Title:
Progressive wave analysis describing wave motions in radiative magnetogasdynamics

dc.contributor.authorNeelam Gupta
dc.contributor.authorVishnu D. Sharma
dc.contributor.authorBishun D. Pandey
dc.contributor.authorRishi R. Sharma
dc.date.accessioned2026-02-09T09:27:29Z
dc.date.issued1991
dc.description.abstractAn asymptotic analysis has been carried out to study the propagation of weak nonlinear waves in radiative magnetofluids. The progressive wave theory has been used to derive an evolution equation governing the propagation of nonlinear waves. It has been solved for high-frequency domain. The solution indicates the possibility of a wave breaking after a finite time tc known as the critical time of shock formation. Effects of the thermal radiation, magnetic field, and the coupling of the thermal radiation with the magnetic field have been studied. The decay behavior of a wave with a sawtooth profile headed by a weak shock front and ending with a weak discontinuity has been investigated. © American Institute of Aeronautics and Astronautics, Inc., 1991, All rights reserved.
dc.identifier.doi10.2514/3.221
dc.identifier.issn8878722
dc.identifier.urihttps://doi.org/10.2514/3.221
dc.identifier.urihttps://dl.bhu.ac.in/bhuir/handle/123456789/55002
dc.titleProgressive wave analysis describing wave motions in radiative magnetogasdynamics
dc.typePublication
dspace.entity.typeArticle

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