@Stephen Benskin Thank you for the "What is Normal" article. I have previously implemented flare-adjusted CI from the Kodak table, I also implemented the variable flare-adjusted CI that is consistent, I think, with your paper. Here's a theoretical curve for the KODAK T-MAX P3200 with the LSLR of 2.13. I think you recommend using the value of 2.2. Mine comes from the "standard" seven-stop range that the BTZS system considers normal. It's not a huge difference. The "Aim CI" is flare-adjusted and is estimated at around 0.58, which I also think is consistent with your paper, isn't it?
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I also wanted to ask your opinion on recalculating the film curves to include the effect of flare on negative density. The effect is going to be most pronounced in the shadows, and the correction does change the calculated parameters somewhat. From what I've read, this is not the orthodox way of doing it, but I did it, mainly because of BTZS. It's essentially an implementation of the "flare density" model from Phil Davis' book.
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My print quadrant does incorporate flare. Since the paper tests use the enlarger I plan to print with, I don't contact the step tablet but enlarge it and allow some clear area around the tablet to introduce flare.
Is this what you mean?2.20 is the statistically average luminance range determined by Jones. As with most things, close enough in practice but a problem when you are doing theory. The aim CI for 0.58 is basically Normal. I like to think the most important part of the paper is how to determine the aims for the pluses and minuses. There's the different average flare for different luminance ranges and the desired aims for shorter and longer luminance ranges. There's a table showing the different CIs resulting from the various variables.
Adding flare to the film density comes from the days of hand drawing curves. It's easy to take a French curve to the toe and redrawn the curve to account for flare. My problem with that is it's not how flare works. Flare reduces the luminance range so the shadows fall further to the right on the curve. A flare factor of means the Illuminance range for a
7 stop luminance range is 6 stops at the film plane.
May I recommend the paper testing method proposed by @Nicholas Lindan over at Darkroom Automation.Good idea. When creating paper-curves, I've been contact-printing my tablet, thus adding no flare.
Is this what you mean?
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Yeah, I agree, though I didn't know about the French curve history of it. I have implemented flare adjustment as changing the relationship between subject luminance and image luminance, based on the work of Jones and Condit, Henry, and others. I also used your paper on variable flare, which I found very insightful.
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But the "flare density" model by Phil Davis is mostly about recalibrating the film curve by primarily increasing shadow density, which may result in some increase in what BTZS calls "Subject Brightness Range" and Effective Film Speed. In principle I agree with you, but I also wanted to include the Davis model for photographers who are familiar with it.
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So I went back to my code. I wrote the flare function a long time ago. It turns out, I had implemented the variable flare model and the fixed flare model. I also added the "practical" flare model from your paper. Here's command line output for the "normal" LSLR table and for the KODAK T-MAX P3200 LSLR data, with the flare factor of 0.4. Trying to keep the discussion relevant to the threadI need to take a closer look at your flare table. The general rule is flare increase with an increase of the luminance range and decreases as the luminance range decreases. The average is a 0.10 increase in flare with every 0.30 increase in luminance range over the average 2.20. Here is the comparison table from the paper.
With adjusting the flare to the film curve, one stop flare is basically the density of the curve 0.30 log-H to the right of the shadow exposure. Two stops is the density 0.60 log-H and so on. You can get an impression using (I believe) the curve family from Henry's book.
May I recommend the paper testing method proposed by @Nicholas Lindan over at Darkroom Automation.
I looked over his support files, and saw no article about testing papers. Could you provide the complete URL?
Good idea. When creating paper-curves, I've been contact-printing my tablet, thus adding no flare.
Elsewhere, you mentioned that AA does not compensate for in-camera flare though he uses a camera. I was thinking that an easy way to add such flare would be to photograph a tablet taped to a large 18% gray surface, thus simulating a typical scene of 18% reflectance. That surface would need to extend well beyond the camera's frame because light from outside the frame contributes to flare. Do you think this approach would work? If so, the same approach could be used when enlarging a tablet by placing the strip of paper on an 18% gray card.
