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This list uses the idcomm address because sendmail is not configured to
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-- 
Ken Lowther
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From mayen1@mwt.net Sun Dec  2 16:42:18 2001
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Subject: [Raytrace] THANKS!!!
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Thanks soooo very much for starting this.  I don't know what it is, but I have
downloaded many ray tracing programs and never have figured out how to use any
of them.  geez!!

Thanks

Joe


From crawford@goingware.com Sun Dec  2 17:08:52 2001
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From: "Michael D. Crawford" <crawford@goingware.com>
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Subject: [Raytrace] Greetings from Mike
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Hi,

I just joined this list after seeing the announcement on the ATM list.  I 
thought I might have something useful to contribute.

I have a long history of _attempting_ to raytrace, without a lot of success.  I 
used to use the procedures I found in Amateur Telescope Making, only with a hand 
calculator instead of trig tables and an adding machine.

Some of my earliest attempts at computer programming were trying to write 
raytracing programs in either FORTRAN or C.  I wasn't a good enough programmer 
back then to do it, but I am now - I've been programming as a career for over 14 
years.

I downloaded OSLO LT recently and plan to use it to study the design for my 8" 
ritchey-chretien, but haven't messed with it yet.

But I'm thinking, over a long period of time, of writing an optical design 
program that would be Free Software in the sense that the Free Software 
Foundation puts it - it would be licensed under the GNU General Public License, 
and so would come with source code.

I think it's great that OSLO LT is provided as freeware but I think it would be 
better if people had a powerful tool that they also possessed the source to, 
with the right to make and redistribute modifications.

So I don't want to just know how raytracing is done working with existing 
programs, I'm interested in understanding how these programs work internally, 
the algorithms and data structures used, what would be the requirements for a 
really useful tool and so on.

Also any program I would write would be cross-platform, probably using the 
ZooLib cross-platform application framework (http://zoolib.sourceforge.net/) so 
you could run it on any OS you like.

I have a web page about my telescope making at

http://www.geometricvisions.com/atm/

When I started college I majored in astronomy at CalTech.  I later changed my 
major to Physics and transferred to the University of California at Santa Cruz, 
where I successfully petitioned for credit in UCSC's optics course because of my 
experience making telescopes as a teenager.

Mike
-- 
Michael D. Crawford
GoingWare Inc. - Expert Software Development and Consulting
http://www.goingware.com
crawford@goingware.com

   Tilting at Windmills for a Better Tomorrow.

     "I give you this one rule of conduct. Do what you will, but speak
      out always. Be shunned, be hated, be ridiculed, be scared,
      be in doubt, but don't be gagged."
      -- John J. Chapman, "Make a Bonfire of Your Reputations"
         http://www.goingware.com/reputation/


From bolenb@pacbell.net Sun Dec  2 17:37:19 2001
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Here's a first one for the archives.  What software is recommended for =
raytracing?

Joseph B. Goins
1091 Harness Circle #1
San Ramon, CA 94583
(925) 277-1351

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<DIV><FONT face=3DArial size=3D2>Here's a first one for the =
archives.&nbsp; What=20
software is recommended for raytracing?</FONT></DIV>
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<DIV><FONT face=3DArial size=3D2>Joseph B. Goins<BR>1091 Harness Circle =
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From klowther@cisnet.com Sun Dec  2 18:27:31 2001
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John is workikng on some preliminary information and was waiting to give
people a chance to sign up before getting started.  OSLO will probably be
the software of choice.  There is a free download version that does more
than us amatures are going to need.

Ken

----- Original Message -----
From: Joseph Goins <bolenb@pacbell.net>
Sent: Sunday, December 02, 2001 7:37:43 PM
To: <raytrace@blackhole.idcomm.com>
Subject: [Raytrace] Where do you get the software for Raytracing?

> Here's a first one for the archives.  What software is recommended for
raytracing?
> 
> Joseph B. Goins
> 1091 Harness Circle #1
> San Ramon, CA 94583
> (925) 277-1351


From klowther@cisnet.com Sun Dec  2 18:32:10 2001
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From: klowther@cisnet.com
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Subject: Re: [Raytrace] Greetings from Mike
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All 'good stuff' but we just announced the list and we hope you will have
to repeat this in a few days because others will have joined. ;-)

Some people do their email from work or don't check it as often as others. 
So everyone, hold on a bit.  Give others a chance to join before we get
into the heart of the issue.

Ken

----- Original Message -----
From: Michael D. Crawford <crawford@goingware.com>
Sent: Sunday, December 02, 2001 7:16:01 PM
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Subject: [Raytrace] Greetings from Mike




From jd-upton@texas.net Mon Dec  3 10:50:04 2001
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Joseph,

At 04:37 PM 12/2/01 -0800, Joseph Goins wrote:
>Here's a first one for the archives.  What software is recommended for 
>raytracing?

     That is an excellent starter question for the list.  It gives us a 
chance to list some of the ray trace resources that are available to ATMs.

     All the programs listed below are available free of charge.  Several 
are scaled back (limited) versions of professional optical design and 
evaluation programs.  The "big brothers" of these programs can cost 
thousands of dollars (US).  The companies that produce them have made these 
free versions available to amateurs and students like us.

     There are a number of other low cost and free ray tracing programs 
available.  Most will do basic ray tracing and spot diagram generation.  I 
do not mean to slight the usefulness of those programs by not listing them 
here.  This list simply consists of the "heavy duty" programs that I have 
at least heard something about.

     For this mail list to achieve its goal of sharing knowledge of these 
programs, we need folks who have used them to actively participate.  I have 
played with OSLO-LT, but have only scratched the surface of what it can 
do.  I expect to learn as much as anyone else on this list.

     Our goal is to generate a set of tutorials and FAQ concerning how to 
use ray tracing programs to answer the types of questions that come up on 
the ATM list from time to time.  The ray tracing FAQ will ultimately reside 
on the ATM_Site web site.  I wrote up one such tutorial for my web site 
last year.
<http://www.atm-workshop.com/dall-setup.html>
Hopefully, this list will inspire other step-by-step tutorials to be 
written for the ATM_Site.  So feel free to ask questions about how to do 
some specific tasks in these ray tracing programs and we will see if the 
group can figure out how to do it.  We will all learn something in the 
process and common questions and procedures will go into the FAQ for future 
use.

     Here is the list of free programs.  I have included the known 
limitations of each as best I know them.  The links will take you to the 
respective companies' web sites where you can download the program.

OSLO-LT (Limited to 10 surfaces)
http://www.sinopt.com/

ZEMAX (Demo only -- Cannot save?? How is it limited??)
http://www.focus-software.com/demo_z.html

MODAS (Limited to 4 surfaces)
http://ivankra.tripod.com/modas.html

ATMOS (Limited to 3 surfaces)
http://web.tiscali.it/ATMOS/

SYNOPSYS (Full featured for 90 days -- Limited to 12 surfaces thereafter)
http://home.gwi.net/OSD/home.htm

Roadrunner LT (Limited to 12 surfaces)
http://www.acmeoptics.com/



John D. Upton
Georgetown, TX
<http://www.atm-workshop.com/>      "The ATM's Workshop Page"
<http://members.aol.com/RonWin20/>  "Ronchi For Windows Software Page"


From klowther@cisnet.com Mon Dec  3 14:35:35 2001
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We have been slowly increasing in number.  Up to 22, less than 24 hours
after anouncing.  We have decided to keep the membership list hidden,
even to members, for a little added security.  I believe the mailer
program gives individual the right to hide their email on that list any
how.  The archives are public however and do show email addresses.  If
there is much concern, we can close the archives to the public, though I
hate to do that.  I get email addresses from the ATM archive from time
to time. ;-)

My provider has good spam filters in place and I hardly ever get
spammed, so it doesn't bother me.  I have posted to the ATM list
hundreds of times.


