I measures a bunch of commercial Star Diagonals years ago (wavefront, spectral transmission, alignment) and found that only 2/15 were premium performers, 4/15 acceptable performers and the other 9 deficent or unusable.
Tom,
these diagonals sit pretty close to the focal plane, so the relevant light beam diameter that gets combined to a single point at the focal plane is MUCH smaller than the full aperture of the mirror. Does your strehl calculation accunt for that ? Would your measurement pick up such small scale surface deviation in the first place ?
For numbers, these diagonals are localted some 50-60mm from the focal plane. A good scope using such a diagonal is likely around f/7 or slower (mind you, these are not used with newtonians), making the relavant spot on the diagonal just under 8mm diameter. Only the relative surface deviation across any such diameter would matter. Its what primary mirror folks would call "surface roughness". The measurement itself would need to pick up such high order deviations across less than 1/6th of the full aperture to be meaningful.
I only worry about strehl close to the center of that diagonal, the part in use for high power observations. If the diagonal mirrors edge is turned or has zones - say even the full outer half of the diameter, that is only relevant for stars near the field stop in a low power, wide FOV eyepiece. And even the best eyepices are far from being diffraction limited out there, even at f/7.
Edited by triplemon, 19 May 2025 - 01:31 PM.