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Thermal effects on weak waves in a radiative magnetogasdynamic media

dc.contributor.authorRai A.; Gaur M.; Ram R.
dc.date.accessioned2025-05-24T09:56:37Z
dc.description.abstractThe singular surface theory has been used to determine the behavior of weak waves under the combined influence of time-dependent gasdynamic, radiation, and electromagnetic fields. The role of thermal radiation and conduction in the growth or decay of a wave has been studied under a quasiequilibrium and quasi-isotropic hypothesis of the differential approximation to the radiative heat-transfer equation. It is shown that there are two distinct modes of wave propagation, namely, a radiation-induced wave and a modified magnetogasdynamic wave. It is observed that a radiation-induced wave decays rapidly and has a negligibly small influence on the gasdynamic field under the nonrelativistic limit, whereas a magnetogasdynamic wave grows into a shock wave under nonlinear steepening effects. Two cases of diverging and converging waves are discussed to answer the question as to when a shock wave appears. © 1987 American Institute of Aeronautics and Astronautics, Inc., All rights reserved.
dc.identifier.doihttps://doi.org/10.2514/3.9734
dc.identifier.urihttp://172.23.0.11:4000/handle/123456789/21197
dc.relation.ispartofseriesAIAA Journal
dc.titleThermal effects on weak waves in a radiative magnetogasdynamic media

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