-- 
Ken Lowther
Youngstown, Ohio
http://www.atmsite.org
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From trickar1@san.rr.com Mon Dec  3 22:41:59 2001
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From: "Tim Rickard" <trickar1@san.rr.com>
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Hello. Thanks Ken for setting up this list.  I look forward to contributing
what I can, though mostly I'll be learning from others for now.

cheers,
Tim


From bolenb@pacbell.net Tue Dec  4 11:04:34 2001
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Subject: [Raytrace] Virus in Email
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Mr. Smith's emails contain virus's.  Be careful.  Don't open them.

Joe


From chen@stars.gsfc.nasa.gov Wed Dec  5 13:43:41 2001
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Subject: [Raytrace] Hi everybody
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Hi folks:

	 Just signed up on this list to see what is going on.  Apparently not much 
activity as yet.   So I thought I'd introduce myself and my area of interest.

	I work on the development of lightweight mirrors.   The details are in a 
web site which unfortunately is not publicly accessible at the moment due 
to NASA concerns about security.   The web site is in the process of being 
relocated to another address where the world can access it.

	 My interest is to design new telescopes around the lightweight 
mirrors.  Hence ray tracing.  I have done a fair amount of  work using 
Beam3, Beam4, and TDesign (Rutten and van Venrooij).   I have played around 
with OSLO LT,  I also have a copy of the latest MODAS and Zemax 10.0.   I'm 
still learning to use those.

	Most of the mirrors we have produced so far are spherical, although we 
just made our first parabola a short while ago.   My current interest is 
therefore to check out existing published designs of spherical mirror 
telescopes (mostly from S&T) and see which ones are the most cost-effective 
to build.  By cost-effective I mean the least number of optical components 
(lenses, secondary and tertiary mirrors, etc), components that are easy to 
make, and where the tolerancing is not too exact.  Not having had any 
formal education in optical design, I'm sort of feeling my way around.

	I look forward to hearing what other members of this group are engaged in.

Regards,
P.C. Chen           


From jd-upton@texas.net Thu Dec  6 17:41:32 2001
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List Members,

     Welcome.

     As background material, I am posting excerpts from some of the 
off-line email conversations that lead to the generation of this list.  My 
cuts of non-pertinent material are denoted by "[snip]".

     Ken Lowther was the driving force behind getting the list started.  I 
didn't find out about being appointed list administrator until after the 
list was created.  Thanks Ken.  (...I think...)  To repay the honor(?), my 
first duty was to make Ken alternate administrator. :^)

= = = = = = = = = = = = = = = = = = = = = = = = = = =

At 12:55 PM 11/27/01 -0500, Ken Lowther wrote on the ATM List:
>Please consider 'donating' your spec files to the atm site so that others 
>can use them for reference.  Having these files could be a useful starting 
>point for some of us that are less adept at these programs.


At 07:57 AM 11/28/01 -0600, John D. Upton wrote off-list:
>     I don't mind sending you the OSLO file I used, but I don't think it 
> would be of use to anyone.  There are already several OSLO and ZEMAX 
> files on the ATM Site.  They represent unusual or sometimes "complex" 
> designs that may be of use to others.  A file describing a single 
> paraboloidal mirror for a Newtonian seems of little use to me.
>
>     What *is* needed is a set of tutorials for each of OSLO, ZEMAX and 
> MODAS that explain how folks can get the information that was discussed 
> in this thread on the ATM List.  The useful data is not in the file -- it 
> is in which buttons you push (and commands you use) to try to get some 
> insight into the problem at hand.  [snip]


At 05:15 PM 11/28/01 -0500, Ken Lowther wrote off-list:
>[snip] When W=B put out the book on lens design with computers I bought it 
>and downloaded OSLO.  It was a very frustrating experience.  I put a lot 
>of time into it with very little in the way of results.  Maybe start with 
>the Newtonian and see how it goes?  If you want to collaborate I can set 
>up a quick email group.  I'm sure we could get a few people from the list 
>to offer input.  [snip]


At 04:56 PM 11/29/01 -0500, Ken Lowther wrote off-list:
>I could set up a list and see who is interested in learning a little OSLO 
>and seeing if we could turn the most common questions and problems into a 
>FAQ or tutorial.  If it works fine.  If there isn't enough interest, you 
>have saved yourself a lot of work. ;-)


At 06:32 PM 11/29/01 +1000, Peter John Smith wrote off-list:
>I have found the level of help provided with Raytracing software as 
>pathetic and I fully relate to Ken's comments.
>
>This includes Zemax.  [snip]  The instructions do tersely cover features 
>but one needs much more because one needs to understand how to use the 
>program before the terse comments make any sense............
>
>I eventually taught myself to use Zemax (well - a useful portion of its 
>features.  Doubt anyone could understand all) by using some demo files 
>which came with it and a real menagerie of mainly old optics books.  [snip]
>
>In my opinion you need
>
>1/  example files of a large range of types of optical instruments.  This 
>is especially true when the ray path inverts and rays pass some surfaces 
>more than once.
>
>2/  some optical background.  Preferably a lot.  But the ironic thing is 
>that a lot of good work can be done with a good modern optimising 
>raytracer with limited optics theory.
>
>3/  more specific info on the ways modern raytracers have 
>developed.  There is almost a set of jargon relating to them.  It is not 
>in the books to my knowledge and is probably best overcome by good tutorials.
>
>I found the most useful technique to work outwards from example 
>files.  Then substitute other specs for other example designs available to 
>me by modifying these files.  The two best books for this I had which gave 
>enough examples and some assessment of them were 'Telescope Optics - 
>Evaluation and Design' by Rutten and VenRooij and Warren J  Smith's 
>'Modern Lens Design - A Resource Manual'.  Also published designs in S&T 
>over the years often gave some assessment as well as specs and were 
>generally correct.  Smith's book is mainly a collection of Patent Specs 
>and some others.  It is not on modern design methods.  But it includes 
>examples of most types of optics designs WITH A SHORT RUNDOWN ON THEIR 
>ASSESSMENT which is really valuable. There is also an introduction to the 
>book which matched a lot of what I wanted to know.  It is not aimed at any 
>one raytracer which is a both a limitation and a strength.  Being general 
>sounds like a good idea but it is amazing how slight variations in the way 
>each raytracer presents and accepts info is such a block to a newcomer.
>
>The least useful books were on raytracing theory.
>
>One real trap was that many designs I had collected were simply wrong or 
>afflicted with typos.  When one has no confidence to recognize this it has 
>a huge negative impact.  You would be amazed at how many prescriptions are 
>bandied around that are simply wrong.
>
>Unfortunately I cannot see a way to solve this problem easily because -
>
>1/  Most top line raytracers with a nice user interface with any 
>reputation are expensive and need a dongle to run.  Thus there is little 
>point in their files being made readily available.  Vary few 'free' 
>programs include optimisation in a simple enough interface for it to be 
>useable.  With all of its limitations, OSLO still stands out here as being 
>useful. [snip]
>
>2/  Files for one program are not readily available to to others.  Despite 
>the fact that some will 'import' others files, I have found this of very 
>limited use.  As raytracers grow in sophistication features are added. 
>Unless everyones import features are all updated these now become 
>unreadable to many other programs.  This is the reason I have not placed 
>more files in the ATM space.  I have had many requests from people for 
>help because they could not import my files and have lately taken more 
>to   ------.txt   files of prescriptions for intercommunication. This is 
>pathetic but it always works.  Of course the recipient must have enough 
>experience to use them. One product I think should be more well known is 
>OPTIX which will translate raytracing file formats reasonably.  The writer 
>has a good simple product and seems to intend extending the freeware LT 
>version to a fully optimising program which will then cost a significant 
>amount.  It is a little like a Zemax lookalike. But, realistically, is 
>there room for another professional raytrace on the market. At the moment 
>the LT version is useful as a file viewer with some assessment capability 
>but unless kept up to date as other programs evolve will lose its usefulness.
>
>At one time I thought of placing files for every design on my web site in 
>the ATM space and am willing to do this  (partly done) but is it 
>worthwhile in Zemax format ? .  Every one of my web articles contains a 
>txt prescription.
>
>[snip]
>
>As a matter of interest, on the Zemax web site there are many files for 
>download.
>
>To download go to: http://www.focus-software.com/file_exchange/
>
>Many of these are of weird setups - things that would take you ages to 
>figure out how to set up in the lens editor.  In fact, some are people 
>showing off their expertise I think.  But many could be the basis for 
>other work.  One set of these files corresponds for all the examples in 
>Wilson's books on reflective telescope optics.  Maybe we should have links 
>to any sites like this in the ATM space..
>
>You can also download a demo version of Zemax which contains many many 
>useful examples.
>
>I think a few more 'Tutorials' like that done by John Upton may be useful 
>but that requires a huge amount of work.  [snip]  And all this work may 
>become void with changes  in the user interface or file structure of the 
>raytracing software.
>
>Articles on any design could include some discussion of evaluation 
>techniques and the evolution of the design.
>
>As a matter of interest, I have not started a new Zemax file in years.  I 
>always modify an existing file of something similar.  Has its good and bad 
>points.  Is very easy but sometimes contains an obscure artifact that 
>becomes a problem.  But it is a powerful approach which suits my lazy 
>inclination.

