Git commit 94c81b8120f4912f087936b0f488183b072edafa by Yuri Chornoivan. Committed on 30/06/2023 at 19:14. Pushed by yurchor into branch 'master'.
Fix minor typos M +2 -2 doc/ekos-focus.docbook https://invent.kde.org/education/kstars/-/commit/94c81b8120f4912f087936b0f488183b072edafa diff --git a/doc/ekos-focus.docbook b/doc/ekos-focus.docbook index 84b82195e3..f2b7bb7106 100644 --- a/doc/ekos-focus.docbook +++ b/doc/ekos-focus.docbook @@ -1029,7 +1029,7 @@ applicable here as well.</para> <para> The difference between CFZ Shuffle and Fixed Steps is that near the center of the sweep (which - should be around the Critical Focus Zone (CFZ) the algorithm takes steps of half the specified size.</para> + should be around the Critical Focus Zone (CFZ)) the algorithm takes steps of half the specified size.</para> </listitem> </itemizedlist> </para> @@ -1255,7 +1255,7 @@ have how many ticks moved the drawtube the distance you measured. From this you can calculate the distance in microns a single tick moves the drawtube.</para> <para> Other types of telescope will have other ways to adjust the focal plane, for example, by moving the primary or - secondary mirrors. You will need to either get the Step Size from the documentation for your equipment of work out how to + secondary mirrors. You will need to either get the Step Size from the documentation for your equipment or work out how to measure it in a way that are consistent with that described above.</para> </listitem>
