Optics data: Ross London Deer Stalker #3

LensBoii

Member
Hi all,

I made an introduction post last night. I'm writing up my investigation into a deer stalking telescope I got in the year 2000. I believe it is the number #3 model from Ross London, without a serial number, circa 1900 AD. I believe it's an imitation made in India. It's quite well-made, smooth draw action, crisp focus but with some aberrations. It came without a case, lens cap or eyepiece shutter. It has blue leather, cross stitched, on the body and the Sun shade. It has 4 knurled edges as seen in the photos (at the end of the writeup).

Not much has been said about all of the lenses themselves, in the originals or imitations. If you can point me to any measurements or specifications, that would be most appreciated. So, I will include my measurements and other observations here, including some geometrical optics calculations. The construction of these telescopes makes it very easy to switch lenses and upgrade them or modify them. There are 5 lenses, including the objective. I have a few photos and an illustration made to scale of the geometrical model.

I like the fact that these telescopes are quite portable and give me a better image than the few binoculars I have owned. My rifle has no separate scope. I also find this telescope useful for general sight-seeing, observing the moon, and just to exercise my eyes. I was shown one at school long ago and my teachers instructed me as to the fragility of the threads, and that the telescope was "worth more than your life"!

Basic measurements:
Weight: 1.2 kg or 2.6 lbs.
Length: 36 1/8" with Sun shade extended, or 33" exactly with it retracted. 11 3/8" closed (unlike original).
OD at edge of shade: 68.5 mm. ID: 63 mm.
OD of Objective lens mount: 58 mm.
OD of Eye relief: 35.5mm. ID: 9 mm.
Balance point: 14.5" from end of extended Sun shade.

Optics:
This is a terrestrial refractor telescope, with original design power of 20x. It did not have any blacking inside. As it has 3 draws, there cannot be baffles. The last draw seems to be twice as long as it needs to be, since the focus comes in at about halfway, whether looking 150ft or at the Moon. The draw closest to the eye (eyetube) may have been interchangeable. There was an upgrade available called a "Pancratic Tube" which was a further extension acting as a zoom lens, but I don't have that and it may have been just for other brands.

There are 5 lenses in the telescope. The objective lens in the original, as far as I know is an achromatic doublet either cemented together or just held together. Mine, as an imitation, may just be a single lens. The inside retaining ring of the Objective has no grip but is screwed in. The other four lenses are held as a pair in each of two cartridges. The cartridges are different lengths. The figures I give below are not exact, and at the principal plane of each lens. I measured focal lengths by imaging the Sun against a dark screen and measuring the focal length. I number lenses starting from the Eye relief.

Objective:
40 mm visible glass. Radius to field side.
Focal length: 450 mm.
All other lenses OD: 21 mm.

Lens number
f (mm)
distance between lenses (mm) or cartridges (( ))
1​
37​
45​
2​
50​
(( 60 ))​
3​
55​
70​
4​
55​

Trying to calculate the magnification is not that difficult, but yielded 8x. The equations were really only valid for lenses closer together. So I switched to ray-tracing the light paths in a full simulation. As below. I used a combination of parallel light rays and a point source, to simulate the stray light. The illustration of my model is to scale, with a scale shown in mm. I can move the objective closer to the eyepiece to make measurements at different focus. I am nearsighted. The brown lines are just to show an outline of the boundaries of the telescope tubes.

Telescope model.webp

Close up at Eye tube:

Telescope model close.webp

As the eye is placed at the focal point in the eye relief, you can see the image. I haven't measured focus with my spectacles on. Between lenses 3 and 4, inside that lens cartridge was a small black stop, with a hole of 3.5mm. The stop is about 2mm thick with the outer ring to hold it in place is 5mm thick. It was in the wrong position and I think the diameter is wrong, so I just removed it. It needs some precise calculations and testing for it to be useful in making the image sharper.

If you extend the rays at the Eye relief back to the Objective plane, you can measure magnification. It is indeed 20x as it should be. However, I can only see a clear image on a sunny day at 8x magnification with the eye tube pushed in half way.

I hope this is useful for restorers.