= = = = = = = = = = = = = = = = = = = = = = = = = = =

John D. Upton
Georgetown, TX
<http://www.atm-workshop.com/>     "The ATM's Workshop"
<http://members.aol.com/RonWin20/> "Ronchi For Windows Home Page"


From jd-upton@texas.net Thu Dec  6 17:46:49 2001
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List,

     Our membership seems to be pretty stable now at about 35.  Let's get 
going.

     Where do you want to get started on this list?  I don't know exactly 
what level of knowledge already exists, so I am unsure.  What do you want 
to discuss?  One possible starting point is to discuss things common to all 
ray-tracing programs -- or whether there is anything in common.

     For starters, do all programs use the same conventions for data entry?

     OSLO uses a "spreadsheet" format.  If you draw out a design on paper 
with light starting from the left, the following rules apply.  Are these 
basic rules the same for all other programs we might be interested in using?

1.  Each surface encountered by the light is numbered in the order that the 
incident light transverses it.  If the light is reflected back onto a 
previous surface, it is numbered again, but the parameters can be picked up 
from the original specification.

2.  If light is travelling left to right, distances are positive.  If right 
to left, they are negative.  At each reflection, the sign of the directions 
changes.  (For example; if light is going left to right, the sign of 
distances is positive.  If that light is reflected, the next distance is 
negative.  If it is again reflected, the sign changes back to positive.)

3.  Each surface has a radius of curvature, aperture, thickness, and media 
associated with it.  Surfaces may also have special data such as conic 
constant associated with them.  The thickness and media are understood to 
be where the light is entering upon traversing the surface.

4.  For a curved surface, if the center of curvature is to the right of the 
surface, the ROC is a positive number.  If the COC is to the left of the 
surface, the ROC is a negative number.

5.  Each surface has a thickness associated with it.  The thickness is 
simply the distance to the next sequential surface.  Lenses have a 
thickness to them, of course.  Air spaces are also considered "thicknesses".

    Are these basic rules the same in all programs?  They seem to be 
consistent with all the optics and ray-tracing texts I have read.  What 
other "rules" might be considered common to most if not all programs?

John D. Upton
Georgetown, TX
<http://www.atm-workshop.com/>     "The ATM's Workshop"
<http://members.aol.com/RonWin20/> "Ronchi For Windows Home Page"


From wchurchill2nh@hotmail.com Thu Dec  6 19:44:26 2001
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From: "Wayne Churchill" <wchurchill2nh@hotmail.com>
To: raytrace@blackhole.idcomm.com
Subject: Re: [Raytrace] Where To Start?
Date: Thu, 06 Dec 2001 21:44:04 -0500
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Hi John, Hello List Members,
A question concerning surfaces:
When considering optically flat reflecting surfaces, how is a change in the 
angle of the direction of the light cone usually denoted?
And thickness:
When considering the thickness of a lens, is the on axis thickness of the 
center of the lens the thickness value used?
For those of us who haven't kept up or brushed up on optical terminologies, 
should we develope a short list of common optical terms and meanings so 
we're able to communicate effectively?
Thankyou,
Wayne Churchill


>From: "John D. Upton" <jd-upton@texas.net>
>To: raytrace@blackhole.idcomm.com
>Subject: [Raytrace] Where To Start?
>Date: Thu, 06 Dec 2001 18:46:13 -0600
>
>List,
>
>     Our membership seems to be pretty stable now at about 35.  Let's get
>going.
>
>     Where do you want to get started on this list?  I don't know exactly
>what level of knowledge already exists, so I am unsure.  What do you want
>to discuss?  One possible starting point is to discuss things common to all
>ray-tracing programs -- or whether there is anything in common.
>
>     For starters, do all programs use the same conventions for data entry?
>
>     OSLO uses a "spreadsheet" format.  If you draw out a design on paper
>with light starting from the left, the following rules apply.  Are these
>basic rules the same for all other programs we might be interested in 
>using?
>
>1.  Each surface encountered by the light is numbered in the order that the
>incident light transverses it.  If the light is reflected back onto a
>previous surface, it is numbered again, but the parameters can be picked up
>from the original specification.
>
>2.  If light is travelling left to right, distances are positive.  If right
>to left, they are negative.  At each reflection, the sign of the directions
>changes.  (For example; if light is going left to right, the sign of
>distances is positive.  If that light is reflected, the next distance is
>negative.  If it is again reflected, the sign changes back to positive.)
>
>3.  Each surface has a radius of curvature, aperture, thickness, and media
>associated with it.  Surfaces may also have special data such as conic
>constant associated with them.  The thickness and media are understood to
>be where the light is entering upon traversing the surface.
>
>4.  For a curved surface, if the center of curvature is to the right of the
>surface, the ROC is a positive number.  If the COC is to the left of the
>surface, the ROC is a negative number.
>
>5.  Each surface has a thickness associated with it.  The thickness is
>simply the distance to the next sequential surface.  Lenses have a
>thickness to them, of course.  Air spaces are also considered 
>"thicknesses".
>
>    Are these basic rules the same in all programs?  They seem to be
>consistent with all the optics and ray-tracing texts I have read.  What
>other "rules" might be considered common to most if not all programs?
>
>John D. Upton
>Georgetown, TX
><http://www.atm-workshop.com/>     "The ATM's Workshop"
><http://members.aol.com/RonWin20/> "Ronchi For Windows Home Page"
>
>_______________________________________________
>Raytrace mailing list
>Raytrace@blackhole.idcomm.com
>http://www.atmsite.org/mailman/listinfo/raytrace


_________________________________________________________________
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From klowther@cisnet.com Thu Dec  6 19:50:17 2001
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"John D. Upton" wrote:
> 
> 
>      Where do you want to get started on this list?  I don't know exactly
> what level of knowledge already exists, so I am unsure.  What do you want
> to discuss?  One possible starting point is to discuss things common to all
> ray-tracing programs -- or whether there is anything in common.

For many of us, a simple file to look at in a program might help.  Maybe
pick a program and look at the file and do simple modifications.  A
simple lens might be a good starting place.  Followed by a reflector. 
Figuring out how/why to set up the original paramaters isn't intuitive
as I recall.



-- 
Ken Lowther
Youngstown, Ohio
http://www.atmsite.org
http://www.atmsite.org/mailman/listinfo/atmswap

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"John D. Upton" wrote:
> 

> 
>      Ken Lowther was the driving force behind getting the list started.

