Please wait a minute...
Chin. Phys. B, 2021, Vol. 30(7): 074701    DOI: 10.1088/1674-1056/abf7ad
ELECTROMAGNETISM, OPTICS, ACOUSTICS, HEAT TRANSFER, CLASSICAL MECHANICS, AND FLUID DYNAMICS Prev   Next  

Investigation of hypersonic flows through a cavity with sweepback angle in near space using the DSMC method

Guangming Guo(郭广明), Hao Chen(陈浩), Lin Zhu(朱林), and Yixiang Bian(边义祥)
College of Mechanical Engineering, Yangzhou University, Yangzhou 225127, China
Abstract  Near space has been paid more and more attentionin recent years due to its military application value. However, flow characteristics of some fundamental configurations (e.g., the cavity) in near space have rarely been investigated due to rarefied gas effects, which make the numerical simulation methods based on continuous flow hypothesis lose validity. In this work, the direct simulation Monte Carlo (DSMC), one of the most successful particle simulation methods in treating rarefied gas dynamics, is employed to explore flow characteristics of a hypersonic cavity with sweepback angle in near space by considering a variety of cases, such as the cavity at a wide range of altitudes 20-60 km, the cavity at freestream Mach numbers of 6-20, and the cavity with a sweepback angle of 30°-90°. By analyzing the simulation results, flow characteristics are obtained and meanwhile some interesting phenomena are also found. The primary recirculation region, which occupies the most area of the cavity, causes pressure and temperature stratification due to rotational motion of fluid inside it, whereas the pressure and temperature in the secondary recirculation region, which is a small vortex and locates at the lower left corner of the cavity, change slightly due to low-speed movement of fluid inside it. With the increase of altitude, both the primary and secondary recirculation regions contract greatly and it causes them to separate. A notable finding is that rotation direction of the secondary recirculation region would be reversed at a higher altitude. The overall effect of increasing the Mach number is that the velocity, pressure, and temperature within the cavity increase uniformly. The maximum pressure nearby the trailing edge of the cavity decreases rapidly as the sweepback angle increases, whereas the influence of sweepback angle on velocity distribution and maximum temperature within the cavity is slight.
Keywords:  flow characteristics      cavity with sweepback angle      hypersonic flow      near space      DSMC  
Received:  16 February 2021      Revised:  02 April 2021      Accepted manuscript online:  14 April 2021
PACS:  47.27.nd (Channel flow)  
  47.40.Ki (Supersonic and hypersonic flows)  
  47.11.Mn (Molecular dynamics methods)  
  47.45.-n (Rarefied gas dynamics)  
Fund: Project partly supported by the National Natural Science Foundation of China (Grant No. 11802264) and the Natural Science Foundation of Jiangsu Province, China (Grant No. BK20180896).
Corresponding Authors:  Guangming Guo     E-mail:  gmguo@yzu.edu.cn

Cite this article: 

Guangming Guo(郭广明), Hao Chen(陈浩), Lin Zhu(朱林), and Yixiang Bian(边义祥) Investigation of hypersonic flows through a cavity with sweepback angle in near space using the DSMC method 2021 Chin. Phys. B 30 074701

