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Similarity solutions for the flow behind an exponential shock in a non-ideal gas. (English) Zbl 1163.76388

Summary: Similarity solutions for the flow of a non-ideal gas behind a strong exponential shock driven out by a piston (cylindrical or spherical) moving with time according to an exponential law are obtained. Similarity solutions exist only when the surrounding medium is of constant density. Solutions are obtained, in both the cases, when the flow between the shock and the piston is isothermal or adiabatic. It is found that the assumption of zero temperature gradient brings a profound change in the density distribution as compare to that of the adiabatic case. Effects of the non-idealness of the gas on the flow-field between the shock and the piston are investigated. The variations of density-ratio across the shock and the location of the piston with the parameter of non-idealness of the gas \({\overline{b}}\) are also obtained.

MSC:

76L05 Shock waves and blast waves in fluid mechanics
76M55 Dimensional analysis and similarity applied to problems in fluid mechanics
76N15 Gas dynamics (general theory)
Full Text: DOI

References:

[1] Parker EN (1963) Interplanetary dynamical processes. Interscience, New York · Zbl 0119.45803
[2] Lee TS, Chen T (1968) Hydromagnetic interplanetary shock waves. Planet Space Sci 16:1483–1502 · doi:10.1016/0032-0633(68)90061-5
[3] Rosenau P, Frankenthal S (1976) Equatorial propagation of axisymmetric magnetohydrodynamic shocks. Phys Fluids 19:1889–1899 · Zbl 0353.76075 · doi:10.1063/1.861424
[4] Director MN, Dabora EK (1977) Predictions of variable energy blast waves. AIAA J 15: 1315–1321 · Zbl 0359.76002 · doi:10.2514/3.60788
[5] Rogers MH (1958) Similarity flows behind strong shock waves. Q J Mech Appl Math 11:411–422 · Zbl 0085.40202 · doi:10.1093/qjmam/11.4.411
[6] Dabora EK (1972) Variable energy blast waves. AIAA J 10:1384–1386 · doi:10.2514/3.6635
[7] Helliwell JB (1969) Self-similar piston problems with radiative heat transfer. J Fluid Mech 37:497–512 · Zbl 0175.51703 · doi:10.1017/S0022112069000693
[8] Sedov LI (1959) Similarity and dimensional methods in mechanics. Academic, New York · Zbl 0121.18504
[9] Mirelsh H (1962) Hypersonic flow over slender bodies associated with power law shocks Adv Appl Mech 7. Academic, New York
[10] Steiner H, Hirschler T (2002) A self-similar solution of a shock propagation in a dusty gas. Eur J Mech B/Fluids 21:371–380 · Zbl 1006.76046 · doi:10.1016/S0997-7546(02)01181-0
[11] Ranga Rao MP, Ramana BV (1976) Unsteady flow of a gas behind an exponential shock. J Math Phy Sci 10:465–476 · Zbl 0364.76052
[12] Higashino F (1983) Characteristic method applied to blast waves in a dusty gas. Z Naturforsch 38a:399–406 · Zbl 0585.76086
[13] Anisimov SI, Spiner OM (1972) Motion of an almost ideal gas in the presence of a strong point explosion. J Appl Math Mech. 36:883–887 · doi:10.1016/0021-8928(72)90144-X
[14] Wu CC, Roberts PH (1993) Shock-wave propagation in a sonoluminescing gas bubble. Phys Rev Lett 70: 3424–3427 · doi:10.1103/PhysRevLett.70.3424
[15] Roberts PH, Wu CC (1996) Structure and stability of a spherical implosion. Phys Lett A213:59–64 · doi:10.1016/0375-9601(96)00082-5
[16] Singh JB, Vishwakarma PR (1983) Unsteady isothermal flow of a gas behind an exponential shock in magnetogasdynamics. Astrophys Space Sci 95:111– 116 · Zbl 0557.76125 · doi:10.1007/BF00661161
[17] Liberman MA, Velikovich AL (1989) Self-similar spherical expansion of a laser plasma or of detonation products into a low-density ambient gas. Phys. Fluids 1:1271–1276 · doi:10.1063/1.859001
[18] Korobeinikov VP (1976) Problems in the theory of point explosion in gases. In: Proceedings of the Steklov institute of mathematics. No.119. American Mathematical Society, Providence, RI
[19] Laumbach DD, Probstein RF (1970) Self-similar strong shocks with radiation in a decreasing exponential atmosphere. Phys Fluids 13:1178–1183 · doi:10.1063/1.1693048
[20] Sachdev PL, Ashraf S (1971) Converging spherical and cylindrical shocks with zero temperature gradient in the rear flow-field. J Appl Math Phys (ZAMP) 22:1095–1102 · Zbl 0246.76073 · doi:10.1007/BF01590878
[21] Ashraf S, Ahmad Z (1975) Approximate analytic solution of a strong shock with radiation near the surface of the star. J Pure Appl Math 6:1090–1098 · Zbl 0367.76060
[22] Zhuravskaya TA, Levin VA (1996) The propagation of converging and diverging shock waves under intense heat exchange conditions. J Appl Math Mech 60: 745–752 · Zbl 0923.76084 · doi:10.1016/S0021-8928(96)00094-9
[23] Landau LD, Lifshitz EM (1958) Course of theoretical physics Statistical physics, vol 5. Pergaman Press, Oxford
[24] Singh RA, Singh JB (1998) Analysis of diverging shock waves in non-ideal gas. Ind J Theor Phys 46:133–138
[25] Ojha SN (2002)Shock waves in non-ideal fluids. Int J Appl Mech Eng 17:445–464 · Zbl 1054.76043
[26] Chandrasekhar S (1939) An introduction to the study of Stellar structure. University Chicago Press, Chicago · JFM 65.1543.02
[27] Vishwakarma JP (2000) Propagation of shock waves in a dusty gas with exponentially varying density. Eur Phys J B 16:369–372 · doi:10.1007/s100510070238
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