Hey, 5 minutes of my time.  In the following messages, it was clear that
John really wanted to help bring amatures up a level.  I simply did a 5
minute exploit of that. ;-)

> I didn't find out about being appointed list administrator until after the
> list was created.  Thanks Ken.  (...I think...)  

Aren't surprises nice. :)  The software allows for multiple admins if
things get hectic we could 'saddle' Peter with night shift.  Depending
on your perspective.





-- 
Ken Lowther
Youngstown, Ohio
http://www.atmsite.org
http://www.atmsite.org/mailman/listinfo/atmswap

From klowther@cisnet.com Thu Dec  6 20:05:28 2001
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Wayne Churchill wrote:
> 
> Hi John, Hello List Members,
> A question concerning surfaces:
> When considering optically flat reflecting surfaces, how is a change in the
> angle of the direction of the light cone usually denoted?
> And thickness:
> When considering the thickness of a lens, is the on axis thickness of the
> center of the lens the thickness value used?
> For those of us who haven't kept up or brushed up on optical terminologies,
> should we develope a short list of common optical terms and meanings so
> we're able to communicate effectively?
> Thankyou,
> Wayne Churchill
> 

I haven't played with the software for a while now, but I believe you
use center thickness on a lens and the software takes care of the
curve.  When last I used OSLO LT. it did come with a few sample files. 
Like I said in my last post, even making simple changes to them wasn't
intuitive.  I would suggest you down load the software and take a look
at the sample files.  I'm sure there is one in there for a lens.


-- 
Ken Lowther
Youngstown, Ohio
http://www.atmsite.org
http://www.atmsite.org/mailman/listinfo/atmswap

From klowther@cisnet.com Thu Dec  6 20:18:25 2001
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There were a couple of noteworthy posts early one.  Not much in the
archives so you may want to check them out.  Michael Crawford introduced
him self along with his credentials early on.  Peter Chen did the same a
few days ago.  I'd recommend you check out those posts if you weren't on
the list yet.

Since one of the purposes of this list is to knock out a FAQ/tutorial,
any of you that fancy your selves as scribes or are proficient at web
content, please keep an eye towards helping with this aspect.  John says
OSLO maintains a mailing list.  No activity as of yet.  We may ask them
to peek in on us.

http://www.atmsite.org/pipermail/raytrace/2001-December/subject.html
-- 
Ken Lowther
Youngstown, Ohio
http://www.atmsite.org
http://www.atmsite.org/mailman/listinfo/atmswap

From jd-upton@texas.net Thu Dec  6 23:17:49 2001
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Wayne,

At 09:44 PM 12/6/2001 -0500, Wayne Churchill wrote:
>A question concerning surfaces:
>When considering optically flat reflecting surfaces, how is a change in 
>the angle of the direction of the light cone usually denoted?

     If the reflecting surface is on axis, you only need to change the 
direction by changing the sign.  If the reflecting surface is at an angle 
to the ray direction, you have to set up the surface tilted to the 
angle.  I have only used that mode once and would have to play with OSLO a 
bit to duplicate the setup.

>When considering the thickness of a lens, is the on axis thickness of the 
>center of the lens the thickness value used?

     Yes, the center axial thickness of a lens is used.  The programs 
figure out everything else.

>For those of us who haven't kept up or brushed up on optical 
>terminologies, should we develope a short list of common optical terms and 
>meanings so we're able to communicate effectively?

     Yes, a great suggestion.  Do we have a volunteer to put together the 
Ray-Tracer dictionary?


John D. Upton
Georgetown, TX
<http://www.atm-workshop.com/>     "The ATM's Workshop"
<http://members.aol.com/RonWin20/> "Ronchi For Windows Home Page"


From jd-upton@texas.net Thu Dec  6 23:18:20 2001
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Ken,

At 09:51 PM 12/6/2001 -0500, Ken Lowther wrote:
>For many of us, a simple file to look at in a program might help.  Maybe
>pick a program and look at the file and do simple modifications.  A
>simple lens might be a good starting place.  Followed by a reflector.

     Perhaps a couple of text prescriptions from OSLO will help illustrate 
the (typical?) data entry formats.

     This is the text printout of an OSLO design for a simple double convex 
lens made of Schott BK7 glass.

*LENS DATA
Simple Double Convex Lens
  SRF      RADIUS      THICKNESS   APERTURE RADIUS       GLASS  SPE
  OBJ       --        1.0000e+20    1.0000e+14             AIR
  AST    10.000000      0.250000      1.000000 AS          BK7 C
   2    -20.000000     12.826432 S    0.991482 S           AIR
  IMS       --            --        1.2937e-05 S

     The lines labeled AST and 2 describe the lens.  (The AST just means 
that the aperture stop for the lens is at the first surface.)  Remember 
that it takes two lines (surfaces) to fully describe a lens.  The left side 
has a ROC of 10.0" and the right side 20.0"  Note that the right side's 
curvature is negative since it is convex and the COC must be to the left of 
the surface.  The thickness of the lens is shown on the AST line.  It is 
0.25" thick.  The thickness shown on line 2 is the "thickness of the air 
between the right surface of the lens and the image plane -- in other words 
the focal length is 12.826".

     Now, here is an example for a concave spherical mirror with a ROC of 30".

*LENS DATA
Simple Spherical Mirror
  SRF      RADIUS      THICKNESS   APERTURE RADIUS       GLASS  SPE
  OBJ       --        1.0000e+20    1.0000e+14             AIR
  AST   -30.000000    -15.000000 S    3.000000 AS   REFL_HATCH
  IMS       --            --        1.5000e-05 S

     In this case, the AST line shows the mirror.  The ROC is negative 
since the COC is to the left of the mirror's surface.  The thickness is 
again the focal length or the thickness of air between the mirror's surface 
and the image plane.  The focal length is negative because the light has 
reflected off the mirror and is now travelling right to left.

     Do these two examples help illustrate the rules or conventions in the 
previous note?


John D. Upton
Georgetown, TX
<http://www.atm-workshop.com/>     "The ATM's Workshop"
<http://members.aol.com/RonWin20/> "Ronchi For Windows Home Page"


From aboskov@pop.wiredcity.com.au Fri Dec  7 07:26:45 2001
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Hi,

Well Peter got the ball rolling so I thought I'd add my bit.

I've got OSLO LT and a few other design packages but the problem I'm having 
is finding decent tutorials that show you how to use this software. Any 
documentation that come with these packages seem to be written in a way 
that assumes the user is a full bottle on the subject.

So if anyone knows any great tutorials or web sites could you please share 
them.


Cheers Alex


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A while back I tried this using John Upton's OSLO-LT file for setting up the
Dahl null test.  I eventually got to the point where I could use the program
and and run through the procedure to do the setup.  And I think I could even
interpret the results correctly.  (I _think_!)

But even at the end of all that I still felt like the monkey who
accidentally manages to type the Ecyclopedia Brittanica.  Something I still
don't really understand is the conceptual basis of it all.  For example, in
the Dahl null test, what are the detailed concepts involved?  What are we
trying to optimize?  What are the meanings of the terms used, such as "error
at the wavefront", "error at the surface", and so on.

I think a discussion of the conceptual framework would be very helpful,
together with a discussion of how raytracing in general helps us set up and
solve optical problems.

BTW, somewhere I have a spreadsheet that I set up that is based on John's
tutorial on the Dahl null test.  It's a detailed description of the
procedure using OSLO-LT.  If others are interested I can make it available.
I don't have a web site so I can't post it myself.

