Strontium Iodide Radiation Instrument (SIRI) -- Early On-Orbit Results
Lee J. Mitchell, Bernard F. Phlips, J. Eric Grove, Theodore Finne,, Mary Johnson-Rambert, W. Neil Johnson

TL;DR
SIRI is a space-based gamma-ray spectrometer testing europium-doped strontium iodide and silicon photomultiplier technology, demonstrating promising on-orbit performance and improved energy resolution over traditional scintillators.
Contribution
This paper reports the first on-orbit use of SrI2:Eu scintillator with SiPM readouts, validating its effectiveness for space radiation detection.
Findings
SrI2:Eu provides a feasible alternative to traditional scintillators.
Spectroscopic resolution of 4.3% at 662 keV achieved.
Over 1000 hours of operational data collected by April 2019.
Abstract
The Strontium Iodide Radiation Instrument (SIRI) is a single detector, gamma-ray spectrometer designed to space-qualify the new scintillation detector material europium-doped strontium iodide (SrI2:Eu) and new silicon photomultiplier (SiPM) technology. SIRI covers the energy range from 0.04-8 MeV and was launched into 600 km sun-synchronous orbit on Dec 3, 2018 onboard STPSat5 with a one-year mission to investigate the detector's response to on-orbit background radiation. The detector has an active volume of 11.6 cm3 and a photo fraction efficiency of 50% at 662 keV for gamma-rays parallel to the long axis of the crystal. Its spectroscopic resolution of 4.3% was measured by the FWHM of the characteristic Cs-137 gamma-ray line at 662 keV. Measured background rates external to the trapped particle regions are 40-50 counts per second for energies greater than 40 keV and are largely the…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
