Onset conditions for positive direct current corona discharges in air under the action of photoionization
Creators
- 1. State Key Laboratory of Power System, Department of Electrical Engineering, Tsinghua University, Beijing 100084 (China)
Description
This paper presents a numerical model for the inception of positive dc corona discharges in air near cylindrical anodes, which plays a bridge role between the classic positive corona onset criterion and the photoionization model considering the effective radiation wavelength. The predicted onset voltages agree well with Peek's experimental data in a wide range of conductor radii and relative air densities. The influence of the collisional quenching of emitting excited states on the surface onset field is significant with low air density or small conductor radius. Within the effective radiation wavelength, numerical expressions for the photon absorption coefficient in air and Townsend's second coefficient due to photoionization are deduced on the basis of the new model. A different perspective on the classic coefficients is given.
Additional details
Identifiers
- DOI
- 10.1063/1.3671970;
Publishing Information
- Journal Title
- Physics of Plasmas
- Journal Volume
- 18
- Journal Issue
- 12
- Journal Page Range
- p. 123503-123503.6
- ISSN
- 1070-664X
- CODEN
- PHPAEN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 44006614
- Subject category
- S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
- Descriptors DEI
- AIR; ANODES; CORONA DISCHARGES; CYLINDRICAL CONFIGURATION; DIRECT CURRENT; ELECTRIC POTENTIAL; EXCITED STATES; NUMERICAL ANALYSIS; PHOTOIONIZATION; PHOTONS; PLASMA; PLASMA DENSITY; PLASMA SIMULATION; QUENCHING
- Descriptors DEC
- BOSONS; CONFIGURATION; CURRENTS; ELECTRIC CURRENTS; ELECTRIC DISCHARGES; ELECTRODES; ELEMENTARY PARTICLES; ENERGY LEVELS; FLUIDS; GASES; IONIZATION; MASSLESS PARTICLES; MATHEMATICS; SIMULATION
Optional Information
- Notes
- (c) 2011 American Institute of Physics