Ov. Aleksandrova et Kv. Bychkov, RADIATIVE COOLING OF A SHOCK WITH ACCOUNT FOR ELECTRON HEAT-CONDUCTION AND ENERGY-EXCHANGE BETWEEN IONS AND ELECTRONS, Astronomy reports, 42(4), 1998, pp. 469-475
A solution is found for stationary radiative cooling of a planar, one-
dimensional flow of ionized hydrogen through the front of a shock wave
. The energy exchange between electrons and protons, electron heat con
duction, and bremsstrahlung cooling are taken into account. The veloci
ty of the unperturbed gas relative to the front is taken to be in the
interval 3000 km/s < u(0) < 10 000 km/s. The calculated radiation spec
trum is presented in the form of the dependence of the color temperatu
re on the photon energy E in the interval 0.5 keV < E < 10 keV. The co
lor temperature grows monotically with E, but remains substantially lo
wer than the shock-front temperature.