oral AMICSA 2014 Keynote

Speaker

Prof. Lawrence Pinsky (University of Houston (US))

Description

While it may seem like a retro-application to use hybrid pixel detectors for applications that consist primarily of observing incident charged particles, given the provenance of these detectors in high energy physics, in actuality the challenges faced are surprisingly novel, at least for these devices. While the space radiation environment consists of mainly charged particles, the routinely seen charges of dosimetric interest range from protons through that of fully ionized iron nuclei, and with energies from stopping to very relativistic. In addition, while their fluxes are not necessarily isotropic, as a practical matter, locally they can appear to be incident from any direction with respect to the detectors. Furthermore, the fluences can vary by many orders of magnitude both in location and time. In the end, the ultimate goal is to characterize the charged particle radiation field as completely as possible in order to be prepared to calculate any potential dosimetric endpoint, and to do so with minimum power and external bandwidth requirements. While devices that enjoy access to spacecraft (or even spacesuit) power, detector stacks with multiple layers can be considered, however for portable battery-powered “film-badge” replacements one is pretty much relegated to a single detector device. Using pattern recognition and an thorough analysis of the pixel cluster created in pixel-based device like the Medipix2 Timepix technology, it is possible to measure the track length of an energetic penetrating charged particle as well as the energy deposited, which leads to knowledge of the Lineal Energy Transferred (LET) to the sensor. Further one can determine the polar and azimuthal angles of the track, and by analyzing the δ-rays for more energetic particle’s tracks the propagation direction can inferred. Likewise the δ-rays can give information about the energy (or more correctly the velocity), which when coupled with the LET can give a reasonable estimate of both the charge and kinetic energy of the particle. Some difficulties that need to be overcome include distinguishing crossing tracks, interactions, and stopping particles as well as having to deal with the huge range of potential input charge per pixel including accurate calibration. Results from 5 Timepix units with over a year and a half in orbit on the International Space Station will be presented.

Primary author

Prof. Lawrence Pinsky (University of Houston (US))

Co-authors

Dr Amir Bahadori (NASA) Daniel Turecek (Czech Technical University (CZ)) Mr Edward Semones (NASA) Mr Hisashi Kitamura (National Institute for Radiological Sciences) Jan Jakubek (Czech Technical University (CZ)) John Paulo Idarraga Munoz (University of Houston (US)) Dr Martin Kroupa (NASA/Wyle Laboratories, Inc.) Mr Nicholas Stoffle (NASA/WYLE INTEG. SCI. & ENG.]) Dr Ryan Rios (NASA/WYLE INTEG. SCI. & ENG) Mr Satoshi Kodaira (National Institute for Radiological Sciences) Dr Son-Minh Hoang (University of Houston) Dr Stanislav Pospisil (Institute of Experimental and Applied Physics, Czech Technical University in Prague) Zdenek Vykydal (Czech Technical University (CZ))

Presentation materials