کد مقاله کد نشریه سال انتشار مقاله انگلیسی نسخه تمام متن
1714793 1013340 2014 9 صفحه PDF دانلود رایگان
عنوان انگلیسی مقاله ISI
Experimental investigation on flow patterns of RP-3 kerosene under sub-critical and supercritical pressures
موضوعات مرتبط
مهندسی و علوم پایه سایر رشته های مهندسی مهندسی هوافضا
پیش نمایش صفحه اول مقاله
Experimental investigation on flow patterns of RP-3 kerosene under sub-critical and supercritical pressures
چکیده انگلیسی


• Study the flow problem of kerosene inside cooling channels of scramjets.
• Identify three distinct phase transition phenomena.
• Recognize two new flow patterns under sub-critical pressures.
• Observe the transition process of RP-3 from liquid to supercritical state.

Active cooling with endothermic hydrocarbon fuel is proved to be one of the most promising approaches to solve the thermal problem for hypersonic aircraft such as scramjet. The flow patterns of two-phase flow inside the cooling channels have a great influence on the heat transfer characteristics. In this study, phase transition processes of RP-3 kerosene flowing inside a square quartz-glass tube were experimentally investigated. Three distinct phase transition phenomena (liquid–gas two phase flow under sub-critical pressures, critical opalescence under critical pressure, and corrugation under supercritical pressures) were identified. The conventional flow patterns of liquid–gas two phase flow, namely bubble flow, slug flow, churn flow and annular flow are observed under sub-critical pressures. Dense bubble flow and dispersed flow are recognized when pressure is increased towards the critical pressure whilst slug flow, churn flow and annular flow disappear. Under critical pressure, the opalescence phenomenon is observed. Under supercritical pressures, no conventional phase transition characteristics, such as bubbles are observed. But some kind of corrugation appears when RP-3 transfers from liquid to supercritical. The refraction index variation caused by sharp density gradient near the critical temperature is thought to be responsible for this corrugation.

ناشر
Database: Elsevier - ScienceDirect (ساینس دایرکت)
Journal: Acta Astronautica - Volume 94, Issue 2, February 2014, Pages 834–842
نویسندگان
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