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I absolutely love the early phase of a start-up.
It is also observed that TEC starts responding to the eclipse after 30 min from start of eclipse and the delay of the maximum TEC deviation from normal trend with respect to the maximum phase of the eclipse was close to one hour in the solar eclipse path.
The partial phase of the eclipse then begins as a small indentation in the western rim of the Sun becomes noticeable.
During the recovery phase of the eclipse, OH-radical, sulphuric acid, (N- HOM aN- HOMster concentrandons reclusternd re-initialize NPF.
The meridional winds in the MLT region show remarkable changes after the maximum phase of the eclipse compared with that during the maximum phase of the eclipse, as shown in Fig. 1 d).
The meridional wind in the MLT region showed noticeable changes only after the maximum phase of the eclipse.
The zonal and meridional wind components in the MLT region clearly show short-period perturbations during, as well as after, the maximum phase of the eclipse, compared with the reference profile (mean of January 2010, except the eclipse day observations).
The height profiles of meridional winds (Fig. 3(b)) show similar variations as during the maximum phase of the eclipse (Fig. 1(b)) except for an increase in northerly winds around the 35 40-km 35 40-kmowaregione end of eclipse.
The MLT region zonal wind showed a reversal at 98 km during the maximum phase of the eclipse and the reversal is further strengthened after the maximum phase.
The penumbral phase of the eclipse changes the appearance of the Moon only slightly and is generally not noticeable.
First, you'll be following the partial phases of the eclipse as the Moon inches over the Sun's disc.
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Since I tried Ludwig back in 2017, I have been constantly using it in both editing and translation. Ever since, I suggest it to my translators at ProSciEditing.

Justyna Jupowicz-Kozak
CEO of Professional Science Editing for Scientists @ prosciediting.com