August 14, 2024
Journal Article

Informing Solar Blind Radioluminescence Imaging through a Calibrated Spectrum

Abstract

While direct radiation detection methods offer great insight into the origin of ionizing particles and photons, their use to locate contaminated areas or concealed radioactive sources can lead to undue exposure of personnel and equipment to ionizing radiation or the potential for contamination. These same sources induce ultraviolet (UV) optical photon fluorescence in air – a process referred to as radioluminescence – that may be imaged from low dose regions over larger attenuation lengths than ionizing radiation. However, most optical detection methods are limited to low lighting conditions to image the more abundant ultraviolet-A (UV-A) photons. To extend this capability to room light or daytime conditions, the solar blind region (Ultraviolet-C (UV-C),

Published: August 14, 2024

Citation

Marshall G.J., C.M. Murzyn, O. Searfus, S.S. Harilal, J.W. Inman, B.S. McDonald, and R.K. Harrison. 2024. Informing Solar Blind Radioluminescence Imaging through a Calibrated Spectrum. Nuclear Instruments and Methods in Physics Research. Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 1067, no. _:Art. No. 169639. PNNL-SA-201328. doi:10.1016/j.nima.2024.169639