Regenerative cooling is widely used in rocket engines as an efficient cooling method, and nowadays spacecraft shows faster flight speed and greater acceleration. Therefore, the fuel is subjected to large inertial force during flight acceleration or deceleration process. Hence, since it is novel, it is necessary to analyze the thermal performance with large acceleration. To reveal the effect of acceleration on the heat transfer of supercritical methane fuel in the cooling channel, the three-dimensional numerical simulation has been performed with structured mesh. Specifically, the effects of acceleration, mass flux, pressure and ratio of heat flux to mass flux on the flow and heat transfer in the cooling channel have been studied, and the buoyancy parameter (Bo*) and thermal acceleration factor (Kv) have been also employed to analyze the buoyancy effect and thermal acceleration. The results show that at the conditions of low supercritical pressure, low mass flux and large ratio of heat flux to mass flux, the buoyancy effect increases significantly when the acceleration increases from 0 g to 6 g. As a result, the heat transfer is deteriorated gradually, and the average heat transfer coefficient decreases from 3800 to 3000. On the other hand, when the acceleration and heat flux exceed a range, the unstable phenomenon of thermal oscillation will occur with the period of oscillation about 90 s. The thermophysical properties of the fluid near-wall will change rapidly when approaching the pseudo-critical region, which leads to the continuous change of the thickness of the viscous boundary layer.
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