1993
DOI: 10.1007/bf01589738
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Optical emission spectra from microwave oxygen plasma produced by surfatron discharge

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Cited by 14 publications
(6 citation statements)
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“…The ionic temperature (300 K) is controlled by a Nosé–Hoover thermostat in all of our ( NVT ) simulations. The components of an oxygen plasma are an important issue and have been identified experimentally in a pressure range from 3 to 100 GPa as atomic oxygen (O) and charged molecular oxygen (O 2 + ), on which we focus here.…”
mentioning
confidence: 99%
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“…The ionic temperature (300 K) is controlled by a Nosé–Hoover thermostat in all of our ( NVT ) simulations. The components of an oxygen plasma are an important issue and have been identified experimentally in a pressure range from 3 to 100 GPa as atomic oxygen (O) and charged molecular oxygen (O 2 + ), on which we focus here.…”
mentioning
confidence: 99%
“…24 The ionic temperature (300 K) is controlled by a Nose− Hoover thermostat 25−27 in all of our (NVT) simulations. The components of an oxygen plasma are an important issue and have been identified experimentally in a pressure range from 3 to 100 GPa as atomic oxygen (O) and charged molecular oxygen (O 2 + ), 28 on which we focus here. A first set of simulations targeting the approach of O to a perfect graphene surface has shown that O can stick on the surface, forming a stable epoxy form, which is consistent with previous static calculations.…”
mentioning
confidence: 99%
“…The continuous shape of the spectrum is attributed to hot NPs 21,24 and can be compared to black-body radiation to deduce the NP temperature. 21 Simultaneously, the emission lines of hydrogen ͑H a 656.28 nm, H ␤ Balmer͒, 25 atomic oxygen ͑777.53 nm͒, 26 and single-ionized atomic oxygen ͑718.2 nm͒ 27 originate from water dissociation as it was assumed previously. Furthermore, the intense molecular carbon band heads are emphasized.…”
Section: Resultsmentioning
confidence: 91%
“…During ZnO depositions in O 2 /Ar working gases, strong emission line from an atomic oxygen (O * ) was detected at 777 nm corresponding to 5p-5s transition, and that from an atomic ion of O + was not detected. Emission line from molecular ion of O þ 2 was detected at 526 nm (first negative system) [17]. The 426 nm emission line was selected for excited Ar corresponding to 5p-4s transition.…”
Section: Plasma Diagnostics During Deposition By Optical Emission Spementioning
confidence: 99%