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Re: Trying establish step size - the question is what is mirror travel per focuser turn.

 

oops again, further correction:

at C-14 FL (391 cm):?
1u at FP = 0.05" at FP
1u of axis error =?0.0045" at FP?(0.05" / f-11)

thus?FWHM bloat for 132u axis error (264u?DOF)?= 0.6"
?
Not acceptable for hi-res; e.g. 1.0 vs 1.6 is 60% obviously worse.
Undesirable for mediocre res; e.g. 3.0" vs 3.6" is 20% noticeably worse.
Almost negligible for low-res; e.g. 5.0 vs 5.6 is 12% marginally worse.

Stan


Re: Trying establish step size - the question is what is mirror travel per focuser turn.

 

Oops! I forgot that C14 is F/11 (I've been using C-11 at f/10 lately)

mathematical revisions:

at C-14 FL (391 cm): 1u at FP = 0.05"
Focus error is arithmetically additive (not quadratic)?so 1u of axis error adds?0.005" to?FWHM

If axis error = 132u (DOF 263 / 2) then FWHM is bloated by 0.67". That's (still) terrible!

If virtual FWHM = 1.0" then max FWHM within DOF = 1.7" (awful)
if virtual FWHM = 2.0" then max FWHM within DOF?= 2.7" (nasty)

So my conclusions are basically the same.

Stan


Re: Trying establish step size - the question is what is mirror travel per focuser turn.

 

"In ideal seeing conditions, with this telescope in the f/10 configuration, we have a depth of focus of 263 microns ... just under 1/3 of a turn of the focus knob"

The rings very untrue.?With good seeing I can easily distinguish degradation within less than 1/10th turn.

at C-14 FL (356 cm): 1u at FP = 0.06" at FP
Focus error is arithmetically additive (not quadratic)?so 1u of axis error adds?0.006" to?FWHM

If axis error = 132u (DOF 263 / 2) then FWHM is bloated by 0.8". That's terrible!

If virtual FWHM = 1.0" then max FWHM within DOF = 1.8" (awful)
if virtual FWHM = 2.0" then max FWHM within DOF?= 2.8" (pretty nasty)

Assuming your calculation is correct, then 1/10th turn error = 0.24" at FP, which is still not all that great.? And that's why many users get a Feather Touch.

Stan


Re: Trying establish step size - the question is what is mirror travel per focuser turn.

Gary Jarrette
 

With any thread the travel of the nut on a screw is equal to the reciprocal of the (TPI) threads per inch. So on a shaft that has a thread pitch of 32 you would divide 32 into 1. You would then get .0313 inches of travel of the nut per turn of the shaft.



In the case of 24 threads TPI, you would get 1/24 or .0417 inches of travel of the nut in one turn of the shaft or just over a millimeter which is .03937 inches.



Most calculators have a Reciprocal Key on them. It is the key that has 1/X or one over X on it. To get travel of any nut or whatever on a threaded Rod or Screw simply put in the pitch, the TPI (Threads Per Inch), push the Reciprocal button and viola you get the travel, how far the nut will advance in one turn of the shaft.



Micrometers use a screw with a pitch of 40, this is a very fine thread. This gives it its characteristic 25 thousandths of an inch for one turn of the barrel or .025 inch.



I hope this helps and clears up your question.



It works the same with metric threads but the units change of course. Be careful not to mix the two.



Gary Jarrette

US Precision

18328 E. Sunnybrook Lane

Gilbert, AZ 85298

USA

Maker of the world famous KISS Focusers

For QSI and SBIG OAG Guide Cameras.



602-312-8797



<mailto:garyjarrette@...> garyjarrette@...











From: C14_EdgeHD@... [mailto:C14_EdgeHD@...]
Sent: Tuesday, May 22, 2018 11:34 AM
To: C14_EdgeHD@...
Subject: [C14_EdgeHD] Re: Trying establish step size - the question is what is mirror travel per focuser turn.





Well what was the measurement?





[Non-text portions of this message have been removed]


Re: Trying establish step size - the question is what is mirror travel per focuser turn.

