Plasma densities, flow, and solar EUV flux at comet 67P - A cross-calibration approach

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Fig. 6.

Mission-wide 2D histogram of MIP density versus simultaneous LAP spacecraft potential proxy U₁ in 100 × 200 bins coloured by log₁₀ counts. The upper sensitivity limit of MIP in LDL mode is just below 300 cm⁻³ and is visible as a partial cut-off.

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