Git commit 1df2733c196205d3b3c44f1c13b42cdcbf0be30d by Yuri Chornoivan.
Committed on 23/03/2018 at 17:01.
Pushed by yurchor into branch 'master'.

Fix minor typos

M  +10   -10   docbook/kst/data-chapter.docbook
M  +3    -3    docbook/kst/debuglog-chapter.docbook
M  +1    -1    docbook/kst/plugins-chapter.docbook
M  +3    -3    docbook/kst/saving-chapter.docbook
M  +2    -2    docbook/kst/tutorial.docbook

https://commits.kde.org/kst-plot/1df2733c196205d3b3c44f1c13b42cdcbf0be30d

diff --git a/docbook/kst/data-chapter.docbook b/docbook/kst/data-chapter.docbook
index 7b478002..d7b9d635 100644
--- a/docbook/kst/data-chapter.docbook
+++ b/docbook/kst/data-chapter.docbook
@@ -57,7 +57,7 @@ However, for other data sources (eg, dirfiles), there may be 
multiple samples pe
   In the figure, imagine that time proceeds from top to bottom.  &kst; assumes 
that the first sample in a frame is simultaneous for every field in the data 
source, and that the rest of the samples are sampled evenly throughout the 
frame, as shown.  
 </para>
 <para>  
-  When plotting one vector agains another, &kst; assumes that the first and 
last samples of each vector are simultaneous, and interpolates the shorter 
vector up to the resolution of the longer vector.  Since only the first sample 
in a frame can be assumed to be simultaneous across fields, <emphasis>when 
&kst; reads data into a vector, it only reads up to the first sample of the 
last frame requested,</emphasis> so that plotting one vector against another 
will make sense.  The rest of the last frame will not be read.  
+  When plotting one vector against another, &kst; assumes that the first and 
last samples of each vector are simultaneous, and interpolates the shorter 
vector up to the resolution of the longer vector.  Since only the first sample 
in a frame can be assumed to be simultaneous across fields, <emphasis>when 
&kst; reads data into a vector, it only reads up to the first sample of the 
last frame requested,</emphasis> so that plotting one vector against another 
will make sense.  The rest of the last frame will not be read.  
 </para>
 <para>
   So if the first three frames of Field1 and Field2 are read from the data 
source in the figure, 3 samples will be read from Field1, and 9 samples will be 
read from Field2 (ending at first sample of Frame 3) - not 12 as one might 
expect.
@@ -157,7 +157,7 @@ icon in the tool bar.
 </para>
 
 <para>
-  Items can also be deleted from this dialog by selecting them and clicking 
<guibutton>Delete</guibutton>.  This will delete the selected item and all 
items which depend on it.  So if you delete a vector, all curves, spectra, 
historgrams, or equations that depend on it will also be deleted.  Be careful, 
because this can not be undone.
+  Items can also be deleted from this dialog by selecting them and clicking 
<guibutton>Delete</guibutton>.  This will delete the selected item and all 
items which depend on it.  So if you delete a vector, all curves, spectra, 
histograms, or equations that depend on it will also be deleted.  Be careful, 
because this can not be undone.
 </para>
 <para>
   Clicking <guibutton>Purge</guibutton> will remove all undisplayed data 
objects.  If deleting an object (and everthing that depends on it) will not 
change any plots or labels, then it is deleted.  Nothing that is displayed is 
deleted.  This can not be undone.
@@ -217,7 +217,7 @@ icon in the tool bar.
 </para>
 
 <para>
-  The plot displays two curves.  One curve takes two data vectors (INDEX and 
Column 2) as inputs.  The other takes INDEX as its X vector, and the ouput 
vector of the Low Pass Filter as its Y vector.  The low pass filter takes the 
Column 2 vector, and two Scalars as its inputs.  The two data vectors get their 
data from the Data Source.
+  The plot displays two curves.  One curve takes two data vectors (INDEX and 
Column 2) as inputs.  The other takes INDEX as its X vector, and the output 
vector of the Low Pass Filter as its Y vector.  The low pass filter takes the 
Column 2 vector, and two Scalars as its inputs.  The two data vectors get their 
data from the Data Source.
 </para>
 
 <para>
@@ -335,11 +335,11 @@ Curves are created by the data wizard, from the creation 
dialog from Data Object
 </para>
 
