Just saw this on the QHY twitter feed. Looks very interesting...
http://qhyccd.com/Po...html#PoleMaster
Posted 10 September 2015 - 12:21 AM
Just saw this on the QHY twitter feed. Looks very interesting...
http://qhyccd.com/Po...html#PoleMaster
Posted 10 September 2015 - 01:31 AM
Nice to see someone thinking along new lines.
Blueman
Posted 10 September 2015 - 11:51 AM
The real question is how easy it will be to align to your Ra axis provided you attach it in the finder bracket.
Posted 10 September 2015 - 12:37 PM
Looks interesting. I was unsuccessful in my attempt to find a PDF manual on it at the site.
Posted 10 September 2015 - 01:00 PM
Yeah, PDF is not up yet.
Paul
Posted 10 September 2015 - 01:33 PM
If it attaches to the finder bracket then you better hope that your finder is orthogonal to your actual mount, not the scope, it's mounted on. I looked at the diagram and it does seem to have some push pull screws to get around that problem, though. Hopefully then it would just need to be adjusted once and could be taken down and put back up without losing its position.
If you take down and remount your finder, though, won't it need to be adjusted again? The RAPAS that AP makes attaches directly to the RA axis. That way, once you get it aligned, it just takes 5 minutes or less to be polar aligned (in my limited experience) and it's accurate to a couple of arc minutes.
Rgrds-Ross
Posted 10 September 2015 - 03:51 PM
Interesting. It looks to me as though you could probably rig a means of attachment directly to the RA axis, depending on your mount.
Now, how much is it going to cost?
Posted 10 September 2015 - 06:23 PM
Just for info, we have a small triangular asterism down here that is right near the pole, and i had always wondered if a sensitive camera could be used to locate it.
To get around any need to really refine the axis of the polarscope to the RA axle, i thought that if you declutched the scope and slewed to HA = 6 and took a shot, then moved to HA = -6 and took a shot, it could simply split the difference.
Andrew Johansen Melbourne Australia
Posted 10 September 2015 - 08:52 PM
Interesting. It looks to me as though you could probably rig a means of attachment directly to the RA axis, depending on your mount.
Now, how much is it going to cost?
$199 according to twitter...
If it attaches to the finder bracket then you better hope that your finder is orthogonal to your actual mount, not the scope, it's mounted on. I looked at the diagram and it does seem to have some push pull screws to get around that problem, though. Hopefully then it would just need to be adjusted once and could be taken down and put back up without losing its position.
If you take down and remount your finder, though, won't it need to be adjusted again? The RAPAS that AP makes attaches directly to the RA axis. That way, once you get it aligned, it just takes 5 minutes or less to be polar aligned (in my limited experience) and it's accurate to a couple of arc minutes.
Rgrds-Ross
Yeah I wouldn't take it on and off. I don't use a finder so I could probably be telrad, this, and star sense all on a scope. Also it looks like you could probably figure out how to attach it to the front of the RA axis. This would be really helpful for ASA, Paramount, and CGE Pro mounts without a built in polar scope.
Posted 11 September 2015 - 02:06 AM
Posted 11 September 2015 - 11:15 AM
Would be cool if you could screw this into the hole for the polar scope cover that some mounts have, like mine.!
Posted 11 September 2015 - 06:05 PM
I spoke to someone at a star party once who used his camera to evaluate polar alignment.
He'd set up his image capture software with crosshairs on the center. He'd then do a 10 second exposure, release the RA clutch, and move the RA through its full range.
Polaris would leave a star trail of a half circle. He'd do this a couple of times and adjust the mount so that the crosshairs were at the center of the circle when he did this.
Posted 11 September 2015 - 06:45 PM
Gday WadeH
Polaris would leave a star trail of a half circle. He'd do this a couple of times and adjust the mount so that the crosshairs were at the center of the circle
I think thats the same concept as what i was thinking, but not sure our asterism would leave trails, as its brightest star is around mag 7.0.
