http://www.cnr.it/ontology/cnr/individuo/prodotto/ID191873
Radial dependence of surface streamer-channel luminosity: experimental evidence of Gaussian radiative profiles in Ar and N2 (Articolo in rivista)
- Type
- Label
- Radial dependence of surface streamer-channel luminosity: experimental evidence of Gaussian radiative profiles in Ar and N2 (Articolo in rivista) (literal)
- Anno
- 2012-01-01T00:00:00+01:00 (literal)
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#doi
- 10.1088/0963-0252/21/5/055014 (literal)
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- M Simek1 and P F Ambrico2 (literal)
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- http://iopscience.iop.org/0963-0252/21/5/055014 (literal)
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- 1 Department of Pulse Plasma Systems, Institute of Plasma Physics v.v.i., Academy Sciences of the Czech Republic, Za Slovankou 3, 182 00 Prague, Czech Republic
2 Istituto di Metodologie Inorganiche e dei Plasmi-CNR, U.O.S. Bari, via Orabona, 4, 70126 Bari, Italy (literal)
- Titolo
- Radial dependence of surface streamer-channel luminosity: experimental evidence of Gaussian radiative profiles in Ar and N2 (literal)
- Abstract
- Radial distributions of electronically excited species produced during surface streamer propagation were obtained by applying the Abel inverse transform to projected luminosities of single streamers. The streamers were generated in an argon and nitrogen surface coplanar dielectric barrier discharge at atmospheric pressure and their magnified microscopic images were registered with high time resolution. Selected regions of the projected luminosities were processed by the Abel inverse transform procedure based on the Hankel-Fourier method assuming cylindrical symmetry of the streamer channel. Projected as well as Abel-inverted profiles were fitted by Gaussian functions. It is shown that the projected profiles, in addition to the Abel-inverted ones, can be well approximated by the sum of two coaxial Gaussians with two different half-widths and weights. The sharper Gaussian component with higher weight characterizes the radial dependence of the primary cathode-directed streamer-channel luminosity. The second (broader) Gaussian component probably originates either from the pre-breakdown Townsend phase or from the second wave propagating towards the anode. (literal)
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