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Published in 2022 at "Solar Physics"
DOI: 10.1007/s11207-021-01940-z
Abstract: We analyse the phase shifts of standing, slow magnetohydrodynamic (MHD) waves in solar coronal loops using a linear MHD model taking into account the role of thermal conductivity, compressive viscosity, radiative losses, and heating–cooling misbalance.…
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Keywords:
density;
phase;
cooling misbalance;
heating cooling ... See more keywords