AVS 45th International Symposium
    Selected Energy Epitaxy Topical Conference Wednesday Sessions
       Session SE-WeA

Paper SE-WeA3
Flow Characteristics of a UHV Nitrogen Arcjet

Wednesday, November 4, 1998, 2:40 pm, Room 327

Session: Novel Sources for Selected Energy Growth
Presenter: C.H. Chang, Thermosciences Institute
Authors: C.H. Chang, Thermosciences Institute
F.J. Grunthaner, Jet Propulsion Laboratory
R. Bicknell-Tassiuis, Jet Propulsion Laboratory
P. Deelman, Jet Propulsion Laboratory
P.J. Grunthaner, Jet Propulsion Laboratory
J.L. Giuliani, Naval Research Laboratory
J.P. Apruzese, Naval Research Laboratory
P. Kepple, Naval Research Laboratory
Correspondent: Click to Email

Flow characteristics in the nozzle of a nitrogen arcjet have been simulated by a model. Electrons, ions, and neutral atoms and molecules are represented as separate species. Dissociation, ionization, and recombination are treated as separate reactions. Thermal non-equilibrium is represented by a two-temperature model. Energy input to plasma from the arc is modeled as a source determined by local current and electrical conductivity. Momentum and energy losses and recombinations at the nozzle wall are included as source/sink determined by fluxes to the wall. The results show essentially frozen gas-phase reactions and thermal nonequilibrium due to Joule heating of electrons and in the expansion part of the nozzle. Wall interactions have strong effects on the results, indicating that they play important roles in the flow due to very high surface area relative to the volume of the plasma. For example, plasma velocity decreases from 6000 m/s without wall interactions to 3000 m/s with modest amount of wall interactions. These results also show reasonable agreement with optical emission measurements, which confirms that the arcjet plasma is far from LTE. The spectra suggest nitrogen dissociation levels of 0.3% - 9%, depending on nitrogen flow rate and arc plasma current, which also determine the relative amounts of excited atomic and molecular nitrogen. Langmuir probe studies of the source show that electron and ion fluxes increase with increasing power, and that the ion energy distribution shifts to lower energies. Typical ion fluxes were on the order of 4E-9 A/cm@super 2@ with a maximum ion kinetic energy of 3.5eV. The median electron energy was 1eV, with a maximum of less than 4eV.