Hi
Pixel scale wrong. 120mm = 3.75.
I think to stand a better chance, maybe try an off axis guider.
Good luck, clear nights and stay safe.
Cheers and HTH.
Steve
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** correction. Pixel scale OK. Pixel size 3.8 is near enough.
Sorry
Do NOT run the mount with an 18 volt supply, which Meade switched to from 12 volts.
The capacitors on the boards were not rated high enough and shorted with age.
Worth replacing yours anyway before they go and wreck the boards, very expensive problem.
Plenty of online detail Meade LX200 Classic Capacitor Replacement.
Michael
Wiltshire UK
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Hi Jack. It’s hard to identify the real source of the problem here. I’m sure you know these scopes were never designed for the kind of imaging we do now and I think you should have modest expectations about how well yours will perform. It seems to me you’ve done a lot of good things and have handled the basics. Let’s take a look at a section of the Dec behavior in one of the GA runs you did:

Look at all the fast, frame to frame movement of the guide star, keeping in mind the Dec motor is not running. You can see there are many times when you get 3 arc-sec movements on a rapid basis. This is much too quick to be able to guide out. So it’s not surprising that your guided sessions would show a Dec guiding RMS of 2.6 arc-sec, it would be very hard for it to be smaller. So where does this come from? The likely answer is seeing conditions, keeping in mind that conditions right around the scope can contribute more than the high-altitude effects discussed in web-based seeing forecasts. It could conceivably also come from vibration anywhere from the ground up to the guiding assembly but I think it’s probably seeing. Long focal-length imaging like what you’re trying to do is hard and you are particularly vulnerable to bad seeing conditions - and my understanding is that the UK is well-known for having poor seeing.
In the meantime, you really need to stop flogging the guiding parameters because guiding isn’t going to deal with any of this. But if you have the settings goofed up, you may not be able to take advantage of better conditions when they do arrive. I recommend resetting all the guiding parameters to their default values.
With regard to the uncorrected RA periodic error in your mount, I’d be surprised if the pre-GPS Meade mounts supported permanent periodic error correction. I really think you are bumping up against the limits of trying to use a 25-year old mount that was never well-suited for imaging even when it was new. No offense intended, that’s just my 2-cents worth as an owner of a 2003 LX200GPS.
Cheers,
Bruce
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So Brian, wait until the winds die down, reset PHD2 to the presets, do a new Calibration after nudging North, do a 5 minute Guide Assistant run and accept the changes, then Guide for 20 minutes without further changes to the settings, and post the logs. 1.5 to 2 sec exposures perhaps.
I seem to remember that the Classic has stored PEC that could be learned and updated, and a search confirmed.
This large site was the pinnacle of LX200 Classic facts and figures, and Doc G particularly employed very precise scientic methods in his research and implementation. His methods of beating Diff Flex were legend.
Another suggestion for long FL guiding is Off Axis Guiding, I found the ZWO ASI 120MM was not sensitive enough to immediately find a star when on target.
http://www.skymtn.com/mapug-astronomy/MAPUG/SmartDrv.htm
Michael
Wiltshire UK
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hi Jacki think something is unfortunately amiss in your 1 hour guiding session. the 0.22" total RMS shows literally zero corrections, so i find it hard to believe that was guiding on an actual star.
On Wed, Apr 15, 2020 at 4:04 PM 'Jack Thewlis' via Open PHD Guiding <open-phd...@googlegroups.com> wrote:
--An update on my LX200 odyssey. I've adjusted the dec worm contact/tension and trained the RA PEC using Meade's tedious eight minute stare and press routine. Whether it has improved things remains to be seen. In that context, I've uploaded my latest Guide Log at the link below.During all this, I redid the drift alignment and got it virtually spot on. The GA said it's now somewhere between 0.0 and 0.1 arcminutes in error.The calibration (of which I ran several between various tweeks of the hardware) confirmed a significant Dec backlash,creating an equally significant orthogonality.error. One of the calibrations showed crazy RA steps and no Dec steps at all. .I believe this was a cable issue, which was followed by a repeat of the earlier one. Not withstanding, I finally settled with a guideing run showing a rediculously impressive 0.2 arc second RMS. Surely this is not possible from a twentyfive year old LX200...? Was I really tracking a hot pixel? I don't thnk so, the star mass trace should confirm it.Am I getting somewhere on this path?Cheers,Jack Thewlis
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Hi Jack. You’re not guiding on a real star, it’s just some random clump of non-black pixels on the sensor. To avoid this, you should use the settings in PHD2 to define what is going to be an acceptable guide star for your system. You do that here:

You should use the Star Profile tool to look at typical half-flux-diameter (HFD) values when you know for sure you’re guiding on a reasonable star. From looking at your log, I’d suggest setting this value to 2.0 and see how things go. When you’re getting this “perfect guiding”, the HFD values are more like 0.1 to 0.2px.
That will help you avoid this particular problem. Then you will need to figure out why you aren’t getting more choices with better stars – maybe you’re in a star-poor region of the sky, maybe the guide camera isn’t critically focused, etc. You should go back to 2-sec exposures for now while you are getting this sorted out.
Hope this helps,
Bruce
From: 'Jack
Thewlis' via Open PHD Guiding [mailto:open-phd...@googlegroups.com]
Sent: Thursday, April 16, 2020
4:20 AM
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