Gary Jarrette
 

Standard Focusing Mechanism <>

The focusing mechanism that comes standard with the Celestron CPC 1100is illustrated to the right. As the focus knob is rotated, the focuser either pushes or pulls a threaded rod, that is connected to the primary mirror, in or out.

The rod and the focuser have a thread pitch of approximately 0.8 threads per millimeter. In other words, each rotation of the knob moves the primary mirror in or out 0.8mm, or 800 microns.

In ideal seeing conditions, with this telescope in the f/10 configuration, we have a depth of focus of 263 microns. So the entire depth of focus can be traversed with just under 1/3 of a turn of the focus knob. With degraded, but great, seeing conditions where the seeing disk is 2¡å in diameter, the depth of focus increases to 542 microns, or 2/3 of a turn of the focus knob. It seems reasonable to expect, and experience has demonstrated, that achieving focus with these constraints is straightforward.

However, when this system is configured to operate at f/2 the depth of focus under ideal conditions is reduced to just 10.5 microns. Even with a seeing disk of 2¡å the depth of focus is only 21 microns. The entire depth of focus is traversed with 1/78 and 1/38 of a turn of the focus knob respectively. These are very tight tolerances that would make achieving focus very difficult.





From: C14_EdgeHD@... [mailto:C14_EdgeHD@...]
Sent: Tuesday, May 22, 2018 11:34 AM
To: C14_EdgeHD@...
Subject: [C14_EdgeHD] Re: Trying establish step size - the question is what is mirror travel per focuser turn.





Well what was the measurement?


Re: Trying establish step size - the question is what is mirror travel per focuser turn.

 

Well what was the measurement?


Re: Trying establish step size - the question is what is mirror travel per focuser turn.

 

Nevermind....took care of this myself.


Trying establish step size - the question is what is mirror travel per focuser turn.

 

I am curious about how far the mirror moves per rotation of the focus knob? ?Or more practically, how far per 10 turns?


In characterizing my autofocuser, I need to know the travel per step of the focuser motor.


Re: Optimization of the positionning of the Schmidt plate in a C14

 

Maybe.? But it seems "common sense" that moving the corrector forward should cause over-correction.? The spot diagram clearly shows that effect on-axis but it is presumably a non-diffraction monochromatic geometrical ray trace.? ?

The geometrical difference might be overwhelmed by diffraction and obscured by chromo but it is still there.? And spider diffractions that result from extending the plate do not help either.??See if you can convince Christopher Go to modify his C14! <g>

In regards to wider FOV a good question is: do you get a better limiting PSF (on and off axis) via plate-distance modification or via lens corrections?? Is Edge-HD inferior to classical SCT on-axis?? What about off-axis compared to this modification?

Stan


Re: Optimization of the positionning of the Schmidt plate in a C14

 

I would agree with Christian.

The ultimate on-axis spot diagram can always be reached by the combination of wavelength and back-focus... sphero-chromatism is really the limiting factor in SCT's

--

On Thu, Dec 28, 2017 at 10:11 AM, viladrich christian christian.viladrich@... [C14_EdgeHD] <C14_EdgeHD@...> wrote:

?

Hello Stan
As a matter of fact, the spot diagrams are a bit deceptive. On the optical axis, the Strelh ratio are about the same with / without moving the plate.
I would say that the main benefit of the modification is for high resolution narrow field imaging (eg. lunar imaging).
Christian
?

Le 28/12/2017 ¨¤ 16:36, stan_ccd@... [C14_EdgeHD] a ¨¦crit?:
The spot diagrams show that the on-axis spot is much smaller for?the normal plate distance than the extended placement.? So this trick would be destructive for narrow FOV such as planetary.? As for wide FOV, there are correctors that achieve similar spot sizes without moving the plate (re Starizona reducer/corrector).

However, if one were to re-formulate and make a?concentric?corrector then you could have the best of both.? Of course it is unlikely that anyone will do so...