- Ken Bertapelle

> -----Original Message-----
> From: raytrace-admin@blackhole.idcomm.com
> [mailto:raytrace-admin@blackhole.idcomm.com]On Behalf Of Hermit
> Sent: Thursday, December 06, 2001 7:51 PM
> Cc: raytrace@blackhole.idcomm.com
> Subject: Re: [Raytrace] Where To Start?
>
>
> "John D. Upton" wrote:
> >
> >
> >      Where do you want to get started on this list?  I don't
> know exactly
> > what level of knowledge already exists, so I am unsure.  What
> do you want
> > to discuss?  One possible starting point is to discuss things
> common to all
> > ray-tracing programs -- or whether there is anything in common.
>
> For many of us, a simple file to look at in a program might help.  Maybe
> pick a program and look at the file and do simple modifications.  A
> simple lens might be a good starting place.  Followed by a reflector.
> Figuring out how/why to set up the original paramaters isn't intuitive
> as I recall.
>
>
>
> --
> Ken Lowther
> Youngstown, Ohio
> http://www.atmsite.org
> http://www.atmsite.org/mailman/listinfo/atmswap
> _______________________________________________
> Raytrace mailing list
> Raytrace@blackhole.idcomm.com
> http://www.atmsite.org/mailman/listinfo/raytrace
>


From mpeck1@ix.netcom.com Fri Dec  7 09:47:19 2001
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At 18:46 12/6/2001 -0600, John D. Upton wrote:

>     For starters, do all programs use the same conventions for data entry?
>
>     OSLO uses a "spreadsheet" format.  If you draw out a design on paper 
> with light starting from the left, the following rules apply.  Are these 
> basic rules the same for all other programs we might be interested in using?

I don't *know* the answer to this, but I think professional level design 
programs are generally consistent in surface numbering and sign conventions 
as long as you stick to centered systems. I don't think that's necessarily 
the case with some of the atm oriented software out there. There seem to be 
no generally accepted standards for specifying tilts & rotations. 
Documenting differences among programs that atm's are likely to use might 
be a worthwhile FAQ item.

>Perhaps a couple of text prescriptions from OSLO will help illustrate the 
>(typical?) data entry formats.
>This is the text printout of an OSLO design for a simple double convex 
>lens made of Schott BK7 glass.

I'd like to make a modest administrative suggestion here. OSLO .len files 
are just text files, and they're usually quite short. Embedding the 
complete file in your posts separated from the text by asterisks or 
something won't waste a lot of bandwidth -- interested readers can cut, 
paste, and save using notepad or any other text editor.

I'd also suggest - if the site owner and list administrators are willing - 
maintaining a file upload/download area for list members (maybe the public 
too). I think Peter Smith is right that the best way to learn this stuff is 
to play around with existing designs. I learned what little I know by 
entering published designs from any source I could find into OSLO, and 
gradually learned new capabilities of the program by trying to extend and 
optimize existing designs. I've never gotten beyond capabilities that can 
be accessed with spreadsheet entries, menu selections, or taskbar clicks, 
but you can do quite a lot without ever mastering the programming language 
that's part of OSLO.

Somewhere on atmsite there are a couple dozen OSLO files that I uploaded a 
year or so ago. Most of them were entered directly from R&vanV or other 
published designs. A few months ago Steve Fejes sent me some optimized, 
flat field APO designs that he built starting from an unoptimized 3 element 
design that I had swiped from some source (I've forgotten where). If 
Steve's on the list maybe he can explain how he got from my simple APO to 
his optimized field corrected version. He really did an amazing design job.

The last bit of advice I'd offer is obvious to anyone who's done any kind 
of design work on a computer. Save files often. If your design goes 
hopelessly astray just give up and go back to your last working layout. 
OSLO LT seems to be pretty stable (at least version 5.4 was), and I've 
rarely crashed it just by doing stupid lens design tricks. I don't think 
I've ever caused my machine to crash with OSLO.

Mike Peck

_________________

Michael Peck
email mpeck1@ix.netcom.com
Wildlife photography page http://home.netcom.com/~mpeck1/index.html
Amateur telescope making http://home.netcom.com/~mpeck1/astro/astro.html


From jd-upton@texas.net Fri Dec  7 10:44:29 2001
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Mike,

At 10:44 AM 12/7/2001 -0600, Michael Peck wrote:
>no generally accepted standards for specifying tilts & rotations. 
>Documenting differences among programs that atm's are likely to use might 
>be a worthwhile FAQ item.

     Yes, I agree.  That is exactly the type of information the FAQ should 
contain.  It also leads into the next point you raised.

>I'd like to make a modest administrative suggestion here. OSLO .len files 
>are just text files, and they're usually quite short. Embedding the 
>complete file in your posts separated from the text by asterisks or 
>something won't waste a

     I can include the full OSLO file for future examples.  There are two 
problems I see with this, however.  The first is that there have been 
changes in file format as OSLO has evolved.  I have both Version 5.4 and 
Version 6.1 installed on my system.  I use 6.1 for some things and 5.4 for 
others.  The reason I keep the older version around is that it supported 12 
surfaces while the new version supports only 10.  I have an on-going design 
project that needs 11 surfaces.

     The second problem is that I was attempting to keep this list 
generalized to all ray-tracers and not overly advocate a specific 
one.  That is why I posted the text form of the design file descriptions to 
the list rather than the files themselves.  The text prescriptions are 
somewhat portable from one program to another (I think) and contain all the 
information about a design in more or less human readable format.  Peter 
John Smith has raised the same concern about ZEMAX files.

     As you pointed out above, the FAQ should reflect how to do things in 
the most common programs.  I didn't want to "standardize" this list on 
OSLO.  Some members are already quite capable with other programs and may 
not want to learn OSLO.  They have much general ray-tracing knowledge to 
share and I don't want them to not participate because we are all using a 
program they are not familiar with.  Standardization here becomes two-edged 
sword.

     What say you, List?  Can we do both effectively?  Perhaps we could use 
OSLO for most of the concept examples (showing the text of the saved design 
files -- *not* file attachments) and have the users of other programs point 
out differences in how to do common tasks as we go along.  I am willing to 
do whatever the list wants in this regard.

>I'd also suggest - if the site owner and list administrators are willing - 
>maintaining a file upload/download area for list members (maybe the public 
>too). I think Peter Smith is right that the best way to learn this stuff is

     Ken is the person to address this.  I think he already has some means 
of accepting file donations for posting on the ATM Site.  Maybe we just 
need a separate page to list the design files with a short description of 
the contents.

>astray just give up and go back to your last working layout. OSLO LT seems 
>to be pretty stable (at least version 5.4 was), and I've rarely crashed it 
>just

     I agree that OSLO is pretty stable.  Version 5.4 is very stable for me 
on Windows 95, 98, and Me.  Version 6.1 has given me some problems on 
Windows Me, but I've learned to work around them.  As you say, they have 
never crashed hard enough to damage any system files.


John D. Upton
Georgetown, TX
<http://www.atm-workshop.com/>     "The ATM's Workshop"
<http://members.aol.com/RonWin20/> "Ronchi For Windows Home Page"