I guess if you did a shot at HA = -6 then HA=0 then HA=+6, you could very quicky triangulate an error offset.
The beauty of this method is you dont need to be aligned or tracking, as any tracking related errors near the pole will be negligible.
Andrew Johansen Melbourne Australia
Posted 11 September 2015 - 07:27 PM
Posted 17 September 2015 - 02:54 AM
This device seems to be based on the same principle as my PARot program
http://www.cloudynig...olar-alignment/
If it is the case, then the misalignment of the camera with the axis of the mount is immaterial. I wonder how they implemented the correction for the atmospheric refraction.
Posted 19 September 2015 - 03:53 AM
Posted 19 September 2015 - 02:07 PM
I looked at the video and from what I could see the idea is that since the stars rotate around the pole, all you need to do is to identify the center of their rotation adjust your az/alt and then you are pointing to the pole. I just can't see how that eliminates orthogonal errors between the scope (pointing in one place) and the mount (offset from the scope). I want to point the MOUNT not the scope at the pole. If they are, for any reason, more than a couple of arc minutes different then this method doesn't work. In that case, if you pointed the mount at the pole and rotate the telescope in RA it's going to go around the pole in a circle. Can you explain why this would work? I know I must be missing something, it's so long ago that I took math!
Rgrds-Ross
Posted 19 September 2015 - 08:26 PM
Posted 20 September 2015 - 11:29 PM
So apparently this attaches into the hole in the front of CGE, CGEM, EQ6 and similar scopes.
http://bbs.qhyccd-ba...hp?topic=5057.0
Posted 21 September 2015 - 07:14 AM
Seems like a half-implemented modeling program, what does this accomplish? Way too many mechanical errors unaccounted, and then there is atmospheric refraction.
Posted 21 September 2015 - 09:23 PM
Posted 21 September 2015 - 11:40 PM
All that is involved is the rotation of the ra axis. Other mechanical issues don't matter at all. Refraction can be corrected easily if needed. Not sure if the software does it - but then drift alignment and other methods don't correct for refraction either unless steps are taken.
You do need a view of the pole though. And a computer. And dark sky. But it has clear advantages to me.
Frank
Again, how is this better than a good polar alignment scope and reticle (e.g. Tak, or A-P)? If I'm going to the trouble of hooking up a camera and computer for polar alignment, I might as well go all the way and build a real pointing model.
Posted 22 September 2015 - 12:32 AM
Posted 22 September 2015 - 01:12 AM
All that is involved is the rotation of the ra axis. Other mechanical issues don't matter at all. Refraction can be corrected easily if needed. Not sure if the software does it - but then drift alignment and other methods don't correct for refraction either unless steps are taken.
You do need a view of the pole though. And a computer. And dark sky. But it has clear advantages to me.
FrankAgain, how is this better than a good polar alignment scope and reticle (e.g. Tak, or A-P)? If I'm going to the trouble of hooking up a camera and computer for polar alignment, I might as well go all the way and build a real pointing model.
You clearly don't suffer from bad knees and lower back pain. Be thankful for small blessings
Posted 22 September 2015 - 05:31 AM
Polar alignment has only one goal: to match the polar axis of the mount with the celestial polar axis. Everything else is irrelevant. I guess that Polemaster functionality is based on simple principles which consist of two steps.
1. Once the camera is attached to the polar axis, we find the coordinates of the pixel that represents the axis. A necessary condition is that the camera was at least approximately parallel to the polar axis of the mount. This ensures that the center of rotation (the searched pixel) will be in the camera view. Ideally, it would be possible to carry out the first step in the daytime and only once, if the attachment be reproducible.
2. The relatively short exposure provides an image of stars near the celestial pole. Plate-solving of this image gives the position of the current celestial pole.
In the image we now have two marked points. I'm interested in how the accompanying program will facilitate the whole procedure. It is likely that the first step will be part of every polar alignment.
Edited by KpS, 22 September 2015 - 05:35 AM.
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