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Bi-monthly INDI Library released with new drivers and bug fixes.

- Hy Murveit
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Got it. OK, I just sent Jasem the fix I had asked Jo to try out with his FCUSB. May as well have it in the nightly for others to test, as I'm pretty sure these FCUSB focusers won't work with the linear algorithm the way I wrote it.

If/When you see v3.1 as the linear focus version, you'll have my change and can test again. I'll try and email out on this thread when I see that this change has been pushed.

If/When you see v3.1 as the linear focus version, you'll have my change and can test again. I'll try and email out on this thread when I see that this change has been pushed.

AP1100 & Orion Atlas Pro, WO/ZS105 w/Moonlight V2 focus, GSO RC10 w/RSF focus

ZWO ASI1600, Astronomik Filters, ST80, QHY 5L-IIm.

KStars/Ekos/Indi on NUC10 & RPi4 w/SSD -- Ubuntu

Projects: Greedy Scheduler, Terrain, Polar Align, Analyze, Linear Focuser, SEP MultiStar & GPG Guide, FITS autostretch.

ZWO ASI1600, Astronomik Filters, ST80, QHY 5L-IIm.

KStars/Ekos/Indi on NUC10 & RPi4 w/SSD -- Ubuntu

Projects: Greedy Scheduler, Terrain, Polar Align, Analyze, Linear Focuser, SEP MultiStar & GPG Guide, FITS autostretch.

3 years 1 week ago
#48404

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- Jose Corazon
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This is the same focuser I am using, Hy, so it might be informative to compare the logs from the different sessions. It is interesting that 'The V-curve looks kind of strange, with two sets of points at the same two x-values.' That is also what happened to me sometimes, but not all the time. Obviously, that would mess up the calculation of the curve.

Your revised version of the algorithm may already have taken care of that. I will test once the clouds are gone here, but currently it does not look promising for the entire next week.

Your revised version of the algorithm may already have taken care of that. I will test once the clouds are gone here, but currently it does not look promising for the entire next week.

Atlas Pro AZ-EQ, ASI1600MM-Pro, ASI120MM-S, ES102ED, WO-Z61, Nikon D3300, ASI-EFW, ZWO LRGB,Ha,O3,S2 filter set

3 years 1 week ago
#48406

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- Hy Murveit
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Jasem pushed the change phabricator.kde.org/D26854 it looks about 12 hours before I'm posting this message. So, it's currently in the latest source code, and I'm not sure if it's in the nightly build now or will be tomorrow .

Let me know what you think.

The "two sets of points at the same x-values" issue is not surprising, given that for timer-based focusers like the fcusb, I believe the x-values were wrong, and often not changing without the most recent fix.

Hopefully this won't happen anymore. I don't have one of those focusers, so it's hard for me to test the change without your help.

Hy

Let me know what you think.

The "two sets of points at the same x-values" issue is not surprising, given that for timer-based focusers like the fcusb, I believe the x-values were wrong, and often not changing without the most recent fix.

Hopefully this won't happen anymore. I don't have one of those focusers, so it's hard for me to test the change without your help.

Hy

AP1100 & Orion Atlas Pro, WO/ZS105 w/Moonlight V2 focus, GSO RC10 w/RSF focus

ZWO ASI1600, Astronomik Filters, ST80, QHY 5L-IIm.

KStars/Ekos/Indi on NUC10 & RPi4 w/SSD -- Ubuntu

Projects: Greedy Scheduler, Terrain, Polar Align, Analyze, Linear Focuser, SEP MultiStar & GPG Guide, FITS autostretch.

ZWO ASI1600, Astronomik Filters, ST80, QHY 5L-IIm.

KStars/Ekos/Indi on NUC10 & RPi4 w/SSD -- Ubuntu

Projects: Greedy Scheduler, Terrain, Polar Align, Analyze, Linear Focuser, SEP MultiStar & GPG Guide, FITS autostretch.

