Hot prominence spicules launched from turbulent cool solar prominences

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Fig. 4.

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Long-term evolution of the prominence spicules exhibiting quasi-periodic propagating intensity disturbances. Similar to Fig. 3, but plotted for the observations obtained on 2015 February 15 along slit a–b in Fig. 1c. See Sect. 2.2 and Appendix B.2 for details.

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