Stan




Re: Optimization of the positionning of the Schmidt plate in a C14

 

¿ªÔÆÌåÓý

Hello Stan
As a matter of fact, the spot diagrams are a bit deceptive. On the optical axis, the Strelh ratio are about the same with / without moving the plate.
I would say that the main benefit of the modification is for high resolution narrow field imaging (eg. lunar imaging).
Christian
?

Le 28/12/2017 ¨¤ 16:36, stan_ccd@... [C14_EdgeHD] a ¨¦crit?:

The spot diagrams show that the on-axis spot is much smaller for?the normal plate distance than the extended placement.? So this trick would be destructive for narrow FOV such as planetary.? As for wide FOV, there are correctors that achieve similar spot sizes without moving the plate (re Starizona reducer/corrector).

However, if one were to re-formulate and make a?concentric?corrector then you could have the best of both.? Of course it is unlikely that anyone will do so...

Stan



Re: Optimization of the positionning of the Schmidt plate in a C14

 

The spot diagrams show that the on-axis spot is much smaller for?the normal plate distance than the extended placement.? So this trick would be destructive for narrow FOV such as planetary.? As for wide FOV, there are correctors that achieve similar spot sizes without moving the plate (re Starizona reducer/corrector).

However, if one were to re-formulate and make a?concentric?corrector then you could have the best of both.? Of course it is unlikely that anyone will do so...

Stan


Re: Optimization of the positionning of the Schmidt plate in a C14

 

¿ªÔÆÌåÓý

Hi Charles,

The coma is much lower with the plate moved forward by 400 mm.

Here are the spot diagrams over a 0.25¡ã field and the classic design. We can see a nice coma:



And with the plate moved forward by 400 mm:


The field curvature is about the same.

Best regards

Christian



Le 27/12/2017 ¨¤ 05:39, charles genovese drgenovese@... [C14_EdgeHD] a ¨¦crit?:

Christian - how do coma and field curvature change as the corrector is moved forward.?
Charles


On Tuesday, December 26, 2017 11:36 PM, charles genovese wrote:


The first 2 images show the rear cell with holes drilled under the fan - much easier than cutting a big hole- and the inside wiring. The picture of the side of the tube with the fan is under the dovetail rail which will be eventually modified with stick on side pieces (and small pieces at the front and back) to make the rail into a conduit to circulate air. (there is also a hole in the tube just below the corrector cell). There are also 4 1" holes in the tube just below the corrector to exhaust air from the fans from the rear cell. When not in use the holes are simply covered with blue painter's tape. when air is just being "circulated the rear fans and 4 holes are covered. Otherwise they are uncovered and the inside of the scope comes to thermal EQ with the surrounding air
Charles




On Tuesday, December 26, 2017 4:32 AM, "viladrich christian christian.viladrich@... [C14_EdgeHD]" wrote:


?
Hi Charles,
Can you post some images of your tube ? I only have two 80 mm holes at the back of the mirror, each of them with a 90 mm fan. This is much better than nothing, but I can see you push it one step further.
Thanks !

Le 26/12/2017 ¨¤ 02:15, charles genovese drgenovese@... [C14_EdgeHD] a ¨¦crit?:
I eliminated tube currents in mine by first putting two 4" fans on the back and 4 holes in the tube under the corrector. With about a 10 degree temp difference it comes to thermal eq in about 30 minutes. and then the fans can just be turned off and it tracks the temperature drop perfectly. But as the temperature would drop to the dew point (it's never very far away here in Louisiana) the inside of the corrector would dew up because of the tube temperature dropping below ambient. This was virtually completely resolved by wrapping the tube in aluminized bubble wrap (from Lowes) but now I have a carbon fiber tube (pretty good insulator) and the bubble wrap is unnecessary. ? I also cut 2 2" holes in the tube- one just ahead of the rear cell and the second just behind the corrector cell all unde r the dovetail and glued a small fan in the rear hole half way countersunk in the tube. I planned to put some plastic (or aluminum) along each side of the rail to seal to the tube so as to make a tunnel to circulate air from front to back (the other holes would be covered) but I haven't gotten around to adding the sealing strips and testing it. I like the low profile Celestron rail which keeps the scope as close as possible to the mount. (I also have one that I may add to the top of the tube with another fan).?
Charles


On Monday, December 25, 2017 4:51 PM, "Benoit Schillings benoit.schillings@... [C14_EdgeHD]" wrote:


?
Hello Charles. I am away from home, so cannot get the right ray tracing...
but :

I do plan to have a small counterweight to keep the secondary assembly in
line... basically on the outside of the corrector.

