Does the field stop of an eyepiece cause vignetting? Or does the clear aperture of the binoviewer cause vignetting? The answer to both questions is "Yes." It is not a matter of either/or but both/and.
The situation is similar to vignetting in Cats. Does the wide field stop of an eyepiece cause vignetting or does the relatively narrow rear aperture of the Cat cause vignetting? Again, the answer is "Yes." Both/and.
In any case, it is NOT the long focal length of an eyepiece which would cause vignetting in a linear binoviewer. The cause is the width of the field stop of the eyepiece interacting with the clear aperture of the binoviewer.
Mike
Please don't be offended by my input. This is not meant as an attack or challenge.
The eyepiece field stop never vignettes the image. The field stop of an eyepiece is at the focal plane. Vignetting only occurs if there is a restriction (almost always circular where telescopes are involved), somewhere between the focal plane and the eyepiece field stop. Since the field stop is at the point where the image is formed, then it simply opaques 100% of the light reaching the focal plane that does not fall into the diameter of the field stop.
The rear aperture of the binoviewer does vignette the image very slightly but because the rear aperture is so close to the focal plane, the opaquing can be a major factor. You likely would not see the opaquing using a 27mm field stop in a 26mm aperture bionviewer, but you can see it using a 27mnm field stop in a smaller prism binocular. Opaquing is identified to occur when the you drift a bright star to the edge of the field and it winks out before you get to the field stop. If it dims before it get to the field stop, that is vignetting. If it disappears before it gets to the field stop, that is opaquing, and it would almost always be caused by the rear aperture of a binoviewer, though when using the widest field eyepieces possible in a C8 or smaller SCT or MCT, you might see some opaquing at the very extreme edge of the field. In the C8, this will happen just before the field stop of a 41mm Panoptic or a 55mm Plossl. If you don't know what to look for, you would never notice it but the true field will be about the same as when using an eyepiece with a field stop about 3mm smaller.
In fact, the primary reason for the field stop of a telescope is to block you from seeing the out of focus inside diameter of the end of the eyepiece barrel.
The primary source of vignetting in the SCT is the front of the baffle, not the rear. The rear baffle is there to opaque the outside of the field so no off axis light that gets through the space between the outside edge of the secondary baffle and the inside edge of the front baffle. In theory, you could make the baffle a cone shape with the larger end of the cone at the back of the scope and this would make the field wider, but the field would still be vignetted by the front of the baffle.
Here is the illumination profile of a C8 type SCT. Notice that the illumination falls off outside of about an 8mm image circle. As you go further off axis, the illumination falls smoothly. This would be the case even if the rear baffle were larger but if the illumination were allowed to fall off much more than 70%, it would not be for imaging with anything other than small sensors.
The sudden downward break in the downward curve is when the rear baffle starts to opaque (completely block) the off axis rays entering the opposite side of the front of the baffle. If you were to make this larger, you would extend the gentle vignetting, but now, if you looked at an angle between the edge of the rear port through the primary baffle, you would see that you could see past the secondary baffle, and that means light could fall on to the focal plane. You could remedy that by making the secondary baffle larger, further shading the primary and lowering contrast, but the field illumination would continue to fall off until the now larger rear port once again opaqued the the front baffle opening. So, the front of the baffle vignettes, and the rear of the baffle opaques any angler larger than the angle between the outside edge of the secondary baffle and the inside edge of the primary baffle, but it does not vignette the system. That is the front of the baffle that does that. You could make the rear baffle as as large as you desire, but the fully illuminated circle size and the illumination falloff would still be the same. The only difference would be where the sharp break in the attached graph shows. Yes, the field would be wider, but once again, off axis light would now be able to get to the focal plane.
The rear baffle of the SCT then is not really causing the illumination falloff It is really there to opaque the field at the point that the designer believed would provide a good compromise between keeping the contrast high and the field illumination at a practical level.
Edited by Eddgie, 20 January 2024 - 02:16 PM.