Publication Date:
2011-08-16
Description:
Shock waves traveling at approximately 16 km/sec into a gas mixture of 7% H2 and 93% He were used to simulate the shock-layer conditions for a representative shallow entry into the Jovian atmosphere. The absolute intensities of line and continuum radiation were measured and the radiative cooling of the shock-heated gas is shown.
Keywords:
THERMODYNAMICS AND COMBUSTION
Type:
Journal of Quantitative Spectroscopy and Radiative Transfer; 13; Oct. 197
Format:
text