The following user(s) said Thank You: Jose Corazon

3 years 1 week ago
#48446

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Great! As I remember, the x values were in the order of 5000, so very far from the other focus algorithms. Sounds like you are on track.

I will test as soon as I get some stars. Next two weeks seem completely cloudy though. Fortunately, the metrologists are often wrong

I will test as soon as I get some stars. Next two weeks seem completely cloudy though. Fortunately, the metrologists are often wrong

3 years 1 week ago
#48460

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- Jose Corazon
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Hy,

The latest focuser algorithm (v3.2) works GREAT with my analog 3D printed focuser based on the Shoestring Astronomy FCUSB focuser.

This is what I get with a 135mm Nikkor lens attached to a cooled ASI183MM. I have a deep red filter in the lightpath, which includes Ha, S2 and extends into the infrared.

This is what my rig looks like (taken this morning after a night of imaging using a 55mm Nikkor Macro lens).

Simple solutions, great results.

Happy to share the STL files for the 3D printed rig, if anyone is interested.

Jo

PS: Here another image of the Linear focus routine, v3.2, this time using SEP, not Centroid.

The latest focuser algorithm (v3.2) works GREAT with my analog 3D printed focuser based on the Shoestring Astronomy FCUSB focuser.

This is what I get with a 135mm Nikkor lens attached to a cooled ASI183MM. I have a deep red filter in the lightpath, which includes Ha, S2 and extends into the infrared.

This is what my rig looks like (taken this morning after a night of imaging using a 55mm Nikkor Macro lens).

Simple solutions, great results.

Happy to share the STL files for the 3D printed rig, if anyone is interested.

Jo

PS: Here another image of the Linear focus routine, v3.2, this time using SEP, not Centroid.

Atlas Pro AZ-EQ, ASI1600MM-Pro, ASI120MM-S, ES102ED, WO-Z61, Nikon D3300, ASI-EFW, ZWO LRGB,Ha,O3,S2 filter set

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- Jose Corazon
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Thanks for writing this code, Hy!

It is very fast and works great with such a simple focuser. Takes care of common backlash issues.

Jo

It is very fast and works great with such a simple focuser. Takes care of common backlash issues.

Jo

Atlas Pro AZ-EQ, ASI1600MM-Pro, ASI120MM-S, ES102ED, WO-Z61, Nikon D3300, ASI-EFW, ZWO LRGB,Ha,O3,S2 filter set

2 years 11 months ago
#48846

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- Hy Murveit
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Thanks Jo.

For everyone: I'm happy to continue iterating and improving this scheme, but at this point have implemented most of what I planned. If anyone has autofocus issue with this algorithm, please send debug logs my way. Please also let me know if it does improve AF where previous focus algorithms didn't perform well.

FYI, the way I've been using autofocus (4" WO f/5.6 refractor with moonlight 2.5" focuser stepper motor and V2 controller) is:

Make sure you have logging set to: Verbose, File, and have at least Focus and Capture set.

Hy

For everyone: I'm happy to continue iterating and improving this scheme, but at this point have implemented most of what I planned. If anyone has autofocus issue with this algorithm, please send debug logs my way. Please also let me know if it does improve AF where previous focus algorithms didn't perform well.

FYI, the way I've been using autofocus (4" WO f/5.6 refractor with moonlight 2.5" focuser stepper motor and V2 controller) is:

- Step size of 25 (that's definitely focuser dependent)
- SEP detection algorithm (haven't carefully compared, but the HFR computation looks better to me this way)
- Full Field HFR measure with annulus of 20% & 75%.
- 5% tolerance
- Max Travel of 400 (probably irrelevant, but don't make it too small)
- no backlash compensation (the moonlight focuser driver doesn't support that anyway.
- 2x2 binning and 3s exposures for RGB and 6s for narrowband gain 200 for my zwo ASI 1600mm

Make sure you have logging set to: Verbose, File, and have at least Focus and Capture set.