You can change these lenses, with better ones. Coated lenses, achromatic doublets, etc. You can also change positioning of the lenses to increase magnification. I might make a separate post about that. I was able to get 80x with this telescope. Those images are rather dim and the field of view is a small fraction of a degree. I think 8x to 20x suits my purposes. I might only use 80x to see a planet if I'm out on a clear night on the hill. It is notable to me that the "Erector tube" (lenses 3 and 4) seem to perform the image inversion at the very end or even outside of itself as I have it focussed. I need more tests to know where to put the stop. Any information from you is welcomed.

Here are the photos! Note the heavy brass bushes have no glands or packing and are perfectly machined for a smooth draw. It feels like a 1 or 2 thou clearance at most. The threads are all smooth except for the eye shield. That metal is so thin that threads on the shield surface were only cut on one half of the circumference! So it has to be whacked on halfway and then screwed the rest of the way. There is a little felt inside the largest bush. No shutter.

Fully extended
20231024_134023.webp

Closed
20231024_134102.webp

Objective end-on view
20231024_134119.webp

4 more photos in next post...
 

There is a very good search function on this forum. @caberslash wrote a superb article on draw scopes.

I now have two Ross scopes. An Aluminium one which I regularly use out in the field, and a better condition brass one which is a bit heavier so it stays at home.
 
Eye Relief end-on
20231024_134139.webp

Closed showing stitching on leather and knurling

20231024_134215.webp

Order of assembly: Objective to body, Sun shade to body, first draw tube, second draw tube, lens cartridges x2 (containing 4 lenses total) to Eye tube, Eye tube to the second draw tube, Eye relief to Eye tube. (With obligatory lens cleaning).
20231024_134601.webp

Engraving or punching
20231024_134622.webp

As it was brighter today, I tried focusing on very nearby objects. At full extension, the closest object I can see clearly is at 10-12 feet. At 30 feet I am around the normal focus length which I used a Sharpie marker to mark. How do you all mark yours? This focus setting is good to about 300 ft. I haven't calibrated beyond that. I want to etch or otherwise mark ranges on the Eye tube.

I think someone replied as I was posting this half of the pictures!

It was my pleasure to share this information, and I look forward to any information the community can contribute to this thread.
 
Caberslash on here could be a possible starting point.?


There is a very good search function on this forum. @caberslash wrote a superb article on draw scopes.

I now have two Ross scopes. An Aluminium one which I regularly use out in the field, and a better condition brass one which is a bit heavier so it stays at home.

Thank you @finnbear270 and @Heym SR20 ! Indeed I used that writeup before I added my contributions and measurements. My writeup is geared towards geometrical optics and lens specifications and my other thoughts. Maybe I should cross-reference my writeup with theirs.
 
@LensBoii ,

Sorry to say, but you've bought a cheap, Indian made fake (off eBay?)

The quality shown in the draws (brass tubes), lenses and leatherwork are all very poor.

Seem to remember warning others in my booklet about such reproductions, which are not a touch on the originals.

Unfortunately, you are not the first one to make this mistake.
 
@LensBoii ,

Sorry to say, but you've bought a cheap, Indian made fake (off eBay?)

The quality shown in the draws (brass tubes), lenses and leatherwork are all very poor.

Seem to remember warning others in my booklet about such reproductions, which are not a touch on the originals.

Unfortunately, you are not the first one to make this mistake.

Thanks for confirming my suspicions @caberslash . I might as well leave this up for the lens data I measured and geometry for people coming in from Google searches in 2123
:lol:

Now I have an excuse to beat up on this one, use it hard and experiment with lenses and carry it in a chunk of PVC pipe :gheyfight:
 
Update with experimental results - useful if you want to know any telescope better. Plus the method. Some older vets might have known, but it's written here now.

Results: (correct for 20:20 or 6/6 vision)
Magnification = 19.94x +/- 0.7x
Field of view = 1.63 degrees +/- 0.004 degrees (98 minutes of arc).


This compares well with people saying it is 20x and the brochure photos in the linked thread.
Knowing the field of view, you can now calibrate your own vision and range estimation abilities.

