2015
DOI: 10.1366/14-07696
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Laser-Induced Fluorescence from N2+ Ions Generated by a Corona Discharge in Ambient Air

Abstract: In this work, we present the measurement of laser-induced fluorescence from N2(+) ions via the B(2)Σu(+)-X(2)Σg(+) band system in the near-ultraviolet. The ions were generated continuously by a plasma glow discharge in low pressure N2 and by a corona discharge in ambient air. The fluorescence decay time was found to rapidly decrease with increasing pressure leading to an extrapolated decay rate of ≍10(10) s(-1) at atmospheric pressure. In spite of this quenching, we were able to observe laser induced fluoresce… Show more

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Cited by 4 publications
(3 citation statements)
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References 29 publications
(46 reference statements)
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“…In plasma physics, laser-induced fluorescence (LIF) [1,2] is currently the leading method for the detection of radicals, [1,3,4] metastables [5,6] and some ions. [7,8] LIF provides high sensitivity, a low limit of detection and high…”
Section: Introductionmentioning
confidence: 99%
See 1 more Smart Citation
“…In plasma physics, laser-induced fluorescence (LIF) [1,2] is currently the leading method for the detection of radicals, [1,3,4] metastables [5,6] and some ions. [7,8] LIF provides high sensitivity, a low limit of detection and high…”
Section: Introductionmentioning
confidence: 99%
“…In plasma physics, laser‐induced fluorescence (LIF) [ 1,2 ] is currently the leading method for the detection of radicals, [ 1,3,4 ] metastables [ 5,6 ] and some ions. [ 7,8 ] LIF provides high sensitivity, a low limit of detection and high spatial and temporal resolution. Unfortunately, the method can be invasive, especially if high‐energy laser pulses are used, which are required in some cases for reaching a sufficient signal‐to‐noise ratio.…”
Section: Introductionmentioning
confidence: 99%
“…In most cases, alpha contamination is surrounded by air, which typically limits the useful species to N 2 . It is the only species that both is sufficiently abundant and at the same time produces radioluminescence that it is not as strongly affected by O 2 and H 2 O quenching like radioluminescence from most other species is 18,2225 . If, however, one can alter the atmosphere around an alpha emitter, then one is no longer limited to relying on N 2 as luminescent species.…”
Section: Introductionmentioning
confidence: 99%