Properties of the singing comet waves in the 67P/Churyumov-Gerasimenko plasma environment as observed by the Rosetta mission

Rosetta mission full comet phase results

Open Access

Fig. 3

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Powerspectral densities of the B_x magnetic field component, estimated using Welch’s method, for time windows of 20 min before (in orange), during (in blue), and after (in green) the outburst event observed at comet 67P at 10:00 UT on 2016 February 19.

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