Skip to main content
U.S. Department of Energy
Office of Scientific and Technical Information

ULTIMATE AND SECONDARY ELECTRON ENERGIES IN THE NEGATIVE GLOW OF A COLD- CATHODE DISCHARGE IN HELIUM

Journal Article · · Journal of Applied Physics (U.S.)
DOI:https://doi.org/10.1063/1.1735620· OSTI ID:4201064
The "ultimate" electron density in the negative glow plasma of a cold- cathode discharge in helium at gas pressures 3-12 mm Hg was determined by simultaneous Langmuir probe and microwave transmission methods. A correlation is obtained at densities above approximately 4 x 10/sup 11/ /cm/sup 3/ when the influence of positive ion scattering of the electrons diffusing to the probe is considered, The ultimate electron temperature in the helium negative glow was measured by the metallic probe to be quite low, approximately 400 ction prod- K and the "secondary" electron temperature was found to be approximately 50,000 ction prod- K. These probe indications are substantiated by measurement of the microwave noise power radiated from the plasma which is found to correspond to an effective temperature varying from 300 to approximately 1000 ction prod- K. (auth)
Research Organization:
General Electric Research Lab., Schenectady, N.Y.
Sponsoring Organization:
USDOE
NSA Number:
NSA-14-011215
OSTI ID:
4201064
Journal Information:
Journal of Applied Physics (U.S.), Journal Name: Journal of Applied Physics (U.S.) Vol. Vol: 31; ISSN JAPIA
Country of Publication:
Country unknown/Code not available
Language:
English

Similar Records

Character of helium excitation in the negative glow of a glow discharge
Journal Article · Sun Nov 30 23:00:00 EST 1975 · Opt. Spectrosc. (USSR) (Engl. Transl.), v. 39, no. 6, pp. 594-597 · OSTI ID:4020371

Electron density and temperature in the pulsed-orbitron-maser glow discharge
Journal Article · Thu Mar 31 23:00:00 EST 1988 · IEEE Trans. Plasma Sci.; (United States) · OSTI ID:7155076

Transmission characteristics of microwave in a glow-discharge dusty plasma
Journal Article · Fri Jul 15 00:00:00 EDT 2016 · Physics of Plasmas · OSTI ID:22600033