Git commit 94a629497ff3676eabb896008e5f7cdca3497741 by Hy Murveit.
Committed on 15/01/2023 at 23:53.
Pushed by murveit into branch 'master'.

Update handbook for polar alignment

M  +52   -130  doc/ekos-align.docbook
M  +1    -1    doc/ekos.docbook
A  +-    --    doc/polar_assistant_main2.png
A  +-    --    doc/polar_assistant_ps1.png
A  +-    --    doc/polar_assistant_ps2.png
A  +-    --    doc/polar_assistant_ps3.png

https://invent.kde.org/education/kstars/commit/94a629497ff3676eabb896008e5f7cdca3497741

diff --git a/doc/ekos-align.docbook b/doc/ekos-align.docbook
index d42375f5e..94a506d0d 100644
--- a/doc/ekos-align.docbook
+++ b/doc/ekos-align.docbook
@@ -27,20 +27,8 @@
             Often, there is a discrepancy between where the telescope thinks 
it is looking at and where it is truly pointing. The magnitude of this 
discrepancy can range from a few arcminutes to a couple of degrees. Ekos can 
then correct the discrepancy by either syncing to the new coordinates, or by 
slewing the mount to the desired target originally requested.
         </para>
         <para>
-            Furthermore, Ekos provides two tools to measure and correct polar 
alignment errors:
+            Furthermore, Ekos provides a Polar Alignment Assistant Tool to 
correct polar alignment errors. It takes three images, slewing between the 
images, and calculates the offset between the mount axis and polar axis. It 
feeds back to the user the altitude and azimuth adjustments needed to align 
these axes. These images are typically taken near the celestial pole (Close to 
Polaris for Northern Hemisphere) but can work well taken from anywhere, usually 
starting near the meridian and slewing either East or West.
         </para>
-        <itemizedlist>
-            <listitem>
-                <para>
-                    <guilabel>Polar Alignment Assistant Tool</guilabel>: A 
very easy tool to measure and correct polar errors. It takes three images near 
the celestial pole (Close to Polaris for Northern Hemisphere) and then 
calculates the offset between the mount axis and polar axis.
-                </para>
-            </listitem>
-            <listitem>
-                <para>
-                    <guilabel>Legacy Polar Alignment Tool</guilabel>: If 
Polaris is not visible, this tool can be used to measure and correct polar 
alignment errors. It captures a couple of images near the meridian and 
east/west of the meridian. This will enable the user to adjust the mount until 
the misalignment is minimized.
-                </para>
-            </listitem>
-        </itemizedlist>
         <para>
             At a minimum, you need a CCD/Webcam and a telescope that supports 
Slew &amp; Sync commands. Most popular commercial telescope nowadays support 
such commands.
         </para>
@@ -336,11 +324,6 @@
                         <guilabel>Polar Alignment Assistant</guilabel>: A 
simple tool to aid in polar alignment of German Equatorial Mounts.
                     </para>
                 </listitem>
-                <listitem>
-                    <para>
-                        <guilabel>Legacy Polar Alignment Tool</guilabel>: 
Measure polar alignment error when a view of the celestial pole (&eg; Polaris 
for Northern Hemisphere) is not available.
-                    </para>
-                </listitem>
             </itemizedlist>
             <warning>
                 <para>
@@ -533,8 +516,6 @@
 
         <sect3 id="ekos-align-polaralignment">
             <title>Polar Alignment</title>
-            <sect4 id="ekos-align-plar-alignment-assistant">
-                <title>Polar Alignment Assistant</title>
                 <para>
                     When setting up a German Equatorial Mount (GEM) for 
imaging, a critical aspect of capturing long-exposure images is to ensure 
proper polar alignment. A GEM mount has two axis: Right Ascension (RA) axis and 
Declination (DE) axis. Ideally, the RA axis should be aligned with the 
celestial sphere polar axis. A mount's job is to track the star's motion around 
the sky, from the moment they rise at the eastern horizon, all the way up 
across the median, and westward until they set.
