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- W2012129812 abstract "The slow magnetosonic waves can, under certain conditions, have a discrete set of regular eigenmodes similar to the discrete Alfvén wave spectrum (Sturmian or anti-Sturmian). The latter were shown to explain the short period (2-8 min) prominence loop oscillations as a global Alfvén modes. Here, we slow that the anti-sturmian discrete slow wave spectrum can explain the long period (24-84 min) oscillations of solar loop prominences. We have also estimated the Q (Q−1 = Imω/ω) factor, due to electron and ion Cherenkov damping, for the loop cavity, and found the value of Q ~ 6 which is compatible with the observations of loop period oscillation and life time." @default.
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- W2012129812 date "1996-01-01" @default.
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- W2012129812 title "Anti-sturmian slow discrete modes modeling long period loop prominence oscillations" @default.
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- W2012129812 doi "https://doi.org/10.1088/0031-8949/1996/t63/042" @default.
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