Equinox Systems GEMINI Manuel d'utilisateur Page 39

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Gemini Users Manual 34
To solve this problem, Gemini now allows you to set a “GoTo Limit” to define a point
past which Gemini will always GoTo the object so that the telescope tube is on the east
side of the mount. Gemini will allow the mount to track past this point, but will not
GoTo any object west of this point without a meridian flip, if needed, to put the telescope
tube on the east side of the mount. Refer to section 5.3.10.2.6 for a description of the
“Set GoTo” limit command.
3.4 Polar Alignment
3.4.1 Definition
Polar alignment is the process of aligning the mount’s polar (RA) axis with the Earth’s
rotational axis. It involves physically adjusting the elevation and azimuth of the mount,
usually accomplished by turning adjustment knobs. Although the mount does not need
to be level to be polar aligned, a level mount can make the alignment process much easier
since adjusting the elevation knob on a level mount just moves the mount in elevation
(and the same for the azimuth adjustment). Moving the elevation knob on a mount that is
not level introduces some azimuth component as well. While leveling is an important
time saver for the Drift Alignment method, it is not necessary at all if you intend to use
Gemini's Polar Axis Correction feature. As mentioned earlier, an accurately polar aligned
mount can track the motions of the sky by driving just the RA motor.
3.4.2 Techniques
There are several techniques that you can use to polar align your mount. Each method
varies in the amount of time it takes and the accuracy it can achieve.
3.4.2.1 Polar Alignment Scope
Most of the German equatorial mounts supported by Gemini have the option of installing
a polar alignment scope (PAS). This is a small telescope that is attached to the mount
parallel to the mount’s polar axis. In most cases, it is actually installed inside the hollow
RA axis. Inside the alignment scope is a reticle with markings for certain alignment
stars. The idea is to adjust the mount in elevation and azimuth until the alignment stars
match up with the marks on the reticule. You should of course refer to the instructions
for your particular polar scope for complete details.
Using a polar alignment scope can be very fast. Its accuracy depends primarily on how
well calibrated the reticle is and the degree of mechanical play between the polar scope
and the mount. For a well-calibrated polar scope, you can expect to be within 2 or 3
minutes of the actual refracted pole. The accuracy is also limited because the stars around
the pole are lifted up somewhat by refraction (most noticeable at lower latitudes). The
PAS will therefore align your mount to the "refracted pole.”
3.4.2.2 Drift Method
The drift method of polar alignment is probably the most accurate and most time
consuming method. It involves centering a couple of well-chosen stars in an eyepiece
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