Exploring the time variability of the solar wind using LOFAR pulsar data

Open Access

Fig. 2.

Simulation scenario 1, only SW. Top: n_e variations simulated (blue) are shown as well as the mean value (red) and the n_e retrieved (green) when fit for a single value with TEMPO2. Middle: Blue points represent the residuals corresponding to the injected values of n_e. Bottom: Green points represent the residuals after a constant ${\bar{n}}_{e}$ $\bar{n}_{\mathrm{e}}$ fit in TEMPO2.

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