The investigation hardware consists of a single, integrated sensor and electronics box with simple electronic and mechanical interfaces to the spacecraft. The CRaTER sensor frontend design is based on standard stacked-detector, cosmic ray telescope systems that have been flown for decades, using detectors developed for other NASA flight programs. The analog electronics design is virtually identical to the robust and flight-proven design of the NASA/POLAR Imaging Proton Spectrometer that has been operating flawlessly on orbit since 1996. The digital processing unit is a simple and straightforward design also based on similar instruments with excellent spaceflight heritage. No new technology developments or supporting research are required for the final design, fabrication, and operation of this instrument.

The CRaTER telescope consists of five ion-implanted silicon detectors (red areas), mounted on four detector boards (green areas), and separated by three pieces of tissue-equivalent plastic, hereinafter referred to as TEP (tan areas). All five of the silicon detectors are 2 cm in diameter. Detector 1 is 20 micrometers thick; the other four are 300 micrometers thick. TEP (such as A-150 manufactured by Standard Imaging) simulates soft body tissue (muscle) and has been used for both ground-based as well as space-based (i.e., Space Station) experiments.

Low LET detectors 9.6 cm^2 circular, 1000 microns thick. 0.2 MeV threshold
High LET detectors 9.6 cm^2 circular, 140 microns thick. 2 MeV threshold
TEP absorber 1 5.4 cm cylinder
TEP absorber 2 2.7 cm cylinder
Zenith FOV 35 degrees, 6-detector coincidence
Nadir FOV 75 degrees, for D3D4D5D6 coincidence
Geometry factor 0.1 cm^2 sr (D1D2 events)
LET range 0.2 - 7 MeV/micron (Si)
Incident particle energy range

>20 MeV (H)
>87 MeV/nucleon (Fe)