Physics
Scientific paper
Jul 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995soph..159..399n&link_type=abstract
Solar Physics, Volume 159, Issue 2, pp.399-402
Physics
41
Scientific paper
The linear properties of the fast magnetosonic modes of a coronal loop modelled as a smooth density inhomogeneity in a uniform magnetic field are compared with the case of a step function slab. It is shown that the group velocityC gof the modes, important in determining the structure of impulsively excited wave packets, possesses a minimum for a wide class of profile including the slab, with the exception of the Epstein profile for which the minimum inC gmoves out to infinity. Results for the simple step profile are thus of wider validity, and likely to be applicable to coronal loops.
Nakariakov Valery M.
Roberts Barney B.
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