I live in Chicago where skies are Venusian and outdoor observing comes with “occupational hazards”. In other words, Chicago is a good place for indoor testing. I often give GeezerGazer (Ray) a heads-up on my NV testing and he often asks “What about Afocal?” He does mostly NV Prime, but Afocal’s extreme reduction is very compelling.
As they say, “Don’t bury the lead”. This is the lead…learn it, know it, live it
Except for the left photo being in color, these two photos are nearly identical. If you’re using Afocal for image reduction, this is what you want. To use a blackjack analogy, this is a 21. In the next photo you’ll see why this analogy is apropos.
The above image on the left, which I’ll refer to as “visual”, was taken through a 102mm f/7 APO with a TeleVue 55mm Plössl (TV55) converted to 67mm (TV67) and an iPhone 12 Pro Max (1x lens). The photo on the right uses the same setup, but in Afocal with an Envis/Mod-3 connected via TNVC adapter. Unless otherwise noted, NV photos are cropped to size and the camera tint is removed.
The point is that there IS a practical limit to Afocal image reduction and that limit is the “visual” image. This is because of the eyepiece field stop and it’s a hard limit. You can reduce ad infinitum, but you can’t go beyond the field of view allowed by the field stop. Here’s what I mean...
Above is a montage of raw NV images. Left to right is Afocal with: 15mm TeleVue DeLite, TV55, TV67 and an 85mm Plössl by Russell Optics. Top row is with the 102mm f/7 APO, the bottom row is with a 6-inch f/4 Newtonian.
From left to right, images are nicely reduced, as expected. As the image reduces, the true field of view (TFOV) increases to fill the NVD eyepiece’s image circle until we get to the Russell 85. Beyond 67mm, you’re basically busted. The field stop is the reason why.
The TV55 (which also applies to the converted TV67) has a 46mm diameter field stop. For a 2” barrel eyepiece, you can’t get much larger. The Russell 85 doesn’t have a true stop, the barrel itself is the stop. Indeed, Russell’s image is more reduced, but there’s no increase in TFOV. Below are the photos scaled to their image circles.
Above, on the left is the TV67, the right is the Russell 85. Top row 102mm f/7 APO, bottom row 6-inch f/4 Newt. When scaled, we see that the Russell 85 gives basically the same image as the TV67. Without the scaling, the Russell 85 image is just a smaller version of the TV67 image. Just to be clear, the Russell 85 is a nice novelty eyepiece, but not for NV Afocal.
So, what’s the big deal about the 67mm focal length? It’s because of two key ratios: Image Plane Reduction and Optical Reduction. If you’re going for perfection, the two ratios should match. Image Plane Reduction is basically the smaller NVD sensor target size compared to the larger 46mm field stop. The clear aperture of my Mod-3 sensor is 18.24mm dia. This ratio is 0.397 (18.24/46). Optical Reduction is the Envis focal length (26.5mm) divided by the 67mm eyepiece focal length is 0.396 (26.5/67).
0.397 vs. 0.396 is not a coincidence. TeleVue obviously chose 67mm as the focal length for their “67mm Converter” to match the TV55 field stop, NVD aperture and Envis focal length. They left nothing on the table. What puzzles me is how they knew ahead of time to thread their TV55’s to accept this future retrofit. Very clever, NostraNagler!
The icing on the cake is that the TV67 40° apparent field of view is the same as the Envis 40° true field of view. As you probably already know, any eyepiece AFOV over 40° is wasted in Afocal. It’s just spillover outside the NVD sensor.
Let’s put this 0.396 reduction in context. Here’s a comparison...
Left to right is Prime with no reduction, Prime with Ackermann reducer/coma corrector (0.73 reduction) and Afocal with TV67 (0.396 reduction). Top row is with 102mm f/7 APO, bottom row is with 6-inch f/4 Newt. That’s a whole lotta reduction!
Now for the downside...Edge of Field drop-off.
Below are two photos Ray took of the Pelican Nebula (IC 5067 and IC 5070) in Cygnus. Both were taken with his 8-inch f/4 Newt and a 7nm Optolong H-Alpha filter. The one on the left is NV Prime with a 0.73x Ackermann reducer at f/2.9. The one on the right is NV Afocal with the TV67 at f/1.6.
Both are great photos, but the Afocal edge of field drop-off in the right photo is considerable. Whether this is a big deal is a matter of taste. Many don’t care about the edge, so long as the center is good. But Ray takes his edges “neat”.
Could the edge drop-off be due to field curvature? Below is a series of photos with a Lake Michigan breakwater at different locations on field. Top is the f/7 APO, bottom is the f/4 Newt. Both showed minor pincushioning. Both f-ratios show the same magnitude of pincushioning. No problem here.
My contention is that the reason for the drop-off is large exit pupils. Below, both photos are Afocal using the TV67. The gain is turned down to reduce image saturation and better show any drop-off. The left photo is with the 102mm f/7 APO, the right photo is with the 6-inch f/4 Newt.
The f/7 photo on the left has very little drop-off. The f/4 photo on the right has a lot of drop-off, very similar to Ray’s Pelican Nebula photo. Normally, a large exit pupil is a good thing. Indeed NV’s ability to go beyond the 7mm limitation of the human iris is a huge benefit.
The formula for exit pupil size is eyepiece focal length divided by objective f-ratio. With the TV67, the f/7 exit pupil is 9.57mm and the f/4 exit pupil is 16.75mm...a big difference! Keep in mind that an exit pupil is not a focal point. In effect, it’s an image of the objective.
Here’s a ray trace drawing that might help. It depicts the f/4 Newt with the TV67, Envis and Mod-3.
To keep things simple, I represent the TV67 and Envis as single lenses. Pay special attention to the dotted lines because they define the exit pupil. Although Envis is big enough for the full exit pupil, the TV67 eyepiece isn’t.
So, what can be done about the edge of field drop-off? Not much. TeleVue could conceivably design a dedicated 67mm 40° AFOV eyepiece for fast NV Afocal, but it would be big, heavy and very expensive. Also, drop-off isn’t a problem with slower scopes. All things considered, TeleVue’s TV67 is Afocal done right. Nearly everyone who uses it swears by it, and now you know why.
One more thing...Narrowband Filters and Afocal. This is an important topic and probably deserves its own report, but in a nutshell, don’t worry about it. For rear-mounted filters (see my post #69)...
https://www.cloudyni...position/page-3
Small ultra-fast objectives (most notably camera lenses) are the toughest for narrowband filters because of band shift. If you’re using a telescope that’s f/4 or slower, you’re good in Afocal for any barrel-mounted H-Alpha filter down to 3.0nm.
As you’ve seen in the lead photo at the top, the “visual” image is the widest TFOV that your NVD can see. This is regardless of any subsequent Afocal reduction. If you have an f/4 scope running Afocal at f/1.6, you don’t need a special f/2 filter. Light has no memory, so everything that happens after the filter is irrelevant. If your filter is okay “visually”, it’s okay with NV Afocal.