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Title: MAGNETOHYDRODYNAMIC SIMULATIONS OF CORONAL RAIN IN SOLAR CORONAL LOOPS   Abstract: Coronal rain constitutes one of the most compelling phenomena in the solar atmosphere, wherein cold, dense plasma condensations form within the hot corona and subsequently precipitate toward the chromosphere along magnetic field lines. In this thesis, we present magnetohydrodynamic (MHD) numerical simulations of coronal rain formation and dynamics using

 

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