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ATM 8" binoculars



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>From atm-owner  Tue Jun  3 04:09:21 1997
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Date: Tue, 3 Jun 1997 18:08:56 +1000 (EST)
From: Mark Suchting <masuch@tip.csiro.au>
To: John Graves <john.graves@nashville.com>
cc: ATM List <atm@shore.net>
Subject: Re: ATM Binocular Telescope ( long post )
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On Sun, 1 Jun 1997, John Graves wrote:

> My next project is going to be a 8 inch binocular telescope... I'm thinking
> f5.5 or so. Anyone have any suggestions about this focal ratio... should it
> be slower or faster? Any tips on grinding two mirrors to the same focal
> length and how much tolerance do I have regarding the f.l. of the two
> mirrors.?

John,

I built 8" F8's 11 years ago now. I recommend f7.5 for comfortable 
viewing at the zenith with the standard `looking over your shoulders' design.

I include here some notes I posted to this list some time ago, new list 
members may be interested also. They were responses to questions from 
an American amateur whose name now escapes me who used them at a star party 
here in Australia in 1994?

> Last question, does anyone happen to remember which issue of S&T > had
>the article where the ATM made a binocular telescope and had a really >
>well designed observing chair for it? 

Not sure but there was a much more detailed write up on them by the 
builder, appearing in a recent ATM Journal issue. The article has been 
fully converted to HTML and appears on their web site. Binocular chairs 
look pretty cumbersome to me. The author of the article for the `Voyager' 
instrument states that he only uses 28X because his heartbeat vibrates 
the image. I find that 1OOX with 65 degree apparent field eyepieces is 
most valuable for me, so I would be wary to tackle a chair until others 
had evaluated this problem. 

At the moment I am designing a Dobsonian mount for my 20 X 80 binoculars 
using a pair of folding mirrors like a big Amici prism to give me a 90 
degree bend in the light path, for viewing comfort, and an altitude axis 
passing through the base of the scull ( virtually speaking!) so I can 
have all the comfort of a binocular chair without all the bulk.. I'll 
keep the list posted.

Mark Suchting 


########################################################################

NOTES ON  8" NEWTONIAN BINOCULAR CONSTRUCTION

1. What is the ideal focal length for an 8" binocular telescope?

I think the ideal focal length is one where you can point the telescope at
the zenith and observe comfortably with your feet firmly on the ground. I
am 5' 10" (178 cm) and at F8 I have to just stand on my tip toes. F7.5
would have been perfect. Binocular eyepieces tend to get very close to the
ground at the horizen, so the more focal length and the higher the 
balance point, the better. 

I originally chose F8 so the field of good definition would be enormous, 
and having no knowledge of the mechanical tolerances required, I played 
it safe.  If I had made F4 first off the project would 
have initially failed...  On this topic, I would make one mirror movable 
temporarily in the X-Y plane before you lock them down so you can adjust 
them so you have good collimation at high power in each side when the 
images are merged. This would be a very sensitive adjustment below F5.

2. What is the tolerance on the focal length of the primary mirrors? I
there a % tolerance ? 

The figure I see repeatedly in the books is that the brain can accomodate
difference in image size of 1%. If we make .5% our top tolerance for
safety, we must decide on our desired high magnification. I usually use
mine at 200X tops, only because that is the limit of eyepiece comfort.
This is achieved with an 8mm focal length. Our 0.5% tolerance represents a
magnification difference of 1X which of course means an allowable focal
length difference of 8mm.  My mirrors are within 1mm FL but that is
probably overkill. I found when I was employed in optical mass manufacture
of telescope mirrors that two mirrors coming in succession off the same
tool would frequently be within a few mm FL. If your mirrors are ground
alternate wets on the same tool, this should be fine. 

3. When using the eyepieces can you use two eyepieces that the
manufacturer states as 16mm for example, or do they have to be matched to
close tolerances ? 

I was suspicious, and working for a retailer at 
the time enabled me to borrow eyepieces first to test their suitability. I 
tested pairs by viewing a distant paper scale through a barlowed C8 to 
check for magnification difference. I found no detectable differances. If 
you want to see the effect, try putting in a 15mm on one side and 16mm on 
the other! I frequently try pairs of eyepieces i don't own at star 
parties, and have never had any problem with differing magnification.

4. As I recall you had a control box with push buttons to make the
alignment change and cause the two images to coincide. Can you please
provide me with some details as to how this control box does the
alignment? Is one of the primary mirrors shifted? 