My C14 is now tubeless, having no tube is really a great improvement Imo.
no more tube currents at all !

-- benoit

On Mon, Dec 25, 2017 at 2:35 PM, drgenovese@... [C14_EdgeHD] <
C14_EdgeHD@...> wrote:

>
>
> Hi Benoit- have been a fan for years :-) I certainly don't doubt your
> ability to build stuff! But supporting a fairly heavy secondary 200mm back
> will be a challenge to avoid vibration and maintain alignment. What would
> the diffraction limited field be at that distance? I too considered putting
> my corrector at the optimal distance - 1400mm- with a carbon fiber tube but
> decided against it. Is field curvature the only aberration with the
> corrector at about prime focus? The field curvature of a C14 is about the
> same as that of a 6"f/8 refractor (1/7th focal length vs 1/3rd). A field
> flattener for a 6" f/8 refractor should be pretty close it would seem.
> I just haven't tried that yet. Charles
>
>
>

[Non-text portions of this message have been removed]










Re: Optimization of the positionning of the Schmidt plate in a C14

 

Christian - how do coma and field curvature change as the corrector is moved forward.?
Charles


On Tuesday, December 26, 2017 11:36 PM, charles genovese wrote:


The first 2 images show the rear cell with holes drilled under the fan - much easier than cutting a big hole- and the inside wiring. The picture of the side of the tube with the fan is under the dovetail rail which will be eventually modified with stick on side pieces (and small pieces at the front and back) to make the rail into a conduit to circulate air. (there is also a hole in the tube just below the corrector cell). There are also 4 1" holes in the tube just below the corrector to exhaust air from the fans from the rear cell. When not in use the holes are simply covered with blue painter's tape. when air is just being "circulated the rear fans and 4 holes are covered. Otherwise they are uncovered and the inside of the scope comes to thermal EQ with the surrounding air
Charles




On Tuesday, December 26, 2017 4:32 AM, "viladrich christian christian.viladrich@... [C14_EdgeHD]" wrote:


?
Hi Charles,
Can you post some images of your tube ? I only have two 80 mm holes at the back of the mirror, each of them with a 90 mm fan. This is much better than nothing, but I can see you push it one step further.
Thanks !

Le 26/12/2017 ¨¤ 02:15, charles genovese drgenovese@... [C14_EdgeHD] a ¨¦crit?:

I eliminated tube currents in mine by first putting two 4" fans on the back and 4 holes in the tube under the corrector. With about a 10 degree temp difference it comes to thermal eq in about 30 minutes. and then the fans can just be turned off and it tracks the temperature drop perfectly. But as the temperature would drop to the dew point (it's never very far away here in Louisiana) the inside of the corrector would dew up because of the tube temperature dropping below ambient. This was virtually completely resolved by wrapping the tube in aluminized bubble wrap (from Lowes) but now I have a carbon fiber tube (pretty good insulator) and the bubble wrap is unnecessary. ? I also cut 2 2" holes in the tube- one just ahead of the rear cell and the second just behind the corrector cell all unde r the dovetail and glued a small fan in the rear hole half way countersunk in the tube. I planned to put some plastic (or aluminum) along each side of the rail to seal to the tube so as to make a tunnel to circulate air from front to back (the other holes would be covered) but I haven't gotten around to adding the sealing strips and testing it. I like the low profile Celestron rail which keeps the scope as close as possible to the mount. (I also have one that I may add to the top of the tube with another fan).?
Charles


On Monday, December 25, 2017 4:51 PM, "Benoit Schillings benoit.schillings@... [C14_EdgeHD]" wrote:


?
Hello Charles. I am away from home, so cannot get the right ray tracing...
but :

I do plan to have a small counterweight to keep the secondary assembly in
line... basically on the outside of the corrector.

