A physical interpretation of relevance to a mathematical argument is the determination of the reality of the universe by applying a radio frequency accelerator with the Sun. The exploitation of the universe deals with the controlled thermonuclear fusion reaction of the Sun at the re sonant level to produce X-ray ernission subject to an irregular fluctuation of a magnetic field in vacuum.
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The authors in compliance with investigations (Ghosh, 1997; 2001; Ghosh and Pop, 2002) prove that resonance exhibits a thermonuclear fusion reaction over the Sun in the presence of an applied inclined magnetic field when a forced oscillation is taken into account. The interstellar space is a great deal of controversy when a forced oscillation is applied to the Sun.
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We have examined the MHD plasma behavior of a rotating environment in the presence of an inclined magnetic field with the positive direction of the axis of rotation. The interplay of a hydromagnetic force and Coriolis force exerts its influence of a dynamo mechanism with reference to the solar and terrestrial context when the Hall current is taken into account. It is stated that the electrical discharge of the solar corona in the presence of a traveling magnetic field experiences an irregular fluctuation at the resonant level to produce thermonuclear fusion reaction of the Sun with regard to excitation frequency. On the other hand, the thermonuclear fusion reaction of the Sun stops when the excitation frequency is switched off and the MHD plasma flow tends to an equilibrium position with regard to a neutral plasma stability parameter.
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The parametric instability behavior of a stiffened plate subjected to uniform in-plane edge loading is studied using the finite element analysis. The method of Hill's infinite determinants is applied to analyze the dynamic instability regions. Numerical results are presented to demonstrate the effects of various parameters, such as the aspect ratio, boundary condition, stiffening scheme, on the dynamic stability of stiffened plates. The results show that the location, size and number of stiffeners have a significant effect on the location of the boundaries of the principal instability regions when compared with those of a flat unstiffened plate.
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