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Investigation of thermodynamic state evolution, phase transition and mixing of the hydrocarbon droplet in convective supercritical environments

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... 204 Considering that the system in this study is a binary ammonia-nitrogen system, it is suitable to determine 205 the mode transition time using the criterion based on the temperature-fuel mole fraction (T-x) line versus the 206 vapor-liquid equilibrium (VLE) line proposed by Mo et al [5]. The Peng-Robinson cubic equation of state 207 (PR-EoS) was used to calculate the VLE of the binary system and the critical parameters for ammonia and 208 nitrogen were shown in Table 3. PR-EoS was widely used to calculate the thermodynamic properties of 209 mixture and phase equilibria at high pressures with good reliability [30,35,36]. Recently, Vrabec et al. [37] 210 studied the VLE of ammonia with supercritical gases (Ar, CH4, H2, N2, O2). ...
... The finding indicated that forced convection may have a greater effect on the 275 diffusion mixing process than the classical evaporation process. In the previous studies [27,30], it was found 276 that the high-pressure environment has an inhibitory effect on the supercritical diffusion of fuels. Combined 277 with the above analyses, it was suggested that the negative effect of high pressure on the diffusion and mixing 278 of fuels can be improved by creating a forced convection environment in the actual high-pressure combustion 279 chamber to accelerate the mixing process of fuels. ...
... It meant that forced convection promoted the movement of ammonia molecules in the x-direction. However, 336 there was almost no difference in the trend of the average z-direction velocity component in all cases with 337 temperature, as shown in Fig. 15 364 [30] as shown in Table 5. The supercritical evaporation of n-heptane droplets in forced convective nitrogen 365 environments was simulated by Ai et al [30]. ...
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A comprehensive numerical model is developed to study a vaporizing n-heptane droplet in a forced convective environment under different temperature conditions, which includes high-pressure effects, liquid phase internal circulation, variable thermophysical properties, solubility of inert species into the liquid phase, and gas and liquid phase transients. Numerical predications of time histories of the dimensionless diameter square of a vaporizing fuel droplet within a zero gravity environment are in very good agreement with the micro-gravity experimental data.The numerical results show that at higher ambient pressure (such as 4 MPa) the droplet swells initially due to the heat-up of the cold droplet and its subsequent regression rate is far from following the d2-law during the early stages of droplet evaporation. However, at the ambient pressure of 0.1 MPa, the droplet swells are not obvious. The droplet presents an almost d2-law behavior in later stages of droplet evaporation for all considered pressures (up to 4 MPa). The numerical results also show that the droplet lifetime decreases with increasing ambient temperature. For example, the droplet lifetime at the ambient temperature 1200 K can be only 50–60% of the droplet lifetime at the ambient temperature 600 K. The final penetration distance of the vaporizing droplet decreases almost linearly with the ambient temperatures considered.
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The ‘extended’ and ‘effective-conductivity’ droplet vaporization models developed by Abramzon and Sirignano [Abramzon B, Sirignano WA. Droplet vaporization model for spray combustion calculations. Int J Heat Mass Transfer 1989;32(9):1605–18] are generalized to take into account the contribution of thermal radiation and the temperature dependence of liquid fuel properties. The thermal radiation effect is simulated using the simplified model for thermal radiation absorption suggested by Dombrovsky and Sazhin [Dombrovsky LA, Sazhin SS. Absorption of thermal radiation in a semi-transparent spherical droplet: a simplified model. Int J Heat Fluid Flow 2003;24: 919–27]. Physical properties of liquid fuel, including density, are evaluated at the average liquid temperature and updated at each time-step. These generalized models are applied to the analysis of the vaporization process of n-decane and diesel fuel droplets injected into hot air. It is pointed out that the radiation absorption in diesel fuel is generally stronger than in n-decane, and it needs to be taken into account in modelling the combustion processes in diesel engines. Calculations of the droplet vaporization rate performed using the simplified ‘effective-conductivity’ model with the internal radiation heat source uniformly distributed show exceptionally good agreement with results obtained based on the more accurate ‘extended’ vaporization model with the non-uniform distribution of radiation absorption. This allows us to recommend using the ‘effective-conductivity’ model with uniform radiation absorption for spray combustion calculations, including applications in internal combustion engines.