My C14 is now tubeless, having no tube is really a great improvement Imo.
no more tube currents at all !

-- benoit

On Mon, Dec 25, 2017 at 2:35 PM, drgenovese@... [C14_EdgeHD] <
C14_EdgeHD@...> wrote:

>
>
> Hi Benoit- have been a fan for years :-) I certainly don't doubt your
> ability to build stuff! But supporting a fairly heavy secondary 200mm back
> will be a challenge to avoid vibration and maintain alignment. What would
> the diffraction limited field be at that distance? I too considered putting
> my corrector at the optimal distance - 1400mm- with a carbon fiber tube but
> decided against it. Is field curvature the only aberration with the
> corrector at about prime focus? The field curvature of a C14 is about the
> same as that of a 6"f/8 refractor (1/7th focal length vs 1/3rd). A field
> flattener for a 6" f/8 refractor should be pretty close it would seem.
> I just haven't tried that yet. Charles
>
>
>

[Non-text portions of this message have been removed]









Re: Optimization of the positionning of the Schmidt plate in a C14

 

¿ªÔÆÌåÓý

Hi Charles,
Can you post some images of your tube ? I only have two 80 mm holes at the back of the mirror, each of them with a 90 mm fan. This is much better than nothing, but I can see you push it one step further.
Thanks !

Le 26/12/2017 ¨¤ 02:15, charles genovese drgenovese@... [C14_EdgeHD] a ¨¦crit?:

I eliminated tube currents in mine by first putting two 4" fans on the back and 4 holes in the tube under the corrector. With about a 10 degree temp difference it comes to thermal eq in about 30 minutes. and then the fans can just be turned off and it tracks the temperature drop perfectly. But as the temperature would drop to the dew point (it's never very far away here in Louisiana) the inside of the corrector would dew up because of the tube temperature dropping below ambient. This was virtually completely resolved by wrapping the tube in aluminized bubble wrap (from Lowes) but now I have a carbon fiber tube (pretty good insulator) and the bubble wrap is unnecessary. ? I also cut 2 2" holes in the tube- one just ahead of the rear cell and the second just behind the corrector cell all unde r the dovetail and glued a small fan in the rear hole half way countersunk in the tube. I planned to put some plastic (or aluminum) along each side of the rail to seal to the tube so as to make a tunnel to circulate air from front to back (the other holes would be covered) but I haven't gotten around to adding the sealing strips and testing it. I like the low profile Celestron rail which keeps the scope as close as possible to the mount. (I also have one that I may add to the top of the tube with another fan).?
Charles


On Monday, December 25, 2017 4:51 PM, "Benoit Schillings benoit.schillings@... [C14_EdgeHD]" wrote:


?
Hello Charles. I am away from home, so cannot get the right ray tracing...
but :

I do plan to have a small counterweight to keep the secondary assembly in
line... basically on the outside of the corrector.

My C14 is now tubeless, having no tube is really a great improvement Imo.
no more tube currents at all !

-- benoit

On Mon, Dec 25, 2017 at 2:35 PM, drgenovese@... [C14_EdgeHD] <
C14_EdgeHD@...> wrote:

>
>
> Hi Benoit- have been a fan for years :-) I certainly don't doubt your
> ability to build stuff! But supporting a fairly heavy secondary 200mm back
> will be a challenge to avoid vibration and maintain alignment. What would
> the diffraction limited field be at that distance? I too considered putting
> my corrector at the optimal distance - 1400mm- with a carbon fiber tube but
> decided against it. Is field curvature the only aberration with the
> corrector at about prime focus? The field curvature of a C14 is about the
> same as that of a 6"f/8 refractor (1/7th focal length vs 1/3rd). A field
> flattener for a 6" f/8 refractor should be pretty close it would seem.
> I just haven't tried that yet. Charles
>
>
>

