Coronal seismology is a specialized field of astrophysics that studies oscillations and waves in the solar corona, the outer layer of the Sun's atmosphere. This technique involves the analysis of various types of wave phenomena, such as acoustic waves, magnetohydrodynamic (MHD) waves, and other oscillations that propagate through the plasma of the corona. These waves can result from disturbances such as solar flares, coronal mass ejections (CMEs), and the solar wind.
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