Hy

AP1100 & Orion Atlas Pro, WO/ZS105 w/Moonlight V2 focus, GSO RC10 w/RSF focus

ZWO ASI1600, Astronomik Filters, ST80, QHY 5L-IIm.

KStars/Ekos/Indi on NUC10 & RPi4 w/SSD -- Ubuntu

Projects: Greedy Scheduler, Terrain, Polar Align, Analyze, Linear Focuser, SEP MultiStar & GPG Guide, FITS autostretch.

ZWO ASI1600, Astronomik Filters, ST80, QHY 5L-IIm.

KStars/Ekos/Indi on NUC10 & RPi4 w/SSD -- Ubuntu

Projects: Greedy Scheduler, Terrain, Polar Align, Analyze, Linear Focuser, SEP MultiStar & GPG Guide, FITS autostretch.

The following user(s) said Thank You: Jose Corazon

2 years 11 months ago
#48876

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- Chris Rowland
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A quick (I hope) question.

The name implies that the focus algorithm is linear but the display seems to show that the points are fitted to a curve. That looks more like the polynomial method to me.

I'm not objecting, some sort of curve fitting seems better to me because it uses more information.

Chris

The name implies that the focus algorithm is linear but the display seems to show that the points are fitted to a curve. That looks more like the polynomial method to me.

I'm not objecting, some sort of curve fitting seems better to me because it uses more information.

Chris

2 years 11 months ago
#48935

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- Jose Corazon
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I intuitively had the same thought initially. I believe the curve is naturally hyperbolic, but can be fitted near its minimum with good approximation using a polynomial algorithm. To obtain that curve and thus the calculated minimum, Hy’s algorithm will first focus out from a position near optimal focus by 10 steps, then move in by 5 steps (to fully engage the gears and removing backlash), then move past the starting point by 5 steps. The HFR values measured at each step are then used to calculate the curve (from watching it perform, I think that calculation is done after each step move). Then the algorithm will move back OUT past the minimum again and then move IN again using smaller steps toward the calculated minimum.

So the movement during which HFR measurements are taken always proceed in only one DIRECTION.

The advantage is, that this minimizes backlash error, as the gears are always fully engaged. By contrast, the “polynomial” method uses movements in AND out once it has calculated the minimum, which would yield the same result, IF there is no backlash.

So, I think you are correct, both methods use polynomial fitting to a hyperbolic curve, but the original “polynomial “ method uses a bidirectional iteration towards the minimum, while Hy’s method uses a UNIDIRECTIONAL linear iteration which eliminates backlash as a variable.

Perhaps the algorithm should be renamed to ‘Unidirectional’ to avoid this confusion, but Hy should weigh in on that one (and also on whether my account of how I think his algorithm performs is factually correct).

Jo

So the movement during which HFR measurements are taken always proceed in only one DIRECTION.

The advantage is, that this minimizes backlash error, as the gears are always fully engaged. By contrast, the “polynomial” method uses movements in AND out once it has calculated the minimum, which would yield the same result, IF there is no backlash.

So, I think you are correct, both methods use polynomial fitting to a hyperbolic curve, but the original “polynomial “ method uses a bidirectional iteration towards the minimum, while Hy’s method uses a UNIDIRECTIONAL linear iteration which eliminates backlash as a variable.

Perhaps the algorithm should be renamed to ‘Unidirectional’ to avoid this confusion, but Hy should weigh in on that one (and also on whether my account of how I think his algorithm performs is factually correct).

Jo

2 years 11 months ago
#48941

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- Chris Rowland
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Thanks Jo.

I agree that the curve is close to a hyperbola but close to the minumum a polynomial, presumably of degree two seems OK.

Part of the reason I hadn't tried it was the linear name. I don't have a lot of backlash so the current polynomial method works well for me. I didn't want to loose that.