From chen@stars.gsfc.nasa.gov Fri Dec  7 11:24:23 2001
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<html>
Hi:<br>
<x-tab>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;</x-tab>Just like
to express my thanks to John Upton for his post on raytrace
origins.&nbsp; The post included a message from Peter John Smith which
contained a pointer to the site
<a href="http://www.focussoftware.com/file_exchange/" eudora="autourl"><font color="#0000FF"><u>http://www.focussoftware.com/file_exchange/<br>
</a></font></u>which I did not know about.<br>
<br>
<x-tab>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;</x-tab>I went to
the site and downloaded the files for the Shafer telescope and Dan
Schroeder's  (author of Astronomical Optics) files.&nbsp; Dan's files
contained, as PJ Smith mentioned, examples of four mirror telescope
designs by RN Wilson.&nbsp;&nbsp; These are exactly the examples I was
looking for.<br>
&nbsp;<br>
<x-tab>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;</x-tab>For those
interested, the designs by RN Wilson are for the next generation of
extremely large (20-100m) ground telescopes.&nbsp; Telescope mirrors this
big cannot be made in one piece (for economical and practical
reasons).&nbsp; Hence they must be made of many segments.&nbsp;&nbsp; For
reasons of affordability and manufacturability, it is best to make all
the mirror segments identical.&nbsp; Hence the segments are all spherical
(spheres and flats are the only possible geometrical figures), resulting
in a giant spherical primary mirror.<br>
<br>
<x-tab>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;</x-tab>The
problem with a spherical primary mirror is that, unlike a parabola, it
does not focus parallel rays from infinity to a point.&nbsp; Therefore a
minimum of three mirrors are required to make a telescope that has good
resolution and an acceptable field of view.&nbsp; Three mirrors, however,
end up sending the light back towards the front of the scope.&nbsp;
That's why four is used in Wilson's design.&nbsp; Having an extra mirror
also permits some optimization, I'm told.<br>
<br>
<x-tab>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;</x-tab>I loaded
the sample files into Zemax and looked at the 3d layout.&nbsp; They look
good.&nbsp; I need to learn more Zemax and raytracing to understand the
details.&nbsp;&nbsp; But thanks to this list, it has saved me a lot of
effort (as I have done in the past) trying to measure the diagrams with a
ruler and infer the optical parameters from the original published
articles.<br>
<br>
Regards,<br>
P.C. Chen<br>
</html>


From chen@stars.gsfc.nasa.gov Fri Dec  7 11:45:38 2001
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Hi:

	Thought to tell the list of another project I'm interested in, although 
I'm not sure how well it will work out.   David Lewis has written an 
excellent program called PLOP which is available from his site 
http://www.eecg.toronto.edu/~lewis/.   PLOP computes the optical surface 
shape of a telescope under various support schemes (3 points, 9 points, 
multiple rings, etc).  It is an excellent program and very user friendly.

	I thought it might be interesting to do raytracing for mirror under a 
variety of support schemes.  This is called 'active optics'.  It is 
especially applicable to large thin mirrors (a la Mel Bartels?).   Acitve 
support is the technique used by the European Southern Observatory in its 
four 8 meter Very Large Telescopes, currently the biggest in the 
world.  The mirrors are thin and therefore very sensitive to how they are 
supported.  In fact, the VLT supports are cleverly designed to compensate 
for astigmatism, spherical aberrations, and coma.

	I wrote to David Lewis some time ago, and he kindly modified a PLOP 
program to output mirror shapes in Zernike terms.  I'm trying to see if  it 
is possible to use the PLOP generated Zernike terms and import them into 
Zemax (or other programs) and do a raytrace.  The ultimate aim, of course, 
is to be able to adjust the support forces on a mirror to keep it at 
optimal shape during observations.
	Wish me luck.  I'll try to keep the list informed of my progress.

P.C. Chen


From klowther@cisnet.com Fri Dec  7 15:30:49 2001
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Michael Peck wrote:
> 
> I'd also suggest - if the site owner and list administrators are willing -
> maintaining a file upload/download area for list members (maybe the public
> too). 

I'll look into it when I have a chance.

-- 
Ken Lowther
Youngstown, Ohio
http://www.atmsite.org
http://www.atmsite.org/mailman/listinfo/atmswap

From klowther@cisnet.com Fri Dec  7 16:27:46 2001
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Peter and all.  The mail program is set so that replys go to the
original poster.    This is 'protection' from accidently sending a
private email to the group.  On my mailer, I must hit 'reply to all' if
I am using the header from another post instead of starting 'fresh'.

Ken


-------- Original Message --------
Subject: [Raytrace] Spherical mirror telescopes
   Date: Fri, 07 Dec 2001 12:36:58 -0500
   From: Peter Chen <chen@stars.gsfc.nasa.gov>
     To: <mailto:@poph-f.gsfc.nasa.gov>

Hi:
Just like to express my thanks to John Upton for his post on raytrace
origins.  The post included a message from Peter John Smith which
contained a pointer to the site
http://www.focussoftware.com/file_exchange/
which I did not know about.

I went to the site and downloaded the files for the Shafer telescope and
Dan Schroeder's (author of Astronomical Optics) files.  Dan's files
contained, as PJ Smith mentioned, examples of four mirror telescope
designs by RN Wilson.   These are exactly the examples I was looking
for.

For those interested, the designs by RN Wilson are for the next
generation of extremely large (20-100m) ground telescopes.  Telescope
mirrors this big cannot be made in one piece (for economical and
practical reasons).  Hence they must be made of many segments.   For
reasons of affordability and manufacturability, it is best to make all
the mirror segments identical.  Hence the segments are all spherical
(spheres and flats are the only possible geometrical figures), resulting
in a giant spherical primary mirror.

The problem with a spherical primary mirror is that, unlike a parabola,
it does not focus parallel rays from infinity to a point.  Therefore a
minimum of three mirrors are required to make a telescope that has good
resolution and an acceptable field of view.  Three mirrors, however, end
up sending the light back towards the front of the scope.  That's why
four is used in Wilson's design.  Having an extra mirror also permits
some optimization, I'm told.

I loaded the sample files into Zemax and looked at the 3d layout.  They
look good.  I need to learn more Zemax and raytracing to understand the
details.   But thanks to this list, it has saved me a lot of effort (as
I have done in the past) trying to measure the diagrams with a ruler and
infer the optical parameters from the original published articles.

Regards,
P.C. Chen
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-------- Original Message --------
Subject: [Raytrace] Raytracing mirror support distortions (active
optics)
Date: Fri, 07 Dec 2001 12:58:08 -0500
From: Peter Chen <chen@stars.gsfc.nasa.gov>
To: <mailto:@poph-f.gsfc.nasa.gov>

Hi:

	Thought to tell the list of another project I'm interested in, although 
I'm not sure how well it will work out.   David Lewis has written an 
excellent program called PLOP which is available from his site 
http://www.eecg.toronto.edu/~lewis/.   PLOP computes the optical surface 
shape of a telescope under various support schemes (3 points, 9 points, 
multiple rings, etc).  It is an excellent program and very user
friendly.

	I thought it might be interesting to do raytracing for mirror under a 
variety of support schemes.  This is called 'active optics'.  It is 
especially applicable to large thin mirrors (a la Mel Bartels?).  
Acitve 
support is the technique used by the European Southern Observatory in
its 
four 8 meter Very Large Telescopes, currently the biggest in the 
world.  The mirrors are thin and therefore very sensitive to how they
are 
supported.  In fact, the VLT supports are cleverly designed to
compensate 
for astigmatism, spherical aberrations, and coma.

	I wrote to David Lewis some time ago, and he kindly modified a PLOP 
program to output mirror shapes in Zernike terms.  I'm trying to see if 
it 
is possible to use the PLOP generated Zernike terms and import them into 
Zemax (or other programs) and do a raytrace.  The ultimate aim, of
course, 
is to be able to adjust the support forces on a mirror to keep it at 
optimal shape during observations.
	Wish me luck.  I'll try to keep the list informed of my progress.

P.C. Chen

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> 
> -------- Original Message --------
> Subject: [Raytrace] Spherical mirror telescopes
>    Date: Fri, 07 Dec 2001 12:36:58 -0500
>    From: Peter Chen <chen@stars.gsfc.nasa.gov>
>      To: <mailto:@poph-f.gsfc.nasa.gov>
> 
>   But thanks to this list, it has saved me a lot of effort (as
> I have done in the past) trying to measure the diagrams with a ruler and
> infer the optical parameters from the original published articles.
> 
> Regards,
> P.C. Chen

It is nice to know that there are results already.  At least for
someone. ;-)

-- 
Ken Lowther
Youngstown, Ohio
http://www.atmsite.org
http://www.atmsite.org/mailman/listinfo/atmswap

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>      What say you, List?  Can we do both effectively?

