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Excitation of vertical coronal loop oscillations by plasma condensations

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Figure

Fig. 1. LeftRight: initial density configuration of the coronal loop with cool condensation region for µ = 0.7
Fig. 2. Top: ripples due to Rayleigh-Taylor instability formed at the in-terface between the condensation region and ambient coronal plasmanear at the top of the loop at t = 5544 s
Table 1. Blob oscillation parameters.
Fig. 6. Internal density profiles used for the calculation of the oscillationperiod in thin flux tube approximation for the µ = 0.7 case

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