                 </para>
@@ -573,10 +554,10 @@
                     However, unless you have a top of the line mount, then 
you'd probably want to use an autoguider to keep the same star locked in the 
same position over time. Despite all of this, if the axis of the mount is not 
properly aligned with the celestial pole, then even a mechanically-perfect 
mount would lose tracking with time. Tracking errors are proportional to the 
magnitude of the misalignment. It is therefore very important for long exposure 
imaging to get the mount polar aligned to reduce any residual errors as it 
spans across the sky.
                 </para>
                 <para>
-                    Before starting the process, point the mount as close as 
possible to the celestial pole. If you are living in the Northern Hemisphere, 
point it as close as possible to Polaris.
+                    Before starting the process, point the mount as close as 
possible to the celestial pole with the counterweights down. If you are living 
in the Northern Hemisphere, point it as close as possible to Polaris. If 
Polaris is not visible (e.g. blocked by trees or  buildings) you may point 
elsewhere, preferably near the Meridian. Make sure there is at 30-60 degrees of 
sky viewable in an arc East or West of the Meridian from the position you 
choose. Select the direction of free sky, the number of degrees for each of two 
slews, the mount slew speed, and whether the mount will be slewing 
automatically (recommended) or manually.
                 </para>
                 <para>
-                    The tool works by capturing and solving three images. 
After capturing each, the mount rotates by a fixed amount and another image is 
captured and solved.
+                    The tool works by capturing and solving three images. 
After capturing each, the mount rotates by the fixed amount you entered and 
another image is captured and solved. If you chose manual, you will need to 
slew the mount by roughly the angle chosen.
                 </para>
                 <screenshot>
                     <screeninfo>
@@ -584,141 +565,82 @@
                     </screeninfo>
                     <mediaobject>
                         <imageobject>
-                            <imagedata fileref="polar_assistant_main.png" 
format="PNG"/>
+                            <imagedata fileref="polar_assistant_main2.png" 
format="PNG"/>
                         </imageobject>
                         <textobject>
                             <phrase>Polar Alignment Assistant</phrase>
                         </textobject>
                     </mediaobject>
                 </screenshot>
+
+            <sect4 id="ekos-align-platesolvecorrection">
+                <title>Plate Solve Correction Scheme</title>
+                
                 <para>
-                    After the first capture, you can rotate the mount by a 
specific amount (default 30 degrees) either West or East. After selecting the 
magnitude and direction, click <guibutton>Next</guibutton> to continue and the 
mount will be rotated. Once the rotation is complete you shall be asked to take 
another capture, unless you have checked <guilabel>Auto Mode</guilabel>. In 
Automated mode, the rest of the process will continue with the same settings 
and direction until a total of three images are captured.
-                </para>
-                <para>
-                    Since the mount's true RA/DE are resolved by astrometry, 
we can construct a unique circle from the three centers found in the astrometry 
solutions. The circle's center is where the mount rotates about (RA Axis) and 
ideally, this point should coincide with the celestial pole. However, if there 
is a misalignment, then Ekos draws a correction vector. This correction vector 
can be placed anywhere in the image. Next, <emphasis>refresh</emphasis> the 
camera feed and make corrections to the mount's Altitude and Azimuth knobs 
until the star is located in the designated cross-hair. To make it easy to make 
corrections, expand the view by clicking on the Fullscreen button 
<inlinemediaobject><imageobject><imagedata fileref="view-fullscreen.png" 
format="PNG"/></imageobject></inlinemediaobject>.
+                  The images below show the workflow when the <emphasis>Plate 
Solve</emphasis> correction technique is used. The image below shows a display 
after the 3 measurement images are captured and solved. It shows an error of 
almost 18' in altitude and that the mount's axis needs to be moved up. 
Similarly it shows an azimuth error of almost 15' and that the axis needs to be 
moved to the right (as viewed from behind the telescope). 