My two cents: For now, we could standardize on OSLO LT, or some other
program
if it is generally preferred, to make things more manageable.  As Ken
suggested, we could start with a simple Newtonian, since presumably all of
us are generally familiar with it.  The goal would be to make sure everyone
has the software and the newt. file working, and to begin exploring how to
do various analyses (e.g. wavefront, vingetting effects of various aperture
stops, spot diagrams, etc). Then a central obstruction could be modeled, and
the MTF analyzed. Then perhaps a simple refractor or a mak-newt., etc. I
have in mind an integrated tutorial and Q&A that could become an FAQ. Over
time there could be several FAQs on different, more advanced topics. The
conceptual stuff is also crucial of course.  For newbies like myself,
however, getting a simple program running and exploring the program's
analysis tools would help to frame the problems concretely while providing a
quick success to maintain motivation...

Of course, threads for discussing other programs and advanced topics would
presumably go on in parallel...

Tim










From mayen1@mwt.net Sat Dec  8 06:42:14 2001
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I like this idea.

And if we actually work out a step by step an actually constructable scope. all
the better.  Like One i have been thinking of,,(he he he)  but yet have been
able to figure out how to get it into the $#%&!#* programs. he he he.

It starts out as a simple 10" f- 6  Newtonian.

Joe

Tim Rickard wrote:

> >      What say you, List?  Can we do both effectively?
>
> My two cents: For now, we could standardize on OSLO LT, or some other
> program
> if it is generally preferred, to make things more manageable.  As Ken
> suggested, we could start with a simple Newtonian, since presumably all of
> us are generally familiar with it.  The goal would be to make sure everyone
> has the software and the newt. file working, and to begin exploring how to
> do various analyses (e.g. wavefront, vingetting effects of various aperture
> stops, spot diagrams, etc). Then a central obstruction could be modeled, and
> the MTF analyzed. Then perhaps a simple refractor or a mak-newt., etc. I
> have in mind an integrated tutorial and Q&A that could become an FAQ. Over
> time there could be several FAQs on different, more advanced topics. The
> conceptual stuff is also crucial of course.  For newbies like myself,
> however, getting a simple program running and exploring the program's
> analysis tools would help to frame the problems concretely while providing a
> quick success to maintain motivation...
>
> Of course, threads for discussing other programs and advanced topics would
> presumably go on in parallel...
>
> Tim
>
> _______________________________________________
> Raytrace mailing list
> Raytrace@blackhole.idcomm.com
> http://www.atmsite.org/mailman/listinfo/raytrace


From bobmay@nethere.com Sat Dec  8 17:06:03 2001
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>>I don't *know* the answer to this, but I think professional level design
programs are generally consistent in surface numbering and sign conventions
as long as you stick to centered systems.
>>
Unfortunately, there are differences between the programs as to the
direction of things.  I'm not familiar with them but have seen notes to that
effect on the SCI.OPTICS newsgroup.  This is because each and every person
that figured out how to do raytracing way back when thought up their
standard directions and the rest of the community has never gotten around to
stating that a particular set of directions is the right way.
I hope this gets to the right path.
Bob May
http://nav.to/bobmay
bobmay@nethere.com
NEW! http://bobmay.astronomy.net



From jd-upton@texas.net Sat Dec  8 18:40:56 2001
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Tim, Joe,

     This sounds okay to me.  We don't seem to have had any takers yet, so 
here is my attempt to start this process.

At 08:28 PM 12/7/2001 -0800, Tim Rickard wrote:
> >      What say you, List?  Can we do both effectively?
>
>My two cents: For now, we could standardize on OSLO LT, or some other
>program
>if it is generally preferred, to make things more manageable.  As Ken
>suggested, we could start with a simple Newtonian, since presumably all of
>us are generally familiar with it.  The goal would be to make sure everyone
>has the software and the newt. file working, and to begin exploring how to
>do various analyses (e.g. wavefront, vingetting effects of various aperture
>stops, spot diagrams, etc). Then a central obstruction could be modeled, and


At 07:43 AM 12/8/2001 -0600, Joe Mayenschein wrote:
>I like this idea.
>
>And if we actually work out a step by step an actually constructable 
>scope. all
>the better.  Like One i have been thinking of,,(he he he)  but yet have been
>able to figure out how to get it into the $#%&!#* programs. he he he.
>
>It starts out as a simple 10" f- 6  Newtonian.

     Here is the text prescription for the 10" F/6 Newtonian.  The full 
text of the OSLO-LT file appears at the bottom of this post.  Cut the text 
between the lines and paste it into a file named "newt_10_F6.len" to 
reconstruct your own copy.

*LENS DATA
10" F/6.0 Newtonian
  SRF      RADIUS      THICKNESS   APERTURE RADIUS       GLASS  SPE  NOTE
  OBJ       --        1.0000e+20    1.0000e+14             AIR
  AST  -120.000000    -60.000000 S    5.000000 AS   REFL_HATCH   *
  IMS       --            --        6.0000e-05 S

     You can also just follow the steps below to create this file 
yourself.  I am using OSLO-LT version 6.1 for this example.

1.  Open OSLO-LT.

2.  Select File | New Lens...

3.  For the file name type newt_10_F6.len

4.  For number of surfaces, enter 1.  The mirror is the only optical 
surface in this example.

5.  Select OK.  The "Surface Data" window will open.  Note that there are 
three lines and multiple columns in the "spreadsheet".  The first is 
labeled OBJ for object, the second is labeled AST for aperture stop, and 
the third is labeled IMS for image surface.  Since there is only one 
optical surface in this example, that is where the aperture stop must be 
placed.  If there were multiple surfaces, the aperture stop could appear on 
any one of them and the others would have a number in the SRF label 
column.  The surface numbers would be in listed in the order that light 
strikes them.

6.  In the "Surface Data" Window, select the Gen button.

7.  In the "General Conditions" Window, select the Units button and set to 
inches.

8.  In the "Lens:" field, enter a name for the design.  I am using '10" 
F/6.0 Newtonian' for my name.  (This is actually a description of the 
design, not a file name, so it can be almost anything you want.  If you 
want, you can enter even more notes by pressing the "Notes" button and 
entering your extra data.)

9.  Click on the green check mark in the upper left corner.  This always 
accepts the data and can be used to close the window.

10. In the "Surface Data" window, click in the "Ent beam radius" 
field.  Enter the value of the entrance beam radius.  This will be the 
radius of the mirror for this example.  Enter 5.0 or you can use the built 
in formula capability by typing 10.0/2.0 (or 10/2).  Press the enter key or 
click on green check mark.  (If you happen to click twice, the "Surface 
Data" window will close.  Open it again by selecting Lens | Update lens data...

11. Click in the RADIUS field of the AST line.  Enter the radius of 
curvature of the mirror.  Remember the data entry conventions presented in 
an earlier post.  Since light starts out moving left to right, the concave 
mirror will have its center of curvature to the left of the mirror 
itself.  This means that the ROC must be entered as a negative 
number.  Again, I will just use the formula capability to enter the ROC of 
the 10" F/6 mirror.  I type -10*6*2 and press enter.

12. Now I have to tell OSLO that this surface is a mirror.  I select the 
button in the GLASS column of line AST and choose Reflect (hatch).  We now 
have a spherical mirror described in the spreadsheet. Save this 
intermediate result by selecting File | Save.

13. To tell OSLO this is a paraboloidal mirror for a Newtonian, we need to 
specify its conic constant.  Click on the button in the SPECIAL column of 
the AST line.  Select Polynomial Asphere | Conic / Tonic.  In the "Conic / 
Tonic Data" window, enter -1.0 in the Conic constant entry field.  Close 
the Conic / Tonic window by clicking the green check mark.