[Non-text portions of this message have been removed]





Re: Optimization of the positionning of the Schmidt plate in a C14

 

¿ªÔÆÌåÓý

It would be nice to have a look at some images of your tubeless C14 when your are back home.
Christian

Le 25/12/2017 ¨¤ 22:51, Benoit Schillings benoit.schillings@... [C14_EdgeHD] a ¨¦crit?:

Hello Charles. I am away from home, so cannot get the right ray tracing...
but :

I do plan to have a small counterweight to keep the secondary assembly in
line... basically on the outside of the corrector.

My C14 is now tubeless, having no tube is really a great improvement Imo.
no more tube currents at all !

-- benoit

On Mon, Dec 25, 2017 at 2:35 PM, drgenovese@... [C14_EdgeHD] <
C14_EdgeHD@...> wrote:


Hi Benoit- have been a fan for years :-)  I certainly don't doubt your
ability to build stuff! But supporting a fairly heavy secondary 200mm back
will be a challenge to avoid vibration and maintain alignment. What would
the diffraction limited field be at that distance? I too considered putting
my corrector at the optimal distance - 1400mm- with a carbon fiber tube but
decided against it. Is field curvature the only aberration with the
corrector at about prime focus? The field curvature of a C14 is about the
same as that of a 6"f/8 refractor (1/7th focal length vs 1/3rd). A field
flattener for a 6" f/8 refractor should be pretty close it would seem.
I just haven't tried that yet. Charles








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Posted by: Benoit Schillings 
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Re: Optimization of the positionning of the Schmidt plate in a C14

 

¿ªÔÆÌåÓý

Very interesting. I have found that moving the plate 200 mm forward increases the diffraction limited flat field from 2.2 arcmin (nominal design) to 4.1 arcmin (in green light).
With 200 mm, you will probably still have a good access to the collimation screws.
Christian


Le 25/12/2017 ¨¤ 22:04, Benoit Schillings benoit.schillings@... [C14_EdgeHD] a ¨¦crit?:

Christian, I am rebuilding my C-14 (will send photos) but decided that moving 200 mm forward would be a good tradeoff (also based on Oslo) between length and field of view. the nice thing with 200 mm is that I can (I think) built it without a spider, just a 3d printed holder that will span the gap.

-- benoit

On Mon, Dec 25, 2017 at 4:49 AM, viladrich christian christian.viladrich@... [C14_EdgeHD] <C14_EdgeHD@...> wrote:
?

Dear All,

I played around with OSLO to found out what is the optimal positioning of the Schmidt plate with the classic C14 design (ie. not relevant to the Edge-HD).

It turned out that if the Schmidt plate is set 400 mm ahead of its original position, the radius of the field limited by diffraction is enlarged by 4 (9 arcmin instead of 2.2 arcmin). This is not as large as the C14 Edge-HD (12.4 arcmin) but not far away.

Of course, the optical tube becomes much longer (there is no free meal ...).

The other optical characteristics do not look to be affected (Strelh ratio on the optical axis, variation of focus with wavelength).

More information here :

Best regards

Christian Viladrich






Re: Optimization of the positionning of the Schmidt plate in a C14

 

Wow 40 degrees- here the total temp variation from 2 PM to 6 AM is rarely more than 20 degrees but much less during the night! Typically only about 6-8 degrees from twilight to midnight and a slower drop after that to the minimum at dawn. I guess due to the high humidity
Charles



On Monday, December 25, 2017 8:55 PM, "Benoit Schillings benoit.schillings@... [C14_EdgeHD]" wrote:


?
I do have 3 fans on the back, but the temperature change in California during the evening is pretty steep... often a change of 40 degrees F. I have typically found that even if I had the fan running for a few hours, some tube currents would still appear when I turn the fans off (Carbon tube).

If the current experiment of tubeless C14 works, I will replace the current Aluminum beams with carbon tubing.

