1988
DOI: 10.1088/0022-3727/21/5/012
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Fast photon counting in negative corona discharges in the Trichel regime

Abstract: Using a fast pulse counting system with a time resolution of 0.7 ns, the intensity has been measured of the light originating from a negative corona discharge in the Trichel regime in air, resolved in time, in position in the gap and in wavelength. The dominant spectral lines originate from the second positive system of N2. Both the current and the emission from the plasma carrying the current show a fast increase on a nanosecond timescale and a successive slower decrease. Repetition frequencies are in the MHz… Show more

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Cited by 17 publications
(9 citation statements)
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“…Single-photon counting techniques, where the weak PM signals from the space, time and spectrally resolved light from millions of streamer pulses were superposed, improved the time resolution to 0.3-0.4 ns [24][25][26][27]. Major progress in the spectroscopic studies of the streamer has been made through the works of Marode, Gallimberti, Goldmann, Hartmann and other researchers [28][29][30][31][32][33][34][35][36][37].…”
Section: Introductionmentioning
confidence: 99%
“…Single-photon counting techniques, where the weak PM signals from the space, time and spectrally resolved light from millions of streamer pulses were superposed, improved the time resolution to 0.3-0.4 ns [24][25][26][27]. Major progress in the spectroscopic studies of the streamer has been made through the works of Marode, Gallimberti, Goldmann, Hartmann and other researchers [28][29][30][31][32][33][34][35][36][37].…”
Section: Introductionmentioning
confidence: 99%
“…Time-Correlated Single Photon Counting Spectroscopy Tomáš Hoder approach was motivated by the results of Gallimberti [18] who used these spectral bands to approach the electron energy in the discharge. Similarly, using the SPS emission the Trichel pulse discharge in low pressure negative corona was investigated by Gravendeel [19]. Using the TC-SPC technique, Gravendeel reached the temporal resolution of 0.7 ns in late 80's.…”
Section: Pos(ecpd2015)008mentioning
confidence: 99%
“…Application of the spatially and time-resolved temporal spectral luminosity waveforms for the determination of the physical parameters in the filamentary streamer head is a complicated inverse problem. Rotational spectra and band intensities of the nitrogen second positive (SPS) and first negative (FNS) emission systems have been successively applied for the determination of neutral gas temperature, electric field and electron number density mainly by a direct method [1][2][3][4][5][6][7][8][9][10][11][12][13][14][15][16][17][18][19][20] with a set of different simplifying assumptions.…”
Section: Introductionmentioning
confidence: 99%