Experimental method:
I focused through the telescope on a brick wall at 120 ft in clear daylight. I adjusted my position until I could see 5 whole bricks with half a width of mortar on each end. I slightly moved my eye to focus at the limits of the field of view. I measured the width of the bricks and mortar. Then I simply used trigonometry to calculate the angular size.
That will give you the apparent angular size *at that distance* that the bricks appear to be - in degrees or radians or arc minutes (as you prefer and convert).
Then I measured out the same width of bricks and marked it on my living room wall about 7 feet away with electrical tape. I took off the eye relief and held it in the same position as if I were looking through the telescope. Then I walked closer to the wall until the marked brick width filled the field of view. Measure the distance to the wall from your eye, d, for this.
If the distance to the object is d and the width is w, use this formula twice. Once for through the telescope, and once for through your bare eyes. You can paste the formula straight into a google search and google calculates it directly. This is in degrees. Use your own values for w and d. Ignore when it says "rad" as I built in the conversion to degrees.

(arctan (w / d)) x (180 / PI) x 2

You will get two numbers for angular size of five bricks across. The first is the field of view of the telescope at 120 feet (for me) and the second was the angular size with bare eyes of the bricks. Divide the second number by the first and you have the magnification. Correcting for near or far sightedness gets complicated, but for most people in a range of +/-5 dioptre spectacles, they will narrow or widen the field of view and magnification by up to around 2.75% respectively (with this telescope). See here for more: link

If you want to be more accurate you can do this at multiple distances and get all scientific. But 120ft is enough distance to get a decent idea about your telescope. Measuring at close range will increase the inaccuracy of your calculations. It's a full moon tonight so I can get a very accurate figure at such a great distance.


Good Observing.
 
No need to mark the tubes. It doesn’t take long to learn how to focus. I pull to nearly full length and then squeeze it down till you get an infocus image.

It is far quicker to drop down using your knee as support and be onto and looking at a beast, than getting a modern scope out spreading tripod etc etc.
 
No need to mark the tubes. It doesn’t take long to learn how to focus. I pull to nearly full length and then squeeze it down till you get an infocus image.

It is far quicker to drop down using your knee as support and be onto and looking at a beast, than getting a modern scope out spreading tripod etc etc.

Great points @Heym SR20 ty.

I've gotten some muscular memory after practising for a week for focus. It just happens automatically now, even without looking through the eyepiece.

I agree that this is much faster and field-expedient than setting up with a tripod. Years of holding long metal objects have made my arms more stable than I realised. When I set it up to 80x mag, I can hold a target and scan even though the FOV is only 24 arc minutes. Some of the positions I tried are comedic, like lying back and using my knee to prop it with my hand resting on the knee.

I also find holding the knurled end of the eyetube with one/two fingers and the rest of the tube with the others, I can quickly micro-adjust focus when looking between brambles to a deeper depth of focus. I have big hands though. It's quite nice to be able to count dew drops on a blade of grass at 500 ft (but rather dim at 80x). Or 125 ft at 20x.

About 30-40 mag seems most useful at most - by customising lenses. As a compromise between brightness and colour purity.

Now I'm going to practise with it more. I can get obsessed with gear like many of us. A passerby complimented the telescope and I showed him how to use it and tended to his dog as he learned how to observe the moon. Something really nice about doing this on a moonlit night. Its also funny that he unscrewed the eye relief to focus :rofl:
 
I have a pleasant surprise! I was wondering why I was getting such good image quality from this telescope, especially sharp focus and colours. I finally managed to be a bit tougher with the objective lens mount - and it does turn apart to release the glass within. Polishing the lens in circles helped loosen it, clockwise looking in from outside. Then gripping the thin retaining rim (from inside) with part of my thumb while riding the threads with the rest (possibly getting cuts) worked. Anticlockwise from the inside as it is a normal right-hand thread). I will lightly use some wire wool to soften these threads for the future.

What I found surprised me. When the originals were made, they used an achromatic doublet objective lens - which brings red and blue light into focus at a point, but not green. The eye only sees three colours (Red, Green and Blue), your brain creates millions of colours based in intensity of each of those three.

I expected that this, being a copy, might just have a singlet. I was shopping for doublet or better lenses. Quality glass is expensive. I was happy to see that the objective in mine is already a modern design apochromatic triplet! For astro photography and astronomy (more than enough for terrestrial).