-- benoit

On Mon, Dec 25, 2017 at 6:15 PM, charles genovese drgenovese@... [C14_EdgeHD] <C14_EdgeHD@...> wrote:
?
I eliminated tube currents in mine by first putting two 4" fans on the back and 4 holes in the tube under the corrector. With about a 10 degree temp difference it comes to thermal eq in about 30 minutes. and then the fans can just be turned off and it tracks the temperature drop perfectly. But as the temperature would drop to the dew point (it's never very far away here in Louisiana) the inside of the corrector would dew up because of the tube temperature dropping below ambient. This was virtually completely resolved by wrapping the tube in aluminized bubble wrap (from Lowes) but now I have a carbon fiber tube (pretty good insulator) and the bubble wrap is unnecessary. ? I also cut 2 2" holes in the tube- one just ahead of the rear cell and the second just behind the corrector cell all under the dovetail and glued a small fan in the rear hole half way countersunk in the tube. I planned to put some plastic (or aluminum) along each side of the rail to seal to the tube so as to make a tunnel to circulate air from front to back (the other holes would be covered) but I haven't gotten around to adding the sealing strips and testing it. I like the low profile Celestron rail which keeps the scope as close as possible to the mount. (I also have one that I may add to the top of the tube with another fan).?
Charles


On Monday, December 25, 2017 4:51 PM, "Benoit Schillings benoit.schillings@... [C14_EdgeHD]" <C14_EdgeHD@...> wrote:


?
Hello Charles. I am away from home, so cannot get the right ray tracing...
but :

I do plan to have a small counterweight to keep the secondary assembly in
line... basically on the outside of the corrector.

My C14 is now tubeless, having no tube is really a great improvement Imo.
no more tube currents at all !

-- benoit

On Mon, Dec 25, 2017 at 2:35 PM, drgenovese@... [C14_EdgeHD] <
C14_EdgeHD@...> wrote:

>
>
> Hi Benoit- have been a fan for years :-) I certainly don't doubt your
> ability to build stuff! But supporting a fairly heavy secondary 200mm back
> will be a challenge to avoid vibration and maintain alignment. What would
> the diffraction limited field be at that distance? I too considered putting
> my corrector at the optimal distance - 1400mm- with a carbon fiber tube but
> decided against it. Is field curvature the only aberration with the
> corrector at about prime focus? The field curvature of a C14 is about the
> same as that of a 6"f/8 refractor (1/7th focal length vs 1/3rd). A field
> flattener for a 6" f/8 refractor should be pretty close it would seem.
> I just haven't tried that yet. Charles
>
>
>









Re: Optimization of the positionning of the Schmidt plate in a C14

 

I do have 3 fans on the back, but the temperature change in California during the evening is pretty steep... often a change of 40 degrees F. I have typically found that even if I had the fan running for a few hours, some tube currents would still appear when I turn the fans off (Carbon tube).

If the current experiment of tubeless C14 works, I will replace the current Aluminum beams with carbon tubing.

-- benoit

On Mon, Dec 25, 2017 at 6:15 PM, charles genovese drgenovese@... [C14_EdgeHD] <C14_EdgeHD@...> wrote:
?

I eliminated tube currents in mine by first putting two 4" fans on the back and 4 holes in the tube under the corrector. With about a 10 degree temp difference it comes to thermal eq in about 30 minutes. and then the fans can just be turned off and it tracks the temperature drop perfectly. But as the temperature would drop to the dew point (it's never very far away here in Louisiana) the inside of the corrector would dew up because of the tube temperature dropping below ambient. This was virtually completely resolved by wrapping the tube in aluminized bubble wrap (from Lowes) but now I have a carbon fiber tube (pretty good insulator) and the bubble wrap is unnecessary. ? I also cut 2 2" holes in the tube- one just ahead of the rear cell and the second just behind the corrector cell all under the dovetail and glued a small fan in the rear hole half way countersunk in the tube. I planned to put some plastic (or aluminum) along each side of the rail to seal to the tube so as to make a tunnel to circulate air from front to back (the other holes would be covered) but I haven't gotten around to adding the sealing strips and testing it. I like the low profile Celestron rail which keeps the scope as close as possible to the mount. (I also have one that I may add to the top of the tube with another fan).?
Charles


On Monday, December 25, 2017 4:51 PM, "Benoit Schillings benoit.schillings@... [C14_EdgeHD]" <C14_EdgeHD@...> wrote:


?
Hello Charles. I am away from home, so cannot get the right ray tracing...
but :

I do plan to have a small counterweight to keep the secondary assembly in
line... basically on the outside of the corrector.

