Plasma characterization at comet 67P between 2 and 4 AU from the Sun with the RPC-MIP instrument

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Fig. 14

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Evolution of the warm (λ_Dh) and cold (λ_Dc) Debye length at the Rosetta spacecraft orbiter locations from January to September 2016. The dispersion of the results was computed and normalized over time intervals of 6 h. The color bar represents the occurrence.

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