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Table 2
Summary of cases studied in Sect. 3.3 and their respective purposes.
| Case | rh 1 | Section | Purpose |
|---|---|---|---|
| May 2016 | 3.1 | 3.3.1 | Symmetric to pre-perihelion October 2014 study performed by Galand et al. (2016) in terms of heliocentric distance. |
| March 2016 | 2.6 | 3.3.2 | Symmetric to pre-perihelion October 2014 study performed by Galand et al. (2016) in terms of local photo-ionization frequency. |
| July 2016 | 3.4 | 3.3.3 | Effect of a CIR on the electron-impact ionization frequency and the induced ionospheric population. |
| August 2016 | 3.5 | 3.3.3 | “Return” of the July 2016 CIR, after one solar rotation, and illustration of a case of high plasma densities purely dependent on the electron-impact ionization. |
| April 2016 | 2.8 | 3.3.4 | Illustration of the robustness of the model to high variations in cometocentric distance undergone during the return from the cometary tail excursion. |
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