My C14 is now tubeless, having no tube is really a great improvement Imo.
no more tube currents at all !

-- benoit

On Mon, Dec 25, 2017 at 2:35 PM, drgenovese@... [C14_EdgeHD] <
C14_EdgeHD@...> wrote:

>
>
> Hi Benoit- have been a fan for years :-) I certainly don't doubt your
> ability to build stuff! But supporting a fairly heavy secondary 200mm back
> will be a challenge to avoid vibration and maintain alignment. What would
> the diffraction limited field be at that distance? I too considered putting
> my corrector at the optimal distance - 1400mm- with a carbon fiber tube but
> decided against it. Is field curvature the only aberration with the
> corrector at about prime focus? The field curvature of a C14 is about the
> same as that of a 6"f/8 refractor (1/7th focal length vs 1/3rd). A field
> flattener for a 6" f/8 refractor should be pretty close it would seem.
> I just haven't tried that yet. Charles
>
>
>

[Non-text portions of this message have been removed]





Re: Optimization of the positionning of the Schmidt plate in a C14

 

I eliminated tube currents in mine by first putting two 4" fans on the back and 4 holes in the tube under the corrector. With about a 10 degree temp difference it comes to thermal eq in about 30 minutes. and then the fans can just be turned off and it tracks the temperature drop perfectly. But as the temperature would drop to the dew point (it's never very far away here in Louisiana) the inside of the corrector would dew up because of the tube temperature dropping below ambient. This was virtually completely resolved by wrapping the tube in aluminized bubble wrap (from Lowes) but now I have a carbon fiber tube (pretty good insulator) and the bubble wrap is unnecessary. ? I also cut 2 2" holes in the tube- one just ahead of the rear cell and the second just behind the corrector cell all under the dovetail and glued a small fan in the rear hole half way countersunk in the tube. I planned to put some plastic (or aluminum) along each side of the rail to seal to the tube so as to make a tunnel to circulate air from front to back (the other holes would be covered) but I haven't gotten around to adding the sealing strips and testing it. I like the low profile Celestron rail which keeps the scope as close as possible to the mount. (I also have one that I may add to the top of the tube with another fan).?
Charles


On Monday, December 25, 2017 4:51 PM, "Benoit Schillings benoit.schillings@... [C14_EdgeHD]" wrote:


?
Hello Charles. I am away from home, so cannot get the right ray tracing...
but :

I do plan to have a small counterweight to keep the secondary assembly in
line... basically on the outside of the corrector.

My C14 is now tubeless, having no tube is really a great improvement Imo.
no more tube currents at all !

-- benoit

On Mon, Dec 25, 2017 at 2:35 PM, drgenovese@... [C14_EdgeHD] <
C14_EdgeHD@...> wrote:

>
>
> Hi Benoit- have been a fan for years :-) I certainly don't doubt your
> ability to build stuff! But supporting a fairly heavy secondary 200mm back
> will be a challenge to avoid vibration and maintain alignment. What would
> the diffraction limited field be at that distance? I too considered putting
> my corrector at the optimal distance - 1400mm- with a carbon fiber tube but
> decided against it. Is field curvature the only aberration with the
> corrector at about prime focus? The field curvature of a C14 is about the
> same as that of a 6"f/8 refractor (1/7th focal length vs 1/3rd). A field
> flattener for a 6" f/8 refractor should be pretty close it would seem.
> I just haven't tried that yet. Charles
>
>
>

[Non-text portions of this message have been removed]