                 </para>
                 <screenshot>
                     <screeninfo>
-                        Polar Alignment Result
+                        Polar Alignment Assistant
                     </screeninfo>
                     <mediaobject>
                         <imageobject>
-                            <imagedata fileref="polar_alignment_result.png" 
format="PNG"/>
+                            <imagedata fileref="polar_assistant_ps1.png" 
format="PNG"/>
                         </imageobject>
                         <textobject>
-                            <phrase>Polar Alignment Result</phrase>
+                            <phrase>Polar Alignment Assistant, Plate Solve 
Workflow 1</phrase>
                         </textobject>
                     </mediaobject>
                 </screenshot>
                 <para>
-                    If you are away from StellarMate or PC, you can use your 
Tablet to monitor the camera feed while making corrections. Use the <link 
linkend="ekos-tutorials-viewer">StellarMate's web-based VNC viewer</link> or 
use any VNC Client on your tablet to access StellarMate. If Ekos is running on 
your PC, you can use applications like TeamViewer to achieve the same results. 
The following is a video demonstrating how to utilize the Polar Alignment 
Assistant tool.
+                  If your error is low enough (e.g. less than an arc-minute) 
then you don't need to make any adjustments. Simply press stop and you're done.
                 </para>
-                <mediaobject>
-                    <videoobject>
-                        <videodata contentdepth="315" contentwidth="560" 
fileref="https://www.youtube.com/embed/sx6Zz9lNd5Q"/>
-                    </videoobject>
-                    <caption>
-                        <para>
-                            <phrase>Polar Alignment</phrase>
-                        </para>
-                    </caption>
-                </mediaobject>
-            </sect4>
-            <sect4 id="ekos-align-legacy-polar-alignment-workflow">
-                <title>Legacy Polar Alignment Workflow</title>
                 <para>
-                    Using the Polar Alignment mode, Ekos can measure and 
correct the polar alignment errors. To measure Azimuth error, point your mount 
to a star close to the meridian. If you live in the northern hemisphere, you 
will point the mount toward the southern meridian. Click on <guibutton>Measure 
Az Error</guibutton> to begin the process. Ekos will try to measure the drift 
between two images and calculates the error accordingly. You can ask Ekos to 
correct Azimuth error by clicking on the <guibutton>Correct Az 
Error</guibutton> button. Ekos will slew to a new location and asks you to 
adjust the mount's azimuth knobs until the star is in the center of the Field 
of View. You can use the Focus Module's <link 
linkend="focus-focuser-group">Framing feature</link> to take a look at the 
image as you make your adjustments.
+                  If you will be making corrections to your mount's axis, you 
should select the adjustment approach (we're using Plate Solve in this 
example), and how often the system should recapture images to re-measure the 
polar alignment error. The refresh interval should be frequent, but it doesn't 
make sense to make it faster that your CPU can capture and plate-solve the 
images. We're using 2s in this example. Then press the Refresh button to begin 
the correction process.
                 </para>
                 <para>
-                    Similarly, to measure Altitude error, click on the 
<guibutton>Measure Alt Error</guibutton> button. You need to point your mount 
either east or west and set the <guilabel>Altitude Direction</guilabel> combo 
box accordingly. Ekos will take two images and calculates the error. You can 
ask Ekos to correct Altitude error by clicking on the <guibutton>Correct Alt 
Error</guibutton> button. As with Azimuth correction, Ekos will slew to a new 
location and asks you to adjust the mount's altitude knobs until the star is in 
the center of the FOV.
+                  The system will capture images, and re-estimate the polar 
alignment error after each image. You can try to reduce the error by adjusting 
the Alititude and Azimuth correction knobs on your mount. The image below shows 
the screen after the altitude error has been almost zeroed. See the difference 
between the  <emphasis>Measured Error</emphasis> row, which shows the 
originally measured error after the original 3 captures, and the  
<emphasis>Updated Error</emphasis> row which shows the current error estimate.