Yes, it's kind of buried in a PDF document. It's the manual of the Precision Enlarging Meter. The direct link to the PDF is here. If you don't use staining developers, you can ignore the section of the document dedicated to it. The meter is very good, and economically priced. You can even use it in place of a bench densitometer. The advantage is that you can measure densities of very small areas, even in 35 mm negatives.
You can use any enlarging meter, as long as it's accurate enough for your needs.
You can also download the worksheet for testing paper.
This is awesome! I am going to conclude that we think alikeGot it. Thanks. I see that Nicholas Lindan recommends projecting (not contacting) a wedge onto the paper, which is the method @Stephen Benskin uses in order to accommodate flare.
@aparat, funny you should mention the Precision Enlarging Meter made by DarkroomAutomation.com. I have one. And I've used it for transmission density measures. In fact, I built an attachment for it that turns it into a reflection densitometer. Here's my posting about that, which has some pictures of it:
Accurate Densitometer for $120 with DIY Part
I have two Stouffer strips and four densitometers:
- An old Tobias that became flakey,
- Tobias TCX,
- DarkroomAutomation Precision Enlarging Meter (plus DIY attachment),
- Printalyzer Densitometer
Cool. I am really glad to hear it. I have only rudimentary experience with non-standard developers, so I'll keep an eye out for your posts.I'm thinking of getting back into creating new developers, which will require extensive testing, measuring, and graphing, so this discussion about evaluation of films is important to me.
I couldn't agree more. The Zone System can be very opinionated, even dogmatic, if taken too seriously or literally. It's a method, some might even call it a framework, and it has its uses. I certainly learned from Ansel's books, but there's more to film photography than that.@DREW WILEY , don't get me started about bad terminology! A serious example is "zone". By definition, a zone is an area/region/sector, but AA uses it to refer to a point -- one specific value, as in "I'll place this spotmeter reading on zone III." You can't place a luminance on an area; you place it on a print-value. Better yet, you "render a luminance as a value." "Value" is a better term; Munsell got that right. "Zone system" should be "value system".
Stated simply, Delta 3200 has an exceptionally long toe to its characteristic curve. That allows "something" to be captured way down there in the shadows when shooting higher than ideal speeds for this film, like the marketed speed of 3200, which is over-optimistic but salvageable at least. Using longer development in relation to those faster speeds is necessary to build up decent overall printing density in the negative, as well as a little better shadow tonality separation.
I have a couple of very high quality enlarging meters - one actually a precision easel densitometer, plus a regular densitometer. But I don't bother with any of them when it comes to the common sense observation I just posted above. Gosh, people can sure can overthink and overcomplicate simple problems.
And bringing in an alternate usage of the term "flare" for lens flare itself, or lack of a sun shade, or bellows flare, is a recipe for confusing people. True film flare occurs when there is a lack of an anti-halation coating, a rather rare kind of film.
I would agree with your take on Delta 3200. I have very fond memories, if you can call it that, from using the film. I have a few dozen negatives from around the time my son was born. The grain and tonality make these old pictures look special, at least to me. I also agree that I take film testing too seriously at times. I certainly don't mean to suggest that there's some special value to film testing. It's just a tool, like any other in photography.
And bringing in an alternate usage of the term "flare" for lens flare itself, or lack of a sun shade, or bellows flare, is a recipe for confusing people. True film flare occurs when there is a lack of an anti-halation coating, a rather rare kind of film.
So I went back to my code. I wrote the flare function a long time ago. It turns out, I had implemented the variable flare model and the fixed flare model. I also added the "practical" flare model from your paper. Here's command line output for the "normal" LSLR table and for the KODAK T-MAX P3200 LSLR data, with the flare factor of 0.4. Trying to keep the discussion relevant to the thread
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KODAK T-MAX P3200
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As far as N-numbers are concerned, I have implemented both the BTZS method and a very similar method to what is in your "What is Normal?" paper, with the BTZS being the default option. Please, don't hate me for it.