[1] Curran E T 2001 J. Propuls. Power 17 1138
[2] Huang W 2016 Aerosp. Sci. Technol. 50 183
[3] Drummond J P, Carpenter M H and Riggins D W 1991, Mixing and Mixing Enhancement in Supersonic Reacting Flow Fields, High Speed Propulsion Systems (Progress in Astronautics and Aeronautics), Vol. 137, S. N. B. Murthy and E. T. Curran, eds., American Institute of Aeronautics and Astronautics, Chap. 7, pp. 383-455
[4] Seiner J M, Dash S M and Kenzakowski D C 2001 J. Propuls. Power 17 1273
[5] Zhang Q H, Zhu T, Yi S H and Wu A P 2016 Chin. Phys. B 25 054701
[6] Wei B X, Chen B, Yan M L, Shi X X, Zhang Y and Xu X 2012 Acta Astronaut. 81 102
[7] Manna P, Behera R and Chakraborty D 2008 J. Propuls. Power 24 274
[8] Bushne D M 1995 J. Propuls. Power 11 1088
[9] Mishra D P and Sridhar K V 2012 J. Aerospace. Eng. 25 161
[10] Vinha N, Meseguer-Garrido F, Vicente J and Valero E 2016 Aerosp. Sci. Technol. 52 198
[11] Ozalp C, Pinarbasi A and Sahin B 2010 Exp Therm Fluid Sci 34 505
[12] Luo S B, Huang W, Liu J and Wang Z G 2011 Sci. China: Technol. Sci. 54 1345
[13] Huang W, Pourkashanian M, Ma L, Ingham D B, Luo S B and Wang Z G 2012 Aerosp. Sci. Technol. 21 24
[14] Jin Y, He X M, Jiang B, Wu Z J, Ding G Y and Zhu Z X 2014 Aerosp. Sci. Technol. 32 10
[15] Jin X H, Wang B, Cheng X L, Wang Q and Huang F 2021 Aerosp. Sci. Technol. 110 106498
[16] Huang W, Wang Z G, Liang J and Liu J 2011 J. Vis. 14 339
[17] Walker S H and Rodgers F 2005 The 13th AIAA Conference 2005-3253
[18] Gerdroodbary M B, Imani M and Ganji D D 2014 Aerosp. Sci. Technol. 39 652
[19] Chandra Murty M S R., Bhandarkar A V and Chakraborty D 2016 Aerosp. Sci. Technol. 50 266
[20] Bird G A 1994 Molecular Gas Dynamics and the Direct Simulation of Gas Flows (New York: Oxford) p. 383
[21] Schwartzentruber T E and Boyd I D 2006 J. Comput. Phys. 215 402
[22] Ren W, Liu H and Jin S 2014 J. Comput. Phys. 276 380
[23] Li L Y, Ren W and Zhang B 2014 J. Aeronaut. Astronaut. Aviat. 46 88
[24] Betelin V B, Kushnirenko A G, Smirnov N N, Nikitin V F, Tyurenkova V V and Stamov L I 2018 Acta Astronaut. 144 363
[25] Liu C F and Ni Y S 2008 Chin. Phys. B 17 4554
[26] Guo G M and Luo Q 2018 Int. J. Mech. Sci. 148 496
[27] Guo G M and Luo Q 2019 Acta Astronaut. 161 87
[28] Chen H, Zhang B and Liu H 2016 J. Spacecraft Rockets 53 619
[29] Zhang B, Chen H, Li L Y and Shao X Y 2018 J. Thermophys. Heat Tr. 32 205
[30] Guo G M, Liu H and Zhang B 2017 Acta Astronaut. 132 256
[31] Chen H, Zhang B and Liu H 2019 Phys.Fluids 31 076102
[32] Guo G M, Luo Q, Zhu L and Bian Y X 2019 Chin. Phys. B 28 064702
[33] Palharini R C and Santos W F N 2019 Aerosp. Sci. Technol. 88 110
[34] Lofthouse A J, Boyd I D and Wright M J 2007 Phys. Fluids 19 027105
[35] Guo G M, Liu H, Zhang B, Zhang Z Y and Zhang Q B 2016 Acta Phys. Sin. 65 074702 (in Chinese)
[1] Numerical simulation of metal evaporation based on the kinetic model equation and the direct simulation Monte Carlo method
Xiaoyong Lu(卢肖勇), Xiaozhang Zhang(张小章), Zhizhong Zhang(张志忠). Chin. Phys. B, 2018, 27(12): 124702.
[2] Analytical approximate solution for nonlinear space-time fractional Klein–Gordon equation
Khaled A. Gepreel, Mohamed S. Mohamed. Chin. Phys. B, 2013, 22(1): 010201.
No Suggested Reading articles found!