                 </para>
+                <screenshot>
+                    <screeninfo>
+                        Polar Alignment Assistant
+                    </screeninfo>
+                    <mediaobject>
+                        <imageobject>
+                            <imagedata fileref="polar_assistant_ps2.png" 
format="PNG"/>
+                        </imageobject>
+                        <textobject>
+                            <phrase>Polar Alignment Assistant, Plate Solve 
Workflow 2</phrase>
+                        </textobject>
+                    </mediaobject>
+                </screenshot>
                 <para>
-                    After making a correction, it is recommended to measure 
the Azimuth and Altitude errors again and gauge the difference. You may need to 
perform the correction more than once to obtain optimal results.
+                  Below the user has also adjust Azimuth to reduce the error 
further. Now the error is very low and the process is done. The user should 
press the stop button.
                 </para>
+                <screenshot>
+                    <screeninfo>
+                        Polar Alignment Assistant
+                    </screeninfo>
+                    <mediaobject>
+                        <imageobject>
+                            <imagedata fileref="polar_assistant_ps3.png" 
format="PNG"/>
+                        </imageobject>
+                        <textobject>
+                            <phrase>Polar Alignment Assistant, Plate Solve 
Workflow 3</phrase>
+                        </textobject>
+                    </mediaobject>
+                </screenshot>
+                </sect4>
+                <sect4 id="ekos-align-move-star-correction">
+                <title>Move Star Correction Scheme</title>
+
                 <para>
-                    Before starting the Polar Alignment tool, you must 
complete the GOTO Workflow above for at least one point in the sky. Once your 
mount is aligned, proceed with the following (assuming you live in the northern 
hemisphere):
+                  We also have an alternative schemes for correcting polar 
alignment. Two variations are <emphasis>Move Star &amp; Calc Error</emphasis> 
and <emphasis>Move Star</emphasis>. When you select this scheme, the system 
place a yellow/green/violet triangle on the screen. The trangle can be moved by 
clicking near a star, and the yellow/violet corner is moved to that star. In 
this scheme the user corrects polar alignment by first adjusting the mount's 
azimuth knob so that the selected star moves along the yellow side of the 
triangle. Once the star is near the next vertex, the azimuth knob should be 
adjusted so that the star moves along the green side of the triangle. Once the 
star is moved to the green/violet vertex, the mount is polar aligned, and the 
user can click <emphasis>stop</emphasis>.
+                </para>
+                  <para>
+                    The difference between <emphasis>Move Star &amp; Calc 
Error</emphasis> and  <emphasis>Move Star</emphasis> is that in the former, the 
system attempts to track the star the user has selected, and places a circle 
around that star. In that scheme it also attempts to update the 
<emphasis>Updated Err</emphasis> row. If the star tracking isn't reliable, 
simply ignore it or use the <emphasis> Move Star </emphasis>scheme and move the 
star by-eye until it's close to the final target. An example of using this 
technique is shown in this video: 
+                    <ulink 
url="https://www.youtube.com/watch?v=iOp7hrxw0oU";>https://www.youtube.com/watch?v=iOp7hrxw0oU</ulink>
                 </para>
-                <orderedlist>
-                    <listitem>
-                        <para>
-                            Slew to a <emphasis role="bold">bright</emphasis> 
star (4th magnitude or below) near the southern meridian (Azimuth 180). Make 
sure <guilabel>Slew to Target</guilabel> is selected. Capture and solve. The 
star should be exactly centered in your CCD field of view.
-                        </para>
-                    </listitem>
-                    <listitem>
-                        <para>
-                            Switch mode to <guilabel>Polar 
Alignment</guilabel>. Click <guibutton>Measure Az Error</guibutton>. It will 
ask you to slew to a star at the southern meridian which we already done. Click 
<guibutton>Continue</guibutton>. Ekos will now perform the error calculation.
-                        </para>
-                    </listitem>
-                    <listitem>
-                        <para>
-                            If all goes well, the error is displayed in the 
output boxes. To correct for the error, click <guibutton>Correct Az 
Error</guibutton>. Ekos will now slew to a different point in the sky, and you 
will be required to <emphasis role="bold">ONLY</emphasis> adjust the mount's 
azimuth knobs to center the star in the field of view. The most convenient way 
of monitoring the star field is by going to the <guilabel>Focus</guilabel> 
module and clicking <guibutton>Start Framing</guibutton>. If the azimuth error 
is great, the star might not be visible in the CCD field of view, and therefore 
you have to make <emphasis>blind</emphasis> adjustments (or simply look through 
the finderscope) until the star enters the CCD FOV.