 <para>
-  The appearance of curves is adjusted in the <guilabel>Appearance</guilabel> 
box.  Some of the flexability of curves in kst is shown in the next figure. 
+  The appearance of curves is adjusted in the <guilabel>Appearance</guilabel> 
box.  Some of the flexibility of curves in kst is shown in the next figure. 
   Note that the options are not exclusive - for example, 
<guilabel>Lines</guilabel> and <guilabel>Points</guilabel> can both be 
selected.  The <guilabel>Size</guilabel> field specifies the dimensions of 
display elements such as points and error flags in points (the same way as font 
sizes are defined.)
   The <guilabel>Weight</guilabel> field specifies the width of lines,
   bar graph borders, and the strokes for points.  The color selector to the 
right of the example line sets the color of lines, points, and bargraph 
borders.  The color selector to the right of the <guilabel>Bargraph</guilabel> 
checkbox sets the fill color for bargraphs.  The last (most recent) point of a
-  curve can be indicated by slecting <guilabel>Head</guilabel> and specifying
+  curve can be indicated by selecting <guilabel>Head</guilabel> and specifying
   a point type and color. The color selector to the right of the 
<guilabel>Head</guilabel> sets the color for this point.  
 </para>
 
@@ -497,7 +497,7 @@ Curves are created by the data wizard, from the creation 
dialog from Data Object
 </screenshot>
 
 <para>
-  The <guilabel>New Equation</guilabel> dialog which created this plot is 
shown below. Note that vectors are identified by enclosing their names in 
<literal>[  ]</literal>.   So Column 2 is indicated by <literal>[Column 2 
(V2)]</literal>.  The <guilabel>Equation</guilabel> line widget has a fairly 
powerful autocomplete mechanism with a scrollable list of all possible scalars 
(in its first colum) or vectors (in its second column) as you enter the name of 
the object.  Similarly, the auto complete lists all valid functions and 
operators as relevant while you type.  The <literal>Esc</literal> key hides the 
autocomplete widget.
+  The <guilabel>New Equation</guilabel> dialog which created this plot is 
shown below. Note that vectors are identified by enclosing their names in 
<literal>[  ]</literal>.   So Column 2 is indicated by <literal>[Column 2 
(V2)]</literal>.  The <guilabel>Equation</guilabel> line widget has a fairly 
powerful autocomplete mechanism with a scrollable list of all possible scalars 
(in its first column) or vectors (in its second column) as you enter the name 
of the object.  Similarly, the auto complete lists all valid functions and 
operators as relevant while you type.  The <literal>Esc</literal> key hides the 
autocomplete widget.
 </para>
 
 <para>
@@ -616,7 +616,7 @@ In the <guilabel>New Histogram</guilabel> dialog, the bins 
can be set manually,
 
 
 <para>
-  The following plot shows an example spectrum.  The plot has been converted 
to log-log mode (hit 'l' and 'g' in the plot window to toggle Y and X log axes 
respectvely).
+  The following plot shows an example spectrum.  The plot has been converted 
to log-log mode (hit 'l' and 'g' in the plot window to toggle Y and X log axes 
respectively).
 </para>
 
 <screenshot>
@@ -682,7 +682,7 @@ Remove a constant from the input vector to make it mean 
zero before calculating
 <listitem>
 <para>
 Apodize the data with the selected function before calculating the power 
spectrum to reduce
-bin to bin leackage.  The default is a Hanning Window.
+bin to bin leakage.  The default is a Hanning Window.
 </para>
 </listitem>
 </varlistentry>
@@ -858,7 +858,7 @@ Auto-generating axes labels for plots will be based on 
these units.
 </para>
 
 <para>
-  For fields such as angles which have (for example) a discontinuity at 360 
degrees, the Unwind Fliter can be used to make the signal continuous.  So if 
the unfiltered signal goes from 359.5 degrees to 0.5 degrees in consecutive 
samples, the filtered signal will go from 359.5 degrees to 360.5 degrees.
+  For fields such as angles which have (for example) a discontinuity at 360 
degrees, the Unwind Filter can be used to make the signal continuous.  So if 
the unfiltered signal goes from 359.5 degrees to 0.5 degrees in consecutive 
samples, the filtered signal will go from 359.5 degrees to 360.5 degrees.
 </para>
 
