Hot prominence spicules launched from turbulent cool solar prominences

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Fig. 2.

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Thermal structuring of prominence spicules. Top left panel: same as the top panel of Fig. 1d. The other panels display the maps of RMS intensity fluctuations obtained from the AIA 193 Å, AIA 131 Å, and AIA 304 Å filter images during 2015 February 15 UT 20:00-20:29. See Sect. 2.1.

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