-                        </para>
-                    </listitem>
-                    <listitem>
-                        <para>
-                            Begin your azimuth adjustments until the bright 
star you slewed to initially is as close to center as you can get it.
-                        </para>
-                    </listitem>
-                    <listitem>
-                        <para>
-                            <guibutton>Stop Framing</guibutton> in the <link 
linkend="focus-focuser-group">Focus module</link>.
-                        </para>
-                    </listitem>
-                    <listitem>
-                        <para>
-                            Repeat the <guibutton>Measure Az Error</guibutton> 
to ensure we indeed corrected the error. You might have to run it more than 
once to ensure the results are valid.
-                        </para>
-                    </listitem>
-                    <listitem>
-                        <para>
-                            Switch mode to <guilabel>GOTO</guilabel>.
-                        </para>
-                    </listitem>
-                    <listitem>
-                        <para>
-                            Now slew to a <emphasis 
role="bold">bright</emphasis> star either on the eastern or western horizon, 
preferably above 20 degrees of altitude. It has to be as close as possible to 
the eastern (90 azimuth) or western (270) cardinal points.
-                        </para>
-                    </listitem>
-                    <listitem>
-                        <para>
-                            After slew is complete, capture and solve. The 
star should be dead center in the CCD FOV now.
-                        </para>
-                    </listitem>
-                    <listitem>
-                        <para>
-                            Switch mode to <guilabel>Polar 
Alignment</guilabel>.
-                        </para>
-                    </listitem>
-                    <listitem>
-                        <para>
-                            Click <guibutton>Measure Alt Error</guibutton>. It 
will ask you to slew to a star at either the eastern (Azimuth 90) or western 
(Azimuth 270) horizon which we already done. Click 
<guibutton>Continue</guibutton>. Ekos will now perform the error calculation.
-                        </para>
-                    </listitem>
-                    <listitem>
-                        <para>
-                            To correct for the error, click <guibutton>Correct 
Alt Error</guibutton>. Ekos will now slew to a different point in the sky, and 
you will be required to <emphasis role="bold">ONLY</emphasis> adjust the 
mount's altitude knobs to center the star in the field of view. Start framing 
as done before in the <link linkend="focus-focuser-group">focus module</link> 
to help you with the centering.
-                        </para>
-                    </listitem>
-                    <listitem>
-                        <para>
-                            After centering is complete, stop framing.
-                        </para>
-                    </listitem>
-                    <listitem>
-                        <para>
-                            Repeat the <guibutton>Measure Alt 
Error</guibutton> to ensure we indeed corrected the error. You might have to 
run it more than once to ensure the results are valid.
-                        </para>
-                    </listitem>
-                    <listitem>
-                        <para>
-                            Polar alignment is now complete!</para>
-                    </listitem>
-                </orderedlist>
-                <warning>
-                    <para>
-                        The mount may slew to a dangerous position and you 
might risk hitting the tripod and/or other equipment. Carefully monitor the 
mount's motion. Use at your own risk.
-                    </para>
-                </warning>
             </sect4>
         </sect3>
-    </sect2>
+</sect2>
diff --git a/doc/ekos.docbook b/doc/ekos.docbook
index e7671a699..d1ab9d134 100644
--- a/doc/ekos.docbook
+++ b/doc/ekos.docbook
@@ -42,7 +42,7 @@
     </listitem>
     <listitem>
         <para>
-            Easy to use <ulink 
url="https://www.youtube.com/watch?v=sx6Zz9lNd5Q";>Polar Alignment 
Assistant</ulink> tool. A very quick and reliable tool to polar align your 
German Equatorial Mount!
+            Easy to use Polar Alignment Assistant tool. A very quick and 
reliable tool to polar align your German Equatorial Mount!
         </para>
     </listitem>
     <listitem>
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