 <para>
@@ -951,7 +951,7 @@ Matrices are two dimensional tables of numbers.  They can 
be used as the inputs
   </listitem>
   <listitem>
     <para>
-      BIT Image Streams (BIS) fiiles.
+      BIT Image Streams (BIS) files.
     </para>
   </listitem>
 </itemizedlist>
diff --git a/docbook/kst/debuglog-chapter.docbook 
b/docbook/kst/debuglog-chapter.docbook
index 55145f1c..dddcf4eb 100644
--- a/docbook/kst/debuglog-chapter.docbook
+++ b/docbook/kst/debuglog-chapter.docbook
@@ -1,18 +1,18 @@
 <appendix id="debuglog">
 <title>Troubleshooting</title>
 <para>
-Unfortunately, things can sometimes go wrong with &kst;.  This section lists 
somee things that can be useful to unbreak things.
+Unfortunately, things can sometimes go wrong with &kst;.  This section lists 
some things that can be useful to unbreak things.
 </para>
 
 <sect3>
   <title>Clearing Defaults</title>
 
   <para>
-    For convenience reasons, &kst; makes agressive use of sticky defaults - 
that is to say, &kst; will generally remember what you did last time, and make 
that the new default behaviour.  Unfortunately, this can sometimes leave the 
program in an odd state where the assumptions it is making make no sense.  This 
most often happens with files and file defaults.
+    For convenience reasons, &kst; makes aggressive use of sticky defaults - 
that is to say, &kst; will generally remember what you did last time, and make 
that the new default behaviour.  Unfortunately, this can sometimes leave the 
program in an odd state where the assumptions it is making make no sense.  This 
most often happens with files and file defaults.
   </para>
 
   <para>
-    If you find that &kst; has broken for you (that is, something that used to 
work no longer does), bad defaults is a pretty plausable explaination (though 
we do keep trying to track these situations down and remove them).  You can 
completely restore &kst; to it's default, just-installed configuration by 
selecting <guimenuitem>Clear datasource settings</guimenuitem> and 
<guimenuitem>Clear settings and defaults</guimenuitem> from the 
<guimenu>Settings</guimenu> menu.  Unfortunately, this will erase all of your 
settings and defaults, but it may be necessary in some cases.  If the problem 
seems to have something to do with data files, try <guimenuitem>Clear 
datasource settings</guimenuitem> first because it is generally less 
destructive and more likely to help.
+    If you find that &kst; has broken for you (that is, something that used to 
work no longer does), bad defaults is a pretty plausible explanation (though we 
do keep trying to track these situations down and remove them).  You can 
completely restore &kst; to it's default, just-installed configuration by 
selecting <guimenuitem>Clear datasource settings</guimenuitem> and 
<guimenuitem>Clear settings and defaults</guimenuitem> from the 
<guimenu>Settings</guimenu> menu.  Unfortunately, this will erase all of your 
settings and defaults, but it may be necessary in some cases.  If the problem 
seems to have something to do with data files, try <guimenuitem>Clear 
datasource settings</guimenuitem> first because it is generally less 
destructive and more likely to help.
   </para>
 </sect3>
 
diff --git a/docbook/kst/plugins-chapter.docbook 
b/docbook/kst/plugins-chapter.docbook
index 59802daf..4a680404 100644
--- a/docbook/kst/plugins-chapter.docbook
+++ b/docbook/kst/plugins-chapter.docbook
@@ -1,7 +1,7 @@
 <chapter id="pluginsandfilters">
 <title>Plugins, Fits, and Filters</title>
 <para>
-Many of the mathematical data operators in &kst;, including fits and filters, 
are implemented as plugins.  Plugins are loaded at run time and use a stable 
API, so it is possible to write your own plugins and include them in your local 
installation without re-compiling &kst;.  Fits and Filters are simply subsets 
of the set of plugins, and thus behave identically to generic plugins, with the 
exception of additional convenience dialog functionality when selected from the 
plot contect menu.  See <link linkend="fits">here</link> for a general 
description of the creation of fits and filters.
+Many of the mathematical data operators in &kst;, including fits and filters, 
are implemented as plugins.  Plugins are loaded at run time and use a stable 
API, so it is possible to write your own plugins and include them in your local 
installation without re-compiling &kst;.  Fits and Filters are simply subsets 
of the set of plugins, and thus behave identically to generic plugins, with the 
exception of additional convenience dialog functionality when selected from the 
plot context menu.  See <link linkend="fits">here</link> for a general 
description of the creation of fits and filters.
 </para>
 
 <para>
diff --git a/docbook/kst/saving-chapter.docbook 
b/docbook/kst/saving-chapter.docbook
index 610aefed..821dd4d4 100644
--- a/docbook/kst/saving-chapter.docbook
+++ b/docbook/kst/saving-chapter.docbook
@@ -47,7 +47,7 @@
 <title>Saving</title>
 
