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Wave systems around an accelerated disk

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Shock Waves
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Abstract

When a flat disk is accelerated away from a base plate, a complex flow system can be set up. If the acceleration is rapid this can include the generation of radial and axial shock waves between the disk and the base plate, and a variety of shock/vortex interactions. The patterns are largely influenced by the velocity variation of the disk. Some of the major features of these flows are identified for the impulsive acceleration of a disk to various values of final velocity.

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References

  1. B.J.P. Mortimer, M. Draxl, B.W. Skews: ‘Flow Development around an Electromagnetically Accelerated Free-flying Metal Disk’. In: 22nd International Symposium on Shock Waves, London, ed. by. G.J. Ball, R. Hillier, G.T. Roberts, (University of Southampton 1999) pp. 977–981

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  2. B.W. Skews, C. Law, B.J.R Mortimer: CFD Journal, April 2003, In Press

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  3. L. Felthun: The Modelling of Compressible Euler Flows with Moving Boundaries. PhD Thesis, University of the Witwatersrand, Johannesburg (2002)

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© 2005 Tsinghua University Press and Springer-Verlag Berlin Heidelberg

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Skews, B.W., Law, C. (2005). Wave systems around an accelerated disk. In: Jiang, Z. (eds) Shock Waves. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-540-27009-6_65

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  • DOI: https://doi.org/10.1007/978-3-540-27009-6_65

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-22497-6

  • Online ISBN: 978-3-540-27009-6

  • eBook Packages: Physics and AstronomyPhysics and Astronomy (R0)

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