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Observation of 2nd Schumann eigenmode on Titan’s surface

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Figure

Table 1. Comparison of peculiarities of the Schumann resonances on Earth and Titan (after Béghin et al., 2012).
Fig. 2. Amplitude distribution (left) and waveform (right) of the first hundred VADC samples of bin 48 of the Cruise checkout # 10
Fig. 4. Amplitude distribution of bin 36 for two sequences for SNR, respectively > 1 (left panel), and < 1 (right panel).
Fig. 5. Frequency variation of the normalized skewed standard deviation σ ′f for the same sequences as in Figs
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