DC discharge experiment in an Ar/N 2/CO 2 ternary mixture: A laboratory simulation of the Martian ionosphere's plasma environment

Abstract

A low-pressure DC plasma discharge sustained in a 1.6%Ar–2.7%N 2–95.3%CO 2 ternary mixture is studied. This plasma was generated in a total pressure range from 1.0 to 4.0 Torr, a power of 6.3 W and a 12 l/min flow rate of gases. The electron temperature was found to be 8.41 eV and the ion density, in the order of 10 9 cm −3. The species observed in the plasma mixture were CO 2, CO 2 +, CN, CO, CO +, O 2, O 2 +, N 2, N 2 +, NO, C +, Ar and Ar +. At the pressure range in the present study, the species observed do not change their intensity due to an increase in the pressure and they separate in two groups according to their emission intensity: the band of the first group (CO 2, CO 2 + and CN) is approximately a factor of 3 more intense than that of the second group (CO, CO +, O 2, O 2 +, N 2, N 2 +, NO, C +, Ar and Ar +). The behavior of the emission intensities may be correlated to the constant ion density and electron temperature measured. Also, we observed the same constant behavior in the ratios of the neutral and positive species intensities to that of the N 2 intensity, as a function of pressure. This may suggest that the different rate coefficients and cross sections of elastic collision, excitation and de-excitation of electronic or vibrational levels, inelastic and superelastic collisions of electrons with the gas phase and products, neutral–neutral interactions, resonant charged transfer processes, recombination, to mention some, to produce these species change in the same proportion, as a function of the pressure to keep the relative ratios of the species almost constant.