Abstract
A straight, steady-state cross-flow arc is burning in an N2 wind tunnel. The arc is held in position by the balance of the Lorentz forces produced by an external magnetic field perpendicular to the arc axis and by the viscous forces of the gas flow acting on the arc column. The temperature field in the discharge is determined spectroscopically using the radiation of N I lines. Because of the lack of rotational symmetry an inversion method developed by Maldonado was used to determine the local emission coefficient from the measured integrated spectral intensity distributions across the arc in various directions. For known local temperature the mass flow field inside the arc may be evaluated from the convective term of the energy equation and the continuity equation. This is done by expanding the terms of these two equations around the point of the temperature maximum into Fourier-Taylor series and determining coefficients of the same order and power. The solution of the resulting set of algebraic equations yields the unknown coefficients of the mass flow. The flow field obtained by these calculations shows a relatively strong counterflow through the arc core. In the region for which the series expansion holds a partial structure pertaining to a closed double vortex can be recognized.
The terms of the momentum equation are calculated on the basis of these results. In order to obtain a better understanding of the importance attributed to the individual local forces acting on the plasma, a simple model was devised which separates the momentum equation into gradient and curl terms. The discussion shows that the gradient part of the Lorentz force causes mainly the pressure gradient, while the much smaller rotational part of thej×B forces is responsible for propelling the mass flow. The momentum transport inside the arc as well as in its neighbourhood is due to the viscous forces and to the pressure gradient. By contrast, at larger distances from the arc it is essentially the inertial force that determines the momentum transport. It is shown that viscosity as a damping mechanism is necessary for the existence of stationary flow fields as investigated in this work.
Similar content being viewed by others
References
H.G.Stäblein: Proc. of the XIII4th I.C.P.I.G., Berlin (1977) (invited paper)
H.L. Dryden, G.B. Schubauer: J. Aeronaut. Sci.14, 221 (1947)
H. Maecker: Z. Phys.136, 119 (1953)
C.D. Maldonado: J. Math. Phys.6, 12 (1965)
C.D.Maldonado, H.N.Olsen: ARL-Report No. 66-0016 (1966)
C.D. Maldonado, H.N. Olsen: J. Opt. Soc. Am.56, 10 (1966)
W.L.Wiese, M.W.Smith, B.M.Glennon: “Atomic Transition Prohabilities”, NBS 4, Vol. I (1966)
H.W. Drawin, P. Felenbok:Data for Plasmas in Local Thermodynamic Equilibrium (Gautier-Villars, Paris 1965)
K.Drellishak et al.: AECD-TDR-64-12, USAF (1964)
A.J. Baker, D.M. Benenson: Proc. IEEE59, 450–457 (1971)
W. Finkelnburg, H. Maecker: InHandbuch der Physik, Vol. 22, ed. by S. Flügge (Springer, Berlin, Göttingen, Heidelberg 1956)
G. Schmitz: Z. Naturforsch.5a, 571 (1950)
U. Plantikow: Z. Phys.237, 388–402 (1970)
M. Capitelli, R.S. Devoto: Phys. Fluids16, 11 (1973)
M. Wurm: private communication
H. Maecker: Proc. IEEE59, 439–449 (1971)
W.T. Lord: J. Fluid Mech.35, 689–709 (1969)
V.R.Malgham, D.M.Benenson: ARL-Report 71-0302, (1971) pp. 147–168