This means it is 3 times better than the design of the authentic ones, as it brings red, green and blue all into focus, and solves major Seidel aberrations. I'm quite happy with that, as it saves me time shopping and £££. The edge is sealed in blacking to prevent separation and mold growth and edge reflections. I'm glad whoever made it chose this design. They also tuned the eye tube as I have tested with different cartridge spacing. Somebody knew what they were doing! If you have one, you can identify it is a triplet by carefully releasing the objective and looking at the edge. You will see three lenses cemented together as ridges in the blacking.

As per these diagrams from Wikipedia:

Apochromat diagram.webp

Apochromat.webp

Not bad eh? For me, utility is mostly what I was interested in. The beauty was a bonus.

Coated lenses are better for reflections and transmission, but you normally find those in binoculars and cameras and compact eyepieces as they are squeezing a lot of optics in a small space. The reason I have some colour fringing is because of the eyetube lenses, which are simply plano-convex singlets like the original. They are in a Ramsden configuration. It is relatively easy to just switch those out with achromatic doublets to make a Plössl configuration. Or better yet, apochromatic triplets with coatings.

The objective is 42mm diameter and 4.2mm thick at the edge. The Sun shade protects from off-axis reflections. The fact that it is thin reduces transmission losses. Commercially available ones are often 8-10mm thick, but there are thinner ones.

Now it makes sense to delve into my collection of fancy aspheric lenses with coatings for the eye tube. Some Televue lenses are ££££ expensive.
But I happen to have about 100 lenses to play with. I might just modify the "Erector Tube" :fib::norty:
in-situ and 3-d print an adaptor for a collection of quality eyepieces.


Happy Days :stir:;)
 
I did some more observations and testing. The eyepiece is not really a Ramsden configuration but looks like a stretched out Huygens eyepiece. I'm basically reverse engineering at this point to recover lost information. Huygens eyepieces work really well with focal ratios of f/10 and slower (bigger denominator). This one is f/11.25. They don't work with modern and faster focal ratios. What they do is, by spacing the two lenses at the eye side, it corrects for spherical and chromatic aberration very well, considering.

There is some theory I forget, but to treat this properly, you have to calculate wavefronts to several orders and the calculus starts getting scary.

I manually ray traced the optics on a spreadsheet and it matched my experiments to 0.1%, so good enough for this task. I will explain how it's faulty to think of the first cartridge (Lenses 4 and 3) as the "erector tube" and the second cartridge (Lenses 2 and 1) as the eyepiece. Lens 4 (closest to objective) is the field lens of the eyepiece. Lenses 3 and 2 are the erector lenses - they flip the image right-side-up. Lens 1 is the Eye lens of the eyepiece.

Following the path of light from the object.
Assume the distant object produces parallel rays of light to the objective, just to simplify things. Note this is a HUGE assumption and is really only good for a notional picture. The objective is apochromatic, so makes a near perfect focus (upside down image) at it's focal length. This makes a cone of light on Lens 4 as I have numbered, which is located at its own focal length away from this point. Lens 4 creates a collimated beam (parallel again). But it has a smaller diameter, so has condensed optical information spatially, so there is a magnification factor here (as the eye would see it at that point). This beam has now captured aberrations. It goes to Lens 3, where it again gets focused to a point, the image flipped upside down and onto Lens 2, where the reverse happens and you have a collimated beam. If Lenses 3 and 2 were identical, there would be no magnification here and it is possible aberrations would cancel out of Lenses 3 and 2. In my case Lens 2 was aspheric and biconvex. That would correct spherical aberrations of the Objective. Lens 4 focuses the image to a series of points called the "eye point". I use the word "focus" very loosely, because a relaxed eye prefers parallel rays. It is a complex topic how the eye forms an image. The Apparent Field of View is about 32.6 degrees of this eye tube. I used an array of point sources of light to improve my model, and all variations create a "circle of confusion" about +/- 1mm radially and laterally from that point. I can omit Lens 1 and still see the central field in focus (about 1/5 th of the FOV), but not the periphery. Designing the field stops and positions takes more calculating. It is worthy to note, that the final stage of magnification occurs within the eye itself in this setup, accounting for about 2.1-2.2x of the system magnification.

So, in the scale model drawing I made in black in the first post, I count lenses from the eye to the objective.
The erector tube is actually not either of the two cartridges, but the sections of them at Lenses 3 and 2 and the empty space between them. This is where a field stop should go of the correct aperture and OD and position (if you want one).

