Characterization of the RaD-X Mission Instruments
Abstract
The NASA Radiation Dosimetry Experiment (RaD-X) stratospheric balloon flight mission, launched on 25 September 2015, provided dosimetric measurements above the Pfotzer maximum. The goal of taking these measurements is to improve aviation radiation models by providing a characterization of cosmic ray primaries, which are the source of radiation exposure at aviation altitudes. The RaD-X science payload consists of four instruments. The main science instrument is a tissue-equivalent proportional counter (TEPC). The other instruments consisted of three solid state silicon dosimeters: Liulin, Teledyne total ionizing dose (TID) and RaySure detectors.To properly interpretate the measurements, it is necessary to evaluate how the payload affects the radiation environment of the detectors. In addition, it is necessary to evaluate how the detectors react to the different particle impacting them.We present the results of the Geant-4 simulations of the interaction of the different radiations with the payload and the instruments, and conclude on how it affect the results of the mission, and which are the instruments better suited for future missions.
- Publication:
-
AGU Fall Meeting Abstracts
- Pub Date:
- December 2016
- Bibcode:
- 2016AGUFMSA41B2374G
- Keywords:
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- 2104 Cosmic rays;
- INTERPLANETARY PHYSICSDE: 2114 Energetic particles;
- INTERPLANETARY PHYSICSDE: 2455 Particle precipitation;
- IONOSPHEREDE: 7984 Space radiation environment;
- SPACE WEATHER