Magnetohydrodynamic Cylindrical Shock in a Rotational Axisymmetric Non-Ideal Gas Under the Action of Monochromatic Radiation

Nath, G.; Sahu, Praveen Kumar; Dutta, Mrityunjoy

doi:10.1016/j.proeng.2015.11.476

Cited by 10 publications

(1 citation statement)

References 17 publications

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“…Vishwakarma and pandey [21] obtained the similarity solution for one-dimensional flow under the action of monochromatic radiation behind a cylindrical magnetogasdynamic shock wave propagating in a non-ideal gas. Nath, sahu and Dutta [22] obtained similarity solution of magnetohydrodynamic cylindrical shock wave in a non-uniform rotating nonideal gas under the action of monochromatic radiation. Nath and Sahu [23] obtained similarity solution of cylindrical shock wave in a rotational axisymmetric non-ideal gas under the action of monochromatic radiation.…”

Section: Introductionmentioning

confidence: 99%

Self similar flow under the action of monochromatic radiation behind a cylindrical shock wave in a self-gravitating, rotating axisymmetric dusty gas

Bajargaan,

Patel

2018

Preprint

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The propagation of a cylindrical shock wave in a self-gravitating, rotating axisymmetric dusty gas under the action of monochromatic radiation with a constant intensity per unit area, which has variable azimuthal and axial components of fluid velocity, is investigated. The gas is assumed to be grey and opaque, and the shock is assumed to be transparent. The dusty gas is considered as a mixture of non-ideal gas and small solid particles, in which solid particles are continuously distributed. To obtain some essential features of shock propagation, small solid particles are considered as a pseudo-fluid, and it is assumed that the equilibrium flow condition is maintained in the entire flow-field. Similarity solutions are obtained as well as the effects of the variation of the radiation parameter, the gravitation parameter, the non-idealness parameter of the gas, the mass concentration of solid particles in the mixture, the ratio of the density of solid particles to the initial density of the gas are worked out in detail. The similarity solution exists under the constant initial angular velocity, and the shock strength is independent from the radiation parameter and the gravitation parameter. It is found that radiation parameter dominates the effect of dusty gas parameters on the variation of radiation heat flux. The total energy of the flow-field behind the shock front is not constant but varies as fourth power of the shock radius.

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Section: Introductionmentioning

confidence: 99%

Self similar flow under the action of monochromatic radiation behind a cylindrical shock wave in a self-gravitating, rotating axisymmetric dusty gas

Bajargaan,

Patel

2018

Preprint

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Motion of Adiabatic or Isothermal Flow Headed by a Magnetogasdynamic Cylindrical Shock Through Rotating Dusty Gas

Sahu¹

2022

Nonlinear Dynamics and Applications

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Effect of Solid Dust Particles on the Propagation of Magnetogasdynamical Shock Waves in a Non-ideal Gas with Monochromatic Radiation

Sahu¹

2022

Mechanisms and Machine Science

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Magnetohydrodynamic Cylindrical Shock in a Rotational Axisymmetric Non-Ideal Gas Under the Action of Monochromatic Radiation

Cited by 10 publications

References 17 publications

Self similar flow under the action of monochromatic radiation behind a cylindrical shock wave in a self-gravitating, rotating axisymmetric dusty gas

Self similar flow under the action of monochromatic radiation behind a cylindrical shock wave in a self-gravitating, rotating axisymmetric dusty gas

Motion of Adiabatic or Isothermal Flow Headed by a Magnetogasdynamic Cylindrical Shock Through Rotating Dusty Gas

Effect of Solid Dust Particles on the Propagation of Magnetogasdynamical Shock Waves in a Non-ideal Gas with Monochromatic Radiation

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