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Numerical simulation of an energy deposition zone in quiescent air and in a supersonic flow under the conditions of interaction with a normal shock

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Abstract

The potential of using the Euler equations to numerically simulate the evolution of localized energy deposition zones interacting with a normal shock in quiescent air and in a supersonic channel flow is demonstrated. Simulation results are compared with available experimental data for an optical discharge in quiescent air and with results calculated for a supersonic flow using the Navier-Stokes equations with allowance for real gas effects. The possibility of predicting gasdynamic effects using the T- and q-models of energy deposition for perfect gas is justified. The variation of the gasdynamic structure and flow parameters near an energy deposition zone developing in a quiescent medium and interacting with a normal shock is analyzed in detail for different energy deposition powers.

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Authors and Affiliations

  1. Khristianovich Institute of Theoretical and Applied Mechanics, Siberian Branch, Russian Academy of Sciences, Institutskaya ul. 4/1, Novosibirsk, 630090, Russia

    A. A. Zheltovodov & E. A. Pimonov

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  1. A. A. Zheltovodov
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  2. E. A. Pimonov
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Correspondence to A. A. Zheltovodov.

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Original Russian Text © A.A. Zheltovodov, E.A. Pimonov, 2013, published in Zhurnal Tekhnicheskoi Fiziki, 2013, Vol. 83, No. 2, pp. 21–35.

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Zheltovodov, A.A., Pimonov, E.A. Numerical simulation of an energy deposition zone in quiescent air and in a supersonic flow under the conditions of interaction with a normal shock. Tech. Phys. 58, 170–184 (2013). https://doi.org/10.1134/S1063784213020278

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