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On Spatial Hydromagnetic Flows
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Intrinsic equations of gasdynamics, magnetogasdynamics, and relativistic gas have been investigated by various authors [2, 3, 5-8, 10]. Truesdell [10], transforming the basic equations governing the motion of the gas flows into instrinsic form, has studied their physical and geometrical properties. Kanwal [2, 3] has discussed the variations of flow quantities of gasdynamics and magnetogasdynamics along streamlines, magneticlines, and their principal normals and binormals. Purushotham [7] has established the relations existing between the flow parameters of steady, viscous, incompressible flows.
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