Turbulence in a Coronal Loop Excited by Photospheric Motions
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DOI: 10.3390/atmos11040409
Abstract: Photospheric motions are believed to be the source of coronal heating and of velocity fluctuations detected in the solar corona. A numerical model, based on the shell technique applied on reduced magnetohydrodynamics equations, is used… read more here.
Keywords: photospheric motions; coronal loop; energy; frequency ... See more keywords