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Numerical Simulations on Flux Tube Tectonic Model for Solar Coronal Heating

-The sun is a G-type main sequence star. Corona is an aura of Plasma that Surrounds the Sun and other Stars. The heating of solar Corona is one of most important problem in Astrophysics. There are several mechanism of Coronal heating. In this paper we discuss Numerical Simulation on Flux tube Tectonic Model For Solar Coronal Heating .