For mounts which can reach a reproducible position but have backlash the second phase could be reduced to a single move out, then a single move to the position calculated in the first phase.

Chris

I agree that the curve is close to a hyperbola but close to the minumum a polynomial, presumably of degree two seems OK.

Part of the reason I hadn't tried it was the linear name. I don't have a lot of backlash so the current polynomial method works well for me. I didn't want to loose that.

For mounts which can reach a reproducible position but have backlash the second phase could be reduced to a single move out, then a single move to the position calculated in the first phase.

Chris

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2 years 11 months ago
#48943

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- Jose Corazon
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Yes, Chris, that would work with stepper motors, but not so well with analog motors which are less precise.

One reason why Hy has designed the algorithm the way he did was to help people like me who are using self-built, primitive analog-based autofocusers. Very adaptable to a wide range of telescopes and cost next to nothing.

That algorithm works REMARKABLY well with the simple 6V micromotor from uxcell I used in the focuser shown in the picture above.

www.amazon.com/30RPM-Shaft-Metal-Gearwhe...7YTWJ364CVV8N9PA3YPE

One can't argue with a $ 7 price tag....

One reason why Hy has designed the algorithm the way he did was to help people like me who are using self-built, primitive analog-based autofocusers. Very adaptable to a wide range of telescopes and cost next to nothing.

That algorithm works REMARKABLY well with the simple 6V micromotor from uxcell I used in the focuser shown in the picture above.

www.amazon.com/30RPM-Shaft-Metal-Gearwhe...7YTWJ364CVV8N9PA3YPE

One can't argue with a $ 7 price tag....

2 years 11 months ago
#48947

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- Hy Murveit
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Chris.

Perhaps I named it poorly, I would be open to renaming it when I remove the "experimental" in the name--so suggestions are welcome. I called it linear, I guess to contrast it to the polynomial algorithm.

The main characteristics of the algorithm (mirroring much of what Jo said) are:

The polynomial that is displayed is used to help find the minimum position, and stopping position, and, for example, as a check to see if there will be a minimum at all for the current sampling plan. A red polynomial means a failure (no minimum, just a maximum). The polynomial is only computed after several samples.

There are some details that may violate the above principles (e.g. it may skip some samples if it thinks it's far from the minimum), but in general that's the way it works.

Hy

Perhaps I named it poorly, I would be open to renaming it when I remove the "experimental" in the name--so suggestions are welcome. I called it linear, I guess to contrast it to the polynomial algorithm.

The main characteristics of the algorithm (mirroring much of what Jo said) are:

- It takes regularly sampled HFR values, i.e. (mostly) moving the position inward by a fixed amount--step size in the 1st pass of the algorithm, and 1/2 step size in the 2nd pass. The polynomial algorithm varies the change in position.
- It hardly ever changes direction, and mostly moves inward. It takes a number of samples inward to establish an approximate minimum-HFR position, then makes a 2nd inward pass looking for that minimum. The polynomial algorithm can move in and out often.
- It only samples the HFR after an inward move. When it needs to move outward, e.g. in between the the 1st and 2nd passes, it moves outward much further than needed, and then back in before capturing an image. Polynomial has no such constraint.

The polynomial that is displayed is used to help find the minimum position, and stopping position, and, for example, as a check to see if there will be a minimum at all for the current sampling plan. A red polynomial means a failure (no minimum, just a maximum). The polynomial is only computed after several samples.

There are some details that may violate the above principles (e.g. it may skip some samples if it thinks it's far from the minimum), but in general that's the way it works.

Hy

ZWO ASI1600, Astronomik Filters, ST80, QHY 5L-IIm.

KStars/Ekos/Indi on NUC10 & RPi4 w/SSD -- Ubuntu

Projects: Greedy Scheduler, Terrain, Polar Align, Analyze, Linear Focuser, SEP MultiStar & GPG Guide, FITS autostretch.

2 years 11 months ago
#48967

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