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3.2.6 Effects of energetic particles propagating downward in the chromosphere

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Created by Yannis Zouganelis, last modified on Jun 19, 2017

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3.2.6 Effects of energetic particles propagating downward in the chromosphere

Generation of heating, shocks, sunquakes in the underlying photosphere (Martinez-Oliveros et al., 2007).

EUI, High-resolution, probably high-cadence.
SPICE, SPICE Waves mode
PHI, STIX