In another thread @jcwu88 posted two links by Roland Christen (Astro Physics):
Notes on Star Testing Refractors
Star Testing Complex Optical Systems
I just purchased my first spotting scope and have never attempted a star test so, this is all new to me.
Therefore I would really appreciate everyone’s comments on the following (copied from the second link above):
“In my experience, when an optic measures 1/10 wave AT THE DESIGN
WAVELENGTH, then the performance will be nothing short of stunning.
Peter's criterion was a bit less at 1/8 wave P-V. Either way, the
customer will have an excellent optic.
By the way, Ceravolo is my mentor on testing of optics. Even though I
have been making optics for a long time, without his guidance in the
testing lab, I never would accomplished what I did. And yes, I used
to use the star test in the distant past when I made longer
refractors. Some of my optics came out good and have surprised me
when retested on the interferometer. But for the fast F6 and F7
triplets I make now, the star test falls short.
The dilemma for manufacturers then is, should we do our best to
produce smooth high contrast optics, or should we please the star
test crowd and do some hand aspherizing to get a more pleasing
out-of-focus star image? I can tell you that it is easy to do some
rough compensation with quick local polishing at several zones to get
more equal inside and outside star patterns, but the result will
almost certainly be a loss of contrast. Add to that a nice big
central obstruction to get rid of the offending inner zones, and
presto! you have a nice "fast food" Mak-Cass that doesn't work any
better than a typical SCT.
In our case, we will do our utmost to produce the closest faximile to
the star patterns in Suiter's book, but they will never be exactly
equal. The overriding concern will be that the optic has a very
smooth and accurate wavefront to produce the highest contrast
possible in the final image, which I assume will be in focus.
Roland Christen ASTRO-PHYSICS”
Thanks,
Randy
Notes on Star Testing Refractors
Star Testing Complex Optical Systems
I just purchased my first spotting scope and have never attempted a star test so, this is all new to me.
Therefore I would really appreciate everyone’s comments on the following (copied from the second link above):
“In my experience, when an optic measures 1/10 wave AT THE DESIGN
WAVELENGTH, then the performance will be nothing short of stunning.
Peter's criterion was a bit less at 1/8 wave P-V. Either way, the
customer will have an excellent optic.
By the way, Ceravolo is my mentor on testing of optics. Even though I
have been making optics for a long time, without his guidance in the
testing lab, I never would accomplished what I did. And yes, I used
to use the star test in the distant past when I made longer
refractors. Some of my optics came out good and have surprised me
when retested on the interferometer. But for the fast F6 and F7
triplets I make now, the star test falls short.
The dilemma for manufacturers then is, should we do our best to
produce smooth high contrast optics, or should we please the star
test crowd and do some hand aspherizing to get a more pleasing
out-of-focus star image? I can tell you that it is easy to do some
rough compensation with quick local polishing at several zones to get
more equal inside and outside star patterns, but the result will
almost certainly be a loss of contrast. Add to that a nice big
central obstruction to get rid of the offending inner zones, and
presto! you have a nice "fast food" Mak-Cass that doesn't work any
better than a typical SCT.
In our case, we will do our utmost to produce the closest faximile to
the star patterns in Suiter's book, but they will never be exactly
equal. The overriding concern will be that the optic has a very
smooth and accurate wavefront to produce the highest contrast
possible in the final image, which I assume will be in focus.
Roland Christen ASTRO-PHYSICS”
Thanks,
Randy