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The top documents tagged [prominence plasma]
Formation of Helium Lines in Prominences
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Acoustic waves (case k = 0 ) -- Important for non-magnetized regions in the low solar atmosphere: Eqs. (10),(6) = (12) Fig. 3: Defined by Eq(12) variation
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Observations Morphology Quantitative properties Underlying Physics Aly-Sturrock limit
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Fig.4: Typical values of the collisional and viscous damping time ratios for propagating a) Alfvén and fast magnetoacoustic waves and b) acoustic wave
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