Optical observations of the beam-plasma discharge phenomenon

Details Optical observations of the beam-plasma discharge phenomenon Optical observations of the beam-plasma discharge phenomenon

Aug 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993p%26ss...41..633s&link_type=abstract

Planetary and Space Science (ISSN 0032-0633), vol. 41, no. 8, p. 633-639

Physics

3

Beam Injection, Earth Magnetosphere, Electron Beams, Emission Spectra, Optical Measurement, Plasma Jets, Plasmas (Physics), Spectroscopic Analysis, Wave-Particle Interactions, Auroras, Computerized Simulation, Electron Transitions, Energy Levels, Hot Electrons, Ionization, Nitrogen, Optical Emission Spectroscopy

Scientific paper

Spectroscopic observations of optical emissions from the beam-plasma discharge (BPD) phenomenon were made with NASA's vacuum chamber facility, at the Johnson Space Center, configured to simulate the physical conditions of magnetospheric electron beam injection into the ionospheric/upper-atmospheric environment. Nonlinear N2 and N2(+) optical emission growth rates (with respect to incremental electron beam current values) were observed from the chamber gas during transition to the BPD state. For electron-beam currents (I) near the BPD transition value (I(sub c)), the band emissions from the chamber gas produced by relatively low energy (less than or equal to 50 eV) electrons interacting with N2 were anomalously more intense than those requiring higher energy (greater than 100 eV) electrons to excite them. For I more greater than I(sub c), the optical emissions increased linearly with I (as was the case for I less than I(sub c)) and their ratios decreased significantly from the peak values attained when I approximately equals I(sub c). These observations suggest that during BPD some of the energy of the primary electron beam is efficiently transferred, via wave-particle interactions, to local electrons produced through ionization of the chamber gas; the resulting suprathermal electrons provide an additional source of excitation for the relatively low energy states (A, B and C) of N2. Such nonlinear excitation of upper atmospheric gas may occur in certain auroral events wherein the current due to the precipitating electrons approaches a value close to I(sub c).

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