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Journal of the Optical Society of America A, 2003
A formula to compute the index of stellar scintillation detected with a finite spectral bandpass and with arbitrary aperture is derived in the limit of weak perturbations. It also applies to differential scintillation (relative fluctuations of light intensity in a pair of apertures), where the effect of finite bandpass turns out to be significant.
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A formula to compute the index of stellar scintillation detected with a finite spectral bandpass and with arbitrary aperture is derived in the limit of weak perturbations. It also applies to differential scintillation (relative fluctuations of light intensity in a pair of apertures), where the effect of finite bandpass turns out to be significant.
openaire +2 more sources
Influence of Isomerism on Radioluminescence of Purely Organic Phosphorescence Scintillators
Angewandte Chemie - International Edition, 2021Huifang Shi, Wenbo Ma, Qiushui Chen
exaly
Aqueous-Based Inorganic Colloidal Halide Perovskites Customizing Liquid Scintillators
Advanced Materials, 2023Huiwang Lian, Chong-Geng Ma, Rui Zou
exaly
Perovskite Scintillators for Improved X-Ray Detection and Imaging
Angewandte Chemie - International Edition, 2023Shuao Wang, Yaxing Wang, Yumin Wang
exaly
Halide Perovskite, a Potential Scintillator for X-Ray Detection
Small Methods, 2020Wei Lan, Liming Ding, Zhiwen Jin
exaly