The cartridge of Lenses 2 and 1 look like a Huygens eyepiece in that the spacing of the lenses and their differing focal lengths can almost exactly cancel chromatic and/or spherical aberration. However, remember, this is a very long eye tube spread out 220mm from outer lens surfaces (ignoring curvature). The two middle lenses are the erector lenses - a type of optical relay. The eyetube is much like a rifle scope on its own, minus an Objective, and with a minor tilting ability.

At some point in the past, someone I know pranked me by jumbling around the lenses and losing collimation. Collimation is very important. All the lenses should be centred and aligned, at least in the eye tube. I think Lens 2 should be swapped with Lens 4, to correct the spherical aberrations of the Objective. The curvatures of these should both face the objective. Then the erector lenses would be a symmetric pair. I need to check which way those lenses should face. I would have to either do a lot of calculations or just swap them and see. So I would not need any fancy lenses to correct for spherical or chromatic aberration as it is all done by the manufacturer.

Today I looked through a tree at 150ft at a bird at 500ft. It was a pigeon, and I could see it's eye and beak clearly, and rustling head hairs/feathers. There was a blue fringe against open sky about 5% laterally. But I am yet to re-collimate. At 1000 feet and medium contrast at ground level, deer-size objects seem fine.

There is a very good sponsored paper with more data:
Chromatic Aberration of Eyepieces in Early Telescopes
M. Eugene Rudd
link
that covers Dollond and other telescopes from this time, but not Ross as much.
My write up nicely complements that paper.

I found that O rings can be a quick and cheap way to take up slack in the lens mounts radially but not axially, and to seal out dust, but you need to dry the air inside if you use them or make a gap for air movement.

You will notice from one lens cleaning to the next, the image might get worse. This is from a collimation issue, the lenses should sit exactly square to the axis.


Good Observing
 
I'm up early updating my computer. So here are some updates while I wait.

I did some exact measurements for tuning collimation of lenses in the eye tube cartridges. There were different sized gaps because of the way lenses in general are made. Exact lens mounts for a single lens can cost ££££ if you're doing high-end work for a single mount!

In the temperatures I use this telescope in, expansion and contraction made a minimal effect. So, armed with measurements, I made thin shims with clear tape on black paper. More or less tape got me to the right thicknesses. My lenses have pre-roughed edges to reduce reflections. The black paper was a bonus. I got mine from WHSmith a while ago. Then I cut very thin strips equal to the lens cavity they were going into. Then curved them around the eye tube to get them to curl. I pulled them against a small cylindrical object to ensure absolutely no kinks from the tape. It's important to leave 50-100 microns of room for expansion/contraction inclusive. Then I cut them to length and carefully finessed the strips into each lens cavity with a pin. Then I dropped in each lens straight, with hardly any pressure, just a gentle twist to get past the edge. I made sure I could still feel a little movement. Leave the lenses in the mounts for now - in order, so you don't mess up. I then cut more black paper to black the inside of the eye tube cartridges. That is easy as the lenses sit flush to those tubes, or you can leave about 1mm of clearance if you need. I curled the paper around the outside of the cartridges to get a shape and then gently placed them inside. I calculated the width of the paper using c=pi x d, where d is the ID measured with Vernier calipers. This way there was no seam and an exact fit. A little overlap will not hurt.

Before I did all this, I cleaned the threads with a very soft and worn down sanding block, but you can use steel wool - gently. I checked the tubes were cut square. The longer cartridge needed squaring at each end as the cuts formed a parallelogram. Off-square by about 0.1mm at each end. I squared these with a small emery board, about 40 strokes softly. I just used a metal engineer's square on its inside corner. Rotated the tube in the corner to check the squareness around the circumference. Took about 25 minutes. Then I flattened it by gently twisting on a piece of glass paper (harder than brass). If it mattered much I would do a final lap on a sharpening stone. A final check with the square all around each end of the cartridge tube ensured it was square to less than 1 thou off along the length (thou means I thousandth of an inch). Soften the edges with the glass paper or steel wool, so they don't chip the lenses.

Then I ensured there was no dust anywhere and could re-assemble. Took a deep breath and made sure I held each lens mount so gravity was keeping my lens down against the inside of the mount. I cleaned the inside of the lens with one cotton bud soaked in isopropyl alcohol (lenses were uncoated) and drying with a separate cotton bud with the spare end for polishing. Blow off any tiny speck of dust left. Then I screwed in the cartridge tube from above - holding everything at eye level to keep alignment. Repeat for each lens.

