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dc.contributor.advisorBhatnagar, P. L
dc.contributor.authorBhat Pradman Krishen
dc.date.accessioned2025-12-30T09:26:42Z
dc.date.available2025-12-30T09:26:42Z
dc.date.submitted1968
dc.identifier.urihttps://etd.iisc.ac.in/handle/2005/7945
dc.description.abstract(a) Exploding shell: We see that the disturbances in the plasma pressure and velocity grow with time. They manifest in the form of unbounded oscillations with their amplitudes varying as time and frequencies proportional to ?=2a1/2.\Pi = 2a^{1/2}.?=2a1/2. The perturbations in the plasma magnetic field die as they manifest in the form of damped oscillations. The perturbations in the plasma electric field are harmonic with unbounded amplitudes. There are no perturbations in the outer vacuum magnetic field up to the order of approximation. We have solved the problem. The electric field disturbances in this region of the system appear in the form of unbounded oscillations with frequency equal to N. The disturbances in the magnetic field of the inner vacuum die as time advances. The disturbances in the electric field of this region appear in the form of unbounded oscillations with frequency equal to N?. Thus we conclude that the exploding shell is overstable against long wavelength disturbances. The frequency of these growing oscillations depends on the thickness of the shell through a², the initial magnetic field and the rate of explosion through 2, and on the initial radii of the shell through m. (b) Imploding shell: Here we note that the disturbances in the plasma pressure, velocity and electric field grow as the shell collapses, the growth rate of the instability being proportional to N=a1/2.N = a^{1/2}.N=a1/2. Similarly, the disturbance in the electric field in the outside vacuum grows as fast ? 1. Thus we conclude that the collapsing shell is unstable, and the growth rate depends on the thickness of the shell through a² and on the rate of collapse through the dimensionless time t.
dc.language.isoen_US
dc.relation.ispartofseriesT00662
dc.rightsI grant Indian Institute of Science the right to archive and to make available my thesis or dissertation in whole or in part in all forms of media, now hereafter known. I retain all proprietary rights, such as patent rights. I also retain the right to use in future works (such as articles or books) all or part of this thesis or dissertation
dc.subjectMagnetic field perturbations
dc.subjectElectric field disturbances
dc.subjectUnbounded oscillations
dc.titleSome stability and flow problems in hydrodynamics
dc.degree.namePhD
dc.degree.levelDoctoral
dc.degree.grantorIndian Institute of Science
dc.degree.disciplineScience


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