RADIATIVE COOLING OF A SHOCK WITH ACCOUNT FOR ELECTRON HEAT-CONDUCTION AND ENERGY-EXCHANGE BETWEEN IONS AND ELECTRONS

Citation
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
Citations number
7
Categorie Soggetti
Astronomy & Astrophysics
Journal title
ISSN journal
10637729
Volume
42
Issue
4
Year of publication
1998
Pages
469 - 475
Database
ISI
SICI code
1063-7729(1998)42:4<469:RCOASW>2.0.ZU;2-P
Abstract
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.