 <para>
-  Selecting <guimenuitem>Save</guimenuitem> or <guimenuitem>Save 
As</guimenuitem> from the <guimenu>File</guimenu> menu will save the state of 
the current kst session.  By default, these session files have the extentions 
<literal>.kst</literal>.  If this session file is opened later, the state of 
kst, including the loading of all data files, and the saving of all plots will 
be returned to the state when it was saved.
+  Selecting <guimenuitem>Save</guimenuitem> or <guimenuitem>Save 
As</guimenuitem> from the <guimenu>File</guimenu> menu will save the state of 
the current kst session.  By default, these session files have the extensions 
<literal>.kst</literal>.  If this session file is opened later, the state of 
kst, including the loading of all data files, and the saving of all plots will 
be returned to the state when it was saved.
 </para>
 
 </sect2>
@@ -164,7 +164,7 @@ To print, select <guimenuitem>Print...</guimenuitem> from 
the <guimenu>File</gui
 If the OS supports it, the plots can be exported here to a pdf file.  
Otherwise, you can use the <link linkend="exportinggraphics">Exporting 
Tabs</link> option described in the next section to export to a pdf file.
 </para>
 <para>
-  Each page will be rescaled to fit whatever page size and orientation has 
been selected.  The scaling and resizing rules are the same when a &kst; window 
is resized.  If the page is the same size as has been set as the 
<guilabel>Reference view size</guilabel> (under <guilabel>Scaling</guilabel> in 
the <guilabel>Kst Settings</guilabel> dialog, selected by 
<guimenuitem>Configure Kst</guimenuitem> from the <guimenu>Settings</guimenu> 
menu), then the fonts will all have the sizes they have been set to in the 
various dialogs.  If the selected print size is larger or smaller than this, 
then the fonts will be also be proportionaly larger or smaller.
+  Each page will be rescaled to fit whatever page size and orientation has 
been selected.  The scaling and resizing rules are the same when a &kst; window 
is resized.  If the page is the same size as has been set as the 
<guilabel>Reference view size</guilabel> (under <guilabel>Scaling</guilabel> in 
the <guilabel>Kst Settings</guilabel> dialog, selected by 
<guimenuitem>Configure Kst</guimenuitem> from the <guimenu>Settings</guimenu> 
menu), then the fonts will all have the sizes they have been set to in the 
various dialogs.  If the selected print size is larger or smaller than this, 
then the fonts will be also be proportionally larger or smaller.
 </para>
 </sect1>
 
@@ -187,7 +187,7 @@ from the <guimenu>File</guimenu> menu.  The following 
dialog box will appear.
 </screenshot>
 
 <para>
-  The root file name is specified in the <guilabel>File name:</guilabel> 
entry.  If <guilabel>Automatic extension</guilabel> is selected, then the file 
name extension appropriate to the file type is automacially added to the file 
name.
+  The root file name is specified in the <guilabel>File name:</guilabel> 
entry.  If <guilabel>Automatic extension</guilabel> is selected, then the file 
name extension appropriate to the file type is automatically added to the file 
name.
 </para>
 
 <para>
diff --git a/docbook/kst/tutorial.docbook b/docbook/kst/tutorial.docbook
index 29430b16..a06ac2f9 100644
--- a/docbook/kst/tutorial.docbook
+++ b/docbook/kst/tutorial.docbook
@@ -577,7 +577,7 @@ using the context menu for this.  Selecting 
<guimenuitem>Maximize</guimenuitem>
 <para>
 Selecting <guimenuitem>Maximize</guimenuitem> (or typing <keycap>Z</keycap> in 
the plot) again will restore it the plots to their previous
 arrangement.  This is especially valuable if you have a grid of many small 
plots
-and want to temporarily look at just one of them.  Obviously typing 
<keycap>Z</keycap> is going to be the most convienient way
+and want to temporarily look at just one of them.  Obviously typing 
<keycap>Z</keycap> is going to be the most convenient way
 to do this, but the context menu is there in case you forget.
 </para>
 
@@ -642,7 +642,7 @@ equivalent to selecting <guimenu>X Mouse Zoom 
Mode</guimenu> from the
 fileref="Icon-kst-xmousezoom.png"
 format="PNG"/></imageobject></inlinemediaobject> toolbar button). If you
 then move the mouse, you will see that it is now dragging a vertical line
-the heght of the plots in both of the plots that are tied to gether.  
+the height of the plots in both of the plots that are tied together.
 While keeping
 &Ctrl; held down, drag a rectangle in the middle plot.
 While dragging, the region you are selecting will be displayed in both 

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