Article
The differences between subcritical liquid drop and supercritical fluid drop behavior are shown to be a direct consequence of the length scales near the fluid drop boundary. Under subcritical, evaporative high emission rate conditions, a film layer is present in the inner part of the drop surface which contributes to the unique determination of the boundary conditions; it is this film layer in conjunction with evaporation which gives to the solution its convective–diffusive character. In contrast, under supercritical conditions the boundary conditions contain a degree of arbitrariness due to the absence of a physical surface, and the solution has then a purely diffusive character. Results from simulations of a free fluid drop under no-gravity conditions are compared to microgravity experimental data from suspended, large drop experiments at high, low and intermediary temperatures and in a range of pressures encompassing the sub- and supercritical regime. Despite the difference between the conditions of the simulations and the experiments, the time rate of variation of the drop diameter square is remarkably well predicted in the linear curve regime. Consistent with the optical measurements, in the simulations the drop diameter is determined from the location of the maximum density gradient. Detailed time-wise comparisons between simulations and data show that this location is very well predicted at 0.1 MPa. As the pressure increases, the data and simulations agreement becomes good to fair, and the possible reasons for this discrepancy are discussed. Simulations are further conducted for a small drop, such as that encountered in practical applications, over a wide range of specified, constant far field pressures. Additionally, a transient pressure simulation crossing the critical point is also conducted. Results from these simulations are analyzed and major differences between the sub- and supercritical behavior are explained. In particular, it is shown that the classical calculation of the Lewis number gives erroneous results at supercritical conditions, and that an effective Lewis number previously defined gives correct estimates of the length scales for heat and mass transfer at all pressures.
Article
This paper addresses the physiochemical mechanisms involved in transcritical and supercritical vaporization, mixing, and combustion processes in contemporary liquid-fueled propulsion and power-generation systems. Fundamental investigation into these phenomena poses an array of challenges due to the obstacles in conducting experimental measurements and numerical simulations at scales sufficient to resolve the underlying processes. In addition to all of the classical problems for multiphase chemically reacting flows, a unique set of problems arises from the introduction of thermodynamic nonidealities and transport anomalies. The situation becomes even more complex with increasing pressure because of an inherent increase in the flow Reynolds number and difficulties that arise when fluid states approach the critical mixing condition. The paper attempts to provide an overview of recent advances in theoretical modeling and numerical simulation of this subject. A variety of liquid propellants, including hydrocarbon and cryogenic fluids, under both steady and oscillatory conditions, are treated systematically. Emphasis is placed on the development of a hierarchical approach and its associated difficulties. Results from representative studies are presented to lend insight into the intricate nature of the problem.
Article
Evaporation of an individual fuel droplet at high pressures and high temperatures has been studied experimentally under microgravity conditions. A suspended n-heptane droplet was used in the experiments at pressures in the range of 0.1–5.0 MPa and temperatures varying from 400 to 800 K. Temporal variations of the droplet diameter were measured with a computer-aided image analysis system. Microgravity conditions, which were produced by using 5-m and 110-m drop towers and parabolic flights, were employed to prevent natural convection that complicates the phenomena.It was observed that dense fuel vapor surrounded a droplet and the droplet surface became obscure at high pressures and high temperatures. The slope of the temporal variations of the squared droplet diameter initially increases but later becomes approximately constant at ambient pressures below the critical pressure of the fuel. At a pressure of 5.0 MPa and temperatures below the critical temperature, the slope becomes less in the latter half of the evaporation lifetime. The ratio of the initial heat-up time to the evaporation lifetime was used as a measure of unsteadiness of droplet evaporation. The ratio is almost independent of ambient temperature at an ambient pressure of 0.1 MPa, but, as ambient pressure is increased, its tendency to rise with ambient temperature becomes noticeable. Corrected evaporation lifetime tc decreases monotonically as ambient temperature is increased. The slope of its curve becomes steeper as ambient pressure increases. Dependence of tc on ambient pressure changes according to ambient temperature. Above 550 K, tc decreases as ambient pressure is increased. Below 450 K, tc tends to increase as ambient pressure is increased. It is suggested that there exists a certain ambient temperature at which ambient pressure has little effect on tc.
Article
The objective of this research is to improve understanding of the combustion of binary fuel mixtures in the vicinity of the critical point. Fiber-supported droplets of mixtures of n-heptane and n-hexadecane, initially 1 mm in diameter, were burned in room-temperature air at pressures from 1 MPa to 6 MPa under free-fall microgravity conditions. For most mixtures the total burning time was observed to achieve a minimum value at pressures well above the critical pressure of either of the pure fuels. This behavior is explained in terms of critical mixing conditions of a ternary system consisting of the two fuels and nitrogen. The importance of inert-gas dissolution in the liquid fuel near the critical point is thereby re-emphasized, and nonmonotonic dependence of dissolution on initial fuel composition is demonstrated. The results provide information that can be used to estimate high-pressure burning rates of fuel mixtures.