Now I had close to perfect collimation in the cartridges themselves. I could have gone overboard with lasers, but I think that was too much. A visual inspection was enough. Then I had to collimate the cartridges to the eye tube. This was much easier, again using Vernier calipers for measurement. I just used clear tape around the OD of the cartridges at each end until they matched the ID of the eye tube - with about 0.05 mm of clearance inclusive. My tape was really thin at 0.025mm (about 25 microns). It should be fairly snug but not forced fit.

Then I cleaned the outer surfaces of the lenses and fit the cartridges into the eye tube. After a few years, the blacking paper might sag, but it doesn't take long to change that. My paper could have been a darker shade, but it didn't matter - it was much better than shiny brass. I could just soak some black ink into the paper next time.

What I found is, this dramatically improved the image quality. At day and night. There was no movement of the image anymore, even if the draw tubes were pushed to the limits of their play side-to-side or up/down. There were some thin felt packing in the bushes I found, which could be a little thicker.

There was much better contrast in the image also. I tested the limits of my vision. I chose a crater on the Moon that was about equal in magnified angular size equal to the field of view of a single cone cell of my retina. I could pick out these details. It is pretty much at the diffraction limit of the telescope lenses and my eye! Needless to say, I was quite impressed when I did the calculations. The chromatic aberration was imperceptible on the features and there was no perceptible spherical or other aberrations.

By studying "Chromatic Aberration of Eyepieces in Early Telescopes" again, at the table at the end - the closest telescope optics are the:

563 Dollond Military with these measured specifications by the Author:
Focal length: –23.1mm (mine is -22.5mm)
Axial Chromatic Aberration (CA) of the eyepiece as a percentage of its focal length: –5.2%
Lateral CA of the eyepiece as a percentage of its focal length: 0.44%
Axial CA of the eyepiece: 1.21
Axial CA of the objective: –1.18
Total axial CA of the telescope as a percentage of the focal length of the objective: 0.0008%.

  • This is remarkable for a telescope of its time, and was used for military purposes.
  • I observed about the same Lateral CA or less (at the edges of a bright object - like the Moon).
  • As I have a longer telescope overall, and better objective, my Total axial CA was about 0.0002%.
  • Axial CA measures colour blur across the visual field.
  • Lateral CA measures colour fringes at sharp boundaries of objects with contrast.
That last number includes a couple of fudge factors. But I'm very happy with the result.

I tried to find similar objective lenses. Only singlets are so thin as commercially available. Doublets are about 6mm-8mm at the thinnest. Triplets get to around 12mm and are very expensive.

I have checked mine to be a triplet. The only way to fake it would be to mill the edges, which is expensive to do and who would care to check it when buying? This lens is a mystery. It's not a doublet or I would see more CA in one colour only. I reason it must have been made special for armed forces, as it would be very expensive to make such a lens for the general public. This jogged my memory of the man selling it to me being so enthusiastic about that lens and that this was a military issue telescope. Which accounted for the price. As for the marking - I think not many of these find their way to the UK. I bought it during my travels to Asia. I'm guessing they were made under license for the Indian Army/Navy/AF. There is no easy explanation for the lens. The image quality is better than the Dollond. Just a thick doublet costs about £165 excluding VAT and a thick triplet is like £800 ex VAT. A thin custom triplet made for field-polishing (without coatings) sounds like something militaries would justify the huge expense of.

There is a decent lens industry in India.
I guess I could ask their Navy. This lens has intrigued me.
I definitely want to make some lens caps now!

I still need to make the spacer for the objective - but that will be 3d printed with a fancier design for temperature compensation. Also a few thin sleeves for collimating the draw tubes better. This is exciting for me.

It's also tempting to get one of those fancy cases made up. But on that point. I like to travel light. I have never seen the body of these types of telescopes crushed. Only dents in draw tubes. When you travel, it is closed. So the only vulnerability is the lenses, in my humble opinion. So, for now I will make some 3d printed caps (which you can do in brass now), and some pretty case when I feel fancy.

More detailed aberration calculations are probably too much for this arena.


Good Observing.
 
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