FALTÝNEK, Jan, Vít KUDRLE, Miroslav ŠNÍRER, Jozef TOMAN and Ondřej JAŠEK. Electron concentration in the non-luminous part of the atmospheric pressure filamentary discharge. Plasma Sources Science and Technology. Bristol: IOP Pub., 2021, vol. 30, No 1, p. 1-16. ISSN 0963-0252. Available from: https://dx.doi.org/10.1088/1361-6595/abcb6b.
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Original name Electron concentration in the non-luminous part of the atmospheric pressure filamentary discharge
Authors FALTÝNEK, Jan (203 Czech Republic, guarantor, belonging to the institution), Vít KUDRLE (203 Czech Republic, belonging to the institution), Miroslav ŠNÍRER (703 Slovakia, belonging to the institution), Jozef TOMAN (703 Slovakia, belonging to the institution) and Ondřej JAŠEK (203 Czech Republic, belonging to the institution).
Edition Plasma Sources Science and Technology, Bristol, IOP Pub. 2021, 0963-0252.
Other information
Original language English
Type of outcome Article in a journal
Country of publisher United Kingdom of Great Britain and Northern Ireland
Confidentiality degree is not subject to a state or trade secret
WWW URL
RIV identification code RIV/00216224:14310/21:00118832
Organization Přírodovědecká fakulta – Repository – Repository
Doi http://dx.doi.org/10.1088/1361-6595/abcb6b
UT WoS 000605909300001
Keywords in English numerical model; atmospheric pressure; filamentary plasma; plasma density; Stark broadening; microwave interferometry; graphene synthesis
Links GA18-08520S, research and development project. CEPLANT, large research infrastructures.
Changed by Changed by: RNDr. Daniel Jakubík, učo 139797. Changed: 28/2/2024 04:01.
Abstract
The non-luminous surroundings of atmospheric pressure plasma jets contain still substantial electron density which can be of practical importance, when e.g. reactant or precursor is introduced into this zone. Low signal-to-noise ratio makes the Stark broadening technique unsuitable there, and so we employed the microwave interferometry to determine the electron density during the plasma synthesis of graphene. The relatively long wavelength, tight geometry and the presence of overcritical plasma filament necessitated the use of a numerical solution of the Maxwell equations. Besides laying the groundwork of the method, the paper also discusses the importance of plasma density profile in the active filament and its surroundings. The results show that in radial distance ten times higher than a visually apparent plasma diameter, the plasma density was still around 1016-1017 m-3.
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