# Strontium Iodide Radiation Instrument (SIRI) -- Early On-Orbit Results

**Authors:** Lee J. Mitchell, Bernard F. Phlips, J. Eric Grove, Theodore Finne,, Mary Johnson-Rambert, W. Neil Johnson

arXiv: 1907.11364 · 2019-07-29

## 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.

## Key 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 result of short- and long-term activation products generated by transits of the SAA and the continual cosmic-ray bombardment. Rate maps determined from energy cuts of the collected spectral data show the expected contributions from the various trapped particle regions. Early spectra acquired by the instrument show the presence of at least 10 characteristic gamma-ray lines and a beta continuum generated by activation products within the detector and surrounding materials. As of April 2019, the instrument has acquired over 1000 hours of data and is expected to continue operations until the space vehicle is decommissioned in Dec. 2019. Results indicate SrI2:Eu provides a feasible alternative to traditional sodium iodide and cesium iodide scintillators, especially for missions where a factor-of-two improvement in energy resolution would represent a significant difference in scientific return. To the best of our knowledge, SIRI is the first on-orbit use of SrI2:Eu scintillator with SiPM readouts.

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Source: https://tomesphere.com/paper/1907.11364