14. Finally, let's let OSLO find the focal length of the mirror for 
us.  Click on the button in the THICKNESS column of the AST line.  Select 
the Solves | Axial ray height... item.  In the "Axial Ray Height" box that 
pops up, enter 0 and select OK.  We just told OSLO we wanted it to find the 
place where the ray has an axial height of 0 -- in other words where is 
crosses the optical axis.  That marks the paraxial focal point.

     We are done.  Save the file.  You now should have a file that is the 
same as what I have appended in text form below.  If you select the "Len" 
button in the OSLO "TW 1" text window, it should print the same human 
readable lens prescription that I included at the top of this note.  Study 
its format.  It actually contains almost all of the data pertaining to this 
design.  The only thing missing is the conic constant for the mirror.  That 
can be included also by clicking the Spe button in the "TW 1" text window. 
The contents of this window may be copied and pasted into any text 
application -- like this post.

Cut this and paste into a new notepad file named "newt_10_F6.len".

===CUT BELOW THIS LINE===========================
// OSLO 6.1 41540     0     0
LEN NEW "10\" F/6.0 Newtonian" -60 2
EBR  5.0
ANG  0.0000572957795
DES  "OSLO"
UNI  25.4
// SRF 0
AIR
TH   1.0e+20
AP  9.9999999995e+13
NXT  // SRF 1
RFH
RD   -120.0
PY   0.0
CC   -1.0
NXT  // SRF 2
AIR
WV 0.58756 0.48613 0.65627
WW 1.0 1.0 1.0
END  2
===CUT ABOVE THIS LINE===========================

     Let me know if I have messed up this description.  Doing a "tutorial" 
like this real time, I often don't recognize mistakes since it is still too 
fresh in my mind.


John D. Upton
Georgetown, TX
<http://www.atm-workshop.com/>     "The ATM's Workshop"
<http://members.aol.com/RonWin20/> "Ronchi For Windows Home Page"


From dchaffee@blitz-it.net Sun Dec  9 01:12:02 2001
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From: "Dan Chaffee" <dchaffee@blitz-it.net>
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Subject: Re: [Raytrace] Where To Start?
Date: Sun, 9 Dec 2001 02:15:29 -0600
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>I'd also suggest - if the site owner and list administrators are willing -
maintaining a file upload/download area for list members (maybe the public
too). I think Peter Smith is right that the best way to learn this stuff is
to play around with existing designs. I learned what little I know by
entering published designs from any source I could find into OSLO, and
gradually learned new capabilities of the program by trying to extend and
optimize existing designs. I've never gotten beyond capabilities that can
be accessed with spreadsheet entries, menu selections, or taskbar clicks,
but you can do quite a lot without ever mastering the programming language
>that's part of OSLO.

Mike, All,

This really sums it up for my experience as well. I've manipulated radii and
glass types from the simple achromat example you sent me a year ago
and learned how to balance enough of the factors to design a decent
176mm f/18(!) BK7-F2 oiled doublet. I wanted to KISS and keep all
surfaces spherical since I don't have a reference flat big enough for a
double bypass knife edge test. Within the simple parameters of the ray
analysis, wavefront evaluation, spot diagrams, and PSF, I've allegedly
got a design that should be well color corrected, very low LA on axis
in 546nm, and coma no worse than a longish newtonian. Actually, I
also arrived at a Fraunhofer of the variant same f/#  that is clearly better
with off axis performance, but I wanted the advantages of the oiled R2&3
for better transmission and reduction of scatter. The advice on designing
lenses in R&V is good and spells out  the proccess of trial and error
for balancing achromatism with acceptable OSC very well.

Here are the specs for the oiled doublet:
R1=1490mm
R2=-1373
R3=-1373
R4=-14900
T1=17mm
T2=16mm
Glass 1 is BK7 with Nd=1.51678,Vd=64.15
Glass 2 is F2 with Nd=1.619; Vd-36.34

und der Fraunhofer:
R1=2004mm
R2=-1106
Air gap= 3.6
R3=-1116
R4=-4330
T1=18
T2=15
Same glasses

If anyone wants, I'll email the actual OSLOlt lens files.
I had Roger C. run my design through Zemax and he seemed to feel it
would be a good performer. I'd welcome anyone elses comments if they
are interested.
At any rate, the grinding is 98% complete, so I'll know shortly whether
or not this will perform to my liking. One possible problem is in the melt
data from the glass broker, which gave an odd rationality of dispersion.,
but was within the range of what is acceptable per the written guarantee,
so I couldn't return it. The sales rep I complained to made the mistake of
telling me he sold glass to Roland Christian. Naturally, I contacted Roland
about the specs and this broker in particular. He advised me to ignore the
supplied melt data, since glass brokers rarely have equiptment accurate
enough to read indicies and dispersions to justify values under .01. At best
their values can only ahow a general trend in higher or lower indicies
resulting
from the fine & precision annealing that they do. He  also said he'd long
since done
business with the broker in question....

Dan Chaffee





From fmilsom@lineone.net Sun Dec  9 07:24:01 2001
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Hi All,

Perhaps a good place to start, especially for those with no background =
in tracing optical systems is for someone who perhaps has the =
experience, to give some details of more popular (free?) downloadable =
programs and their url's. That way those without the programs can get up =
to speed more easily and contribute to the list in a more understandable =
way.

Francis

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<DIV><FONT face=3DArial size=3D2>Hi All,</FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>Perhaps a good place to start, =
especially for those=20
with no background&nbsp;in tracing optical systems is for someone who =
perhaps=20
has the experience, to give some details of&nbsp;more =
popular&nbsp;(free?)=20
downloadable programs and their url's. That way those without the =
programs can=20
get up to speed more easily and contribute to the list in a more =
understandable=20
way.</FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>Francis</FONT></DIV></BODY></HTML>

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From mayen1@mwt.net Sun Dec  9 08:12:54 2001
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Date: Sun, 09 Dec 2001 09:13:52 -0600
From: Joe Mayenschein <mayen1@mwt.net>
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Hi All,

I just made or at yahoo groups a place we can store files, images, plans,
whatever.  a somewhat crude archive for files etc.

It is usually used as a message board e-mail reflector type of thing.. but it
has a lot of more features also like the file data storage feature.  we can
stuff 20 meg's of files there for free.

The front door to the area is,,

http://groups.yahoo.com/group/learn_to_raytrace

I'm putting in the 10" f-6  oslo file in there as soon as i'm done with this
message.

let me know if you guys like the storage idea?

Joe

P.S.  On yahoo,, i'm fuzzydog1   ,,,   don't ask.. he he


From klowther@cisnet.com Sun Dec  9 08:34:11 2001
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Joe Mayenschein wrote:

I personaly have given up on Yahoo.  Our club has a list there.  I sent
my final message to it yesterday.  It never showed up.  Maybe because I
refuse to sign up with Yahoo?  You cannot access the files and archives
unless you open an account with Yahoo.  The list owner can directly
subscribe someone to a mailing list but all of the options are closed to
them.

Yahoo's taking over egroups is the main reason I learned how to install
and configure the Mailman software. ;-)  Since the files are text base,
it shouldn't be a big deal for people to save them as files in a
directory on their hard disks.

-- 
Ken Lowther
Youngstown, Ohio
http://www.atmsite.org
http://www.atmsite.org/mailman/listinfo/atmswap

From mayen1@mwt.net Sun Dec  9 08:58:29 2001
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From: Joe Mayenschein <mayen1@mwt.net>
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If you haven't noticed or read their messages  Yahoo is killing all the "Clubs"
they are moving to the "Groups" format and names.  You need to change your
"Club" over to a "Group"  I am the member of over 50 "Groups" and all work
fine.  It's the clubs that are erratic and not working at all if any ,, anymore.

Joe

Hermit wrote:

> Joe Mayenschein wrote:
>
> I personaly have given up on Yahoo.  Our club has a list there.  I sent
> my final message to it yesterday.  It never showed up.  Maybe because I
> refuse to sign up with Yahoo? 