[7] Nath, G.:
Self-similar solutions for unsteady flow behind an exponential shock in an axisymmetric rotating dusty gas. Shock Waves 24 (2014), 415-428.
DOI 10.1007/s00193-013-0474-3 |
MR 3357255
[8] Nath, G., Sahu, P. K., Chaurasia, S.:
Self-similar solution for the flow behind an exponential shock wave in a rotational axisymmetric non-ideal gas with magnetic field. Chinese J. Phys. 58 (2019), 280-293.
DOI 10.1016/j.cjph.2019.02.007
[10] Palo, N. D., Jena, J., Chadha, M.:
An analytical approach to study kinematics of shock waves in a dusty, cylindrical gas flow. ZAMM, Z. Angew. Math. Mech. 102 (2022), Article ID e202200019, 20 pages.
DOI 10.1002/zamm.202200019 |
MR 4559166
[13] Sahu, P. K.:
Propagation of an exponential shock wave in a rotational axisymmetric isothermal or adiabatic flow of a self-gravitating non-ideal gas under the influence of axial or azimuthal magnetic field. Chaos Solitons Fractals 135 (2020), Article ID 109739, 22 pages.
DOI 10.1016/j.chaos.2020.109739 |
MR 4083012 |
Zbl 1489.76034
[17] Vishwakarma, J. P., Nath, G.:
Similarity solution for a cylindrical shock wave in a rotational axisymmetric dusty gas with heat conduction and radiation heat flux. Commun. Nonlinear Sci. Numer. Simul. 17 (2012), 154-169.
DOI 10.1016/j.cnsns.2011.04.021 |
MR 2825996 |
Zbl 1242.76106