Yes, I am using a formula for everything. Nothing is hard-coded. I do have a few look-up tables, similar to the Kodak one you just posted, but that's for reference, never for computation.The question is always what most closely conforms to reality. I've seen all of these used at some point and by serious people. Notice how +2 fixed flare is practically the same as +3 variable flare? Both can't be right. Dick Dickerson at Kodak once gave me a sheet with the CIs for different paper grades and different luminance ranges (attached). It uses a fixed density model with 0.40 for flare. Kodak's development data sheets; however, have different aim CIs.. Those CIs more closely fit the variable model, but the data sheets don't use luminance ranges. They use EIs. Pushing for speed works differently than stickily pushing for contrast. In Way Beyond Monochrome, Ralph's developmental model is almost identical to my practical model even though we approached it differently.
So the values are hard wired into the program? What if a condenser enlarger is used or the aim is make Platinum prints? I believe platinum has an LER of 1.60. That would make normal CI 0.88, Are you able to use a formula instead?
Yes, I am using a formula for everything. Nothing is hard-coded. I do have a few look-up tables, similar to the Kodak one you just posted, but that's for reference, never for computation.
Thank you for posting the Kodak table. I will see if I can figure out a statistical model for it. Do you happen to know how they came up with it?
Two different roads leading to the same destination. That is always cool.
Very cool. I have this book and learned a lot from it. It's got a lot of detail, but with clear explanations and beautiful graphics.It is sounding like it's going to be a very effective and versatile tool.
Check the CI for Grade 2 (1.05) and 7 1/3 stops. - CI 0.58. The table is based on the statistical average luminance range of 2.20 and a fixed flare of 0.40. LER / (LSLR - Flare). Here is a table from Photographic Materials and Processes that references the LERs for different paper grades.
It is sounding like it's going to be a very effective and versatile tool.
Check the CI for Grade 2 (1.05) and 7 1/3 stops. - CI 0.58. The table is based on the statistical average luminance range of 2.20 and a fixed flare of 0.40. LER / (LSLR - Flare). Here is a table from Photographic Materials and Processes that references the LERs for different paper grades.
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This brings up something that disturbs me. The LER used to determine grade is
log(exposure(for density 0.9*Dmax)) - log(exposure(for density 0.09)).
My measured Dmax for Ilford RC is 2.10, and Dmax for Foma RC is 1.87. Because Foma's LER uses a lower Dmax, LER itself is lower, even when the straight-line portion of its curve matches that of Ilford. In other words, the grade computed for Foma is too high. Consequently, if you were to print the same image on both Ilford's and Foma's at exactly grade 2 as computed above (which is possible using LEDs and a microcontroller), Foma's print would have lower contrast. In effect, the term 0.9*Dmax lets Foma cheat and claim higher contrast than it actually achieves.
In order for different papers to print at the same contrast (and thus look the same) for the same grade, it seems to me that grade should be based on the slope of the central portion of the paper's HD curve. I see two ways to do this:
I suspect the second way computes the central slope more accurately, but it's more complex.
- Use the LER between the densities of zones VII to III (i.e., densities of 0.19 and 1.61). This solution assumes 1.61 is off the shoulder for all papers. Grade would be determined by LER, as in the past, but the thresholds for grades would change.
- Use the LER between densities Dmin+0.07*DR and Dmax-0.10*DR, where DR = Dmax - Dmin. The constants 0.07 and 0.10 match zones VII and III when Dmax=2.1, but we can use 0.08 or somesuch for both -- I doubt it matters. Grade would be determined by slope and not by LER.
I believe this has not been a problem in the past because most people use tungsten lamps with filters, and as long as Foma yields the same visual contrast as Ilford with the same filters, users are happy. But when we apply the standard definitions to make LER (and thus grade) the same between papers via a microcontroller, the papers don't respond with the same contrast. I think this problem will become more serious as LEDs become more popular.
Your thoughts about this problem?
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