TY - JOUR
T1 - 194 nm microplasma lamps driven by excitation transfer
T2 - Optical sources for the 199Hg ion atomic clock and photochemistry
AU - Park, S.
AU - Mironov, A. E.
AU - Kim, J.
AU - Park, S. J.
AU - Eden, J. G.
N1 - Funding Information:
Valuable discussions with J D Prestage, T Le, T M Hong, and N Yu of the Jet Propulsion Laboratory (JPL: Pasadena, California), as well as their design, construction and testing of the clock physics package, are gratefully acknowledged. We also wish to thank Dr Zhihu Liang of EPL Power Electronics for the design and construction of the pulsed power supplies that made these results possible. This work was supported by Jet Propulsion Laboratory Contract Nos. 1562980 and 1613910 under the Defense Advanced Research Projects Agency (DARPA) Atomic Clock With Enhanced Stability (ACES) Program. SJP also wishes to acknowledge the support of VUV lamp development by the Ministry of Education of the Republic of Korea through the Global Top Environmental Technologies Program.
Publisher Copyright:
© 2022 IOP Publishing Ltd.
PY - 2022/4
Y1 - 2022/4
N2 - A series of miniature, microcavity plasma lamps emitting predominantly at 194 nm has been successfully developed and tested as the optical pump for the microwave 199Hg-ion atomic clock (40.507 GHz), replacing low pressure, RF-powered Ar/Hg discharges. Intense fluorescence on the 6p 2P1/2 → 6s 2S1/2 transition of the singly-charged 202Hg ion at 194.23 nm has been generated in arrays of cylindrical microplasmas through electron-impact excitation of He, followed by three-body formation of He2(a 3 ςu+ ) and Penning ionization of Hg. Emission spectroscopy and kinetic modeling of He/Hg vapor plasmas demonstrate that the population of the Hg+(62P1/2) radiating state (16.82 eV), produced by direct or two-step electron impact processes, is < 1% of that generated by excitation transfer to Hg by H e2∗ . Flat, fused silica lamps having emitting areas as small as 4 mm2 and containing several mg of 202Hg and 50-800 Torr of He have been fabricated and serve as optical drivers for the Hg+ atomic clock cycle. Based on small arrays of 500 μm-1 mm diameter microcavities, these lamps produce peak and average intensities at 194 nm greater than those associated with the Hg resonance transition at ∼254 nm, despite the factor of $?> > 3 difference between the energies of the 6p 3P1 and 6p 2P1/2 states of neutral Hg and Hg+, respectively. These lamps are unique in the sense that the desired radiating species is an excited ion and the background He gas pressure can reach 1 atm, both of which contribute to a dense glow plasma placing severe demands on E/N, power conditioning, and materials selection. Nevertheless, with proper attention given to design, vacuum processing, and preparation of the lamps, lifetimes above 1500 h have been realized to date. When these lamps drive Jet Propulsion Laboratory Hg+ clocks, the stability floor has been measured to be a 1/410 -14. The implications of this lamp for gas-phase and solid-state photochemistry are also discussed.
AB - A series of miniature, microcavity plasma lamps emitting predominantly at 194 nm has been successfully developed and tested as the optical pump for the microwave 199Hg-ion atomic clock (40.507 GHz), replacing low pressure, RF-powered Ar/Hg discharges. Intense fluorescence on the 6p 2P1/2 → 6s 2S1/2 transition of the singly-charged 202Hg ion at 194.23 nm has been generated in arrays of cylindrical microplasmas through electron-impact excitation of He, followed by three-body formation of He2(a 3 ςu+ ) and Penning ionization of Hg. Emission spectroscopy and kinetic modeling of He/Hg vapor plasmas demonstrate that the population of the Hg+(62P1/2) radiating state (16.82 eV), produced by direct or two-step electron impact processes, is < 1% of that generated by excitation transfer to Hg by H e2∗ . Flat, fused silica lamps having emitting areas as small as 4 mm2 and containing several mg of 202Hg and 50-800 Torr of He have been fabricated and serve as optical drivers for the Hg+ atomic clock cycle. Based on small arrays of 500 μm-1 mm diameter microcavities, these lamps produce peak and average intensities at 194 nm greater than those associated with the Hg resonance transition at ∼254 nm, despite the factor of $?> > 3 difference between the energies of the 6p 3P1 and 6p 2P1/2 states of neutral Hg and Hg+, respectively. These lamps are unique in the sense that the desired radiating species is an excited ion and the background He gas pressure can reach 1 atm, both of which contribute to a dense glow plasma placing severe demands on E/N, power conditioning, and materials selection. Nevertheless, with proper attention given to design, vacuum processing, and preparation of the lamps, lifetimes above 1500 h have been realized to date. When these lamps drive Jet Propulsion Laboratory Hg+ clocks, the stability floor has been measured to be a 1/410 -14. The implications of this lamp for gas-phase and solid-state photochemistry are also discussed.
KW - VUV lamps
KW - atomic clocks
KW - excitation transfer
KW - microcavity plasma arrays
KW - microplasma lamps
KW - rare gas excimers
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U2 - 10.1088/1361-6595/ac5c5c
DO - 10.1088/1361-6595/ac5c5c
M3 - Article
AN - SCOPUS:85128928273
SN - 0963-0252
VL - 31
JO - Plasma Sources Science and Technology
JF - Plasma Sources Science and Technology
IS - 4
M1 - 045007
ER -