I set up my motorised right primary, not so much for myself, but to 
help other people view through the binoculars. For some inexplicable reason 
their are subtle differences between collimation settings between people. 
I think it has a lot to do with how accurately thay set their inter-pupil 
distance, because the problem seems much less marked at higher powers, 
where the eye pupil is overfilling the telescope exit pupil. People 
rarely have to adjust collimation at X100 but often at X50. You also get 
small errors in eyepiece centering with the higher powers. I found it 
very difficult to collimate the binos for people when I was doing the 
adjustment at the back via verbal instruction from the observer. People 
not familiar with binocular telescopes just don't understand what they 
are seeing. I found with the two axis push button control that people could 
play with the buttons and collimate without instruction. When they are in 
control it seems to come naturally, even with people unfamiliar with 
using telescopes. 

In my set up I have my right mirror on a plywood plate about 10" square. 
I have Edmund 2 rpm 3 volt DC gear motors mounted  on diagonal corners 
with their shafts pointing to the bottom of the tube. In the other corner 
I have a cap head bolt going through the mirror mount base plate into a 
t-nut hammered into the front of the mirror mount plate.It goes through a 
spring sandwiched between the two boards. This way if I need to make an 
adjustment to the overall foacl plane position on the right side, I can 
turn this bolt from outside the telescope. Then turn the two motorised XY 
collimation bolts to level the mirror up again. I have only done this 
once. The motor shafts are attached to small collars which attach the 
motor shafts to a lengths of 5/32" threaded rod which like the corner 
bolt pass through sandwiched springs and then into t - nuts hammered into 
the main mounting plate. One corner is thus unsupported, but I have only 
noticed a very slight loss of collimation at high power when I go to the 
horizen.  

To clarify then, we have the vertical motor in the top left corner
of the mirror plate, the corner pinion bolt in bottom left corner and the 
horizontal adjustment motor on the bottom right corner. I found the 2rpm 
motor driving the 3/16" rods just right for this scope. As far as wiring 
the handbox, I mounted a battery pack in the handbox and they have been 
going for 5 years. I wired a simple circuit with two discreet connections 
to the battery for each motor,  giving reverse directions. I'm sure it 
could have been done more elegantly. An expert friend tells me I could 
short the thing if I hold down two buttons at once, but I've had no 
problems yet. For my next binocs I will probably dispense with the motors 
and have two rods running down the tube to drive the mirror adjustments, 
particularly if my 20" binocs ever get built.

5. We intend to make the binoculars as a Dob design. Is there any
differeces when making it fit two telescopes ? 

 There is no problem using the Dobsonian mount. Most Newt dobs are built
like this. I think the side boards need to be thicker due to the extra
load of the tube assembly. I cut big holes in my side boards to save
weight and now they are flaring out under the weight of the tubes. I like
box section sides ie pine frames with thin plywood skins: they are very
rigid and light. My 24" is built this way. 


Just a couple of minor points on mirror collimation.

1. When you are adjusting the the collimation it is good to throw the
focus on the adjustable primary mirror out till you see a small `donut'. 
Then move the `donut' around till it is centered on the in focus star in
the other eye. I found that if you have them both focused, your eyes will
chase ahead of the motors and try and strain the images to merge. It can
then get very confusing and stressful trying to collimate this way. When
you are more experienced you can collimate by moving the image around
while your eyes have pulled thje images together, finding the point at
which your eyes feel most relaxed and comfortable. I find after using them
for years that my eyes have much better accomodation for fusing images
than most. 

 We are used to converging our eyes to see close in stereo but most people
have very little vertical accomodation. Your scope must be rigid in the
vertical direction at least. Even if the images are 25% of the field apart
in the horizontal you can often pull them in. The result is a strange bowl
effect to the field and overlapping field edges. If people get way out
with the collimation I often just centre the star in one eye, moving
collimation on the other mirror to also center it in its own field then
open both eyes for fine adjustment. 

2.  Our accomodation for field rotation is ZERO ! The adjustment of
tertiary mirrors rotating around their own optical axis effects this
adjustment. I am talking here about the tiniest nudge ! If the feilds are
rotated slightly you cant see it easily but the view looks strange at
lower power and you can get a headache that lasts for days... 

The way I adjust this, is to go to the highest power, picking two stars 
that are separated by most of the field. I then decollimate in a vertical 
direction enough to see a parallogram of 4 stars. If the two sides of the 
parallelogram aren't parallel then you have field rotation. A slight 
rotation of the tertiary mirror (  around the axis coming out the side of 
the tube ) will move two stars in the field but also rotate the optical 
axis. Move the stars again by primary collimation to form the 
parallelogram until you see parallel sides. As you get better you can 
move the star pair till thay are almost merged for fine tuning.

Doing these adjustments will ensure you get no eye strain at lower powers.

*********************************************************************



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