2021
DOI: 10.1016/j.proci.2020.06.193
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Combustion-relevant aerosol phosphor thermometry imaging using Ce,Pr:LuAG, Ce:GdPO4, and Ce:CSSO

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Cited by 9 publications
(11 citation statements)
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“…As noted in [2], Ce:CSSO exhibits a significant amount of host defect emission when excited at 266 nm. To reduce interference and better observe the photophysical properties of the rare-earth ions, the Ce:CSSO and Ce,Pr:CSSO phosphor samples were annealed.…”
Section: Experimental Methods and Materialsmentioning
confidence: 58%
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“…As noted in [2], Ce:CSSO exhibits a significant amount of host defect emission when excited at 266 nm. To reduce interference and better observe the photophysical properties of the rare-earth ions, the Ce:CSSO and Ce,Pr:CSSO phosphor samples were annealed.…”
Section: Experimental Methods and Materialsmentioning
confidence: 58%
“…Singly-doped Pr:CSSO has the brightest emission (before quenching), while Ce 3+ in general has the lowest roomtemperature signal. However, Ce 3+ emission increases up to 950 K and does not quench significantly until 1200 K, making its signal intensity the strongest at temperatures >700 K. In fact, for both the singly-doped and co-doped phosphors the Ce 3+ signal is higher than its room temperature value until at least 1100 K. Therefore, is a viable option for temperature imaging above 1000 K as previously demonstrated for the singlydoped Ce:CSSO [2]. Interestingly, the co-doped and singlydoped Ce 3+ emission intensities are similar above 1000 K after the host and Pr 3+ emissions have quenched significantly.…”
Section: Relative Signalmentioning
confidence: 73%
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