Bill Burk
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Will this information allow me to take better photographs?
You already take better photographs.
Will this information allow me to take better photographs?
I’m very curious about this effective film speed. Is there any evidence to support it? Did Phil Davis just make it up?
Phil Davis just keyed 0.1 density above B+F to ASA speeds. Despite the fact that I strongly disparage following this moving speed point, I mark my own graphs with the moving 0.1 above base+fog points and label them with the corresponding EI.
It’s easy and illustrates how much that point moves with development changes.
But when I choose an exposure index of my own, I use Delta-X speeds for the planned development time.
That’s when I am shooting for excellent negatives. (like when I have a tripod).
As anyone else would do, I bend the speed a bit when shooting handheld in difficult lighting.
I’m very curious about this effective film speed. Is there any evidence to support it? Did Phil Davis just make it up?
Then, individual curve EI values are obtained for the Zone System N-number series (N-2, N-1, N, N+1, N+2).
My confusion stems from this sentence. What is the method to determine your EI used to create the graph of EI vs (anything).
ic-racer said:My confusion stems from this sentence. What is the method to determine your EI used to create the graph of EI vs (anything).
As I was reading Way Beyond Monochrome again, I couldn't help but wonder about their proposed method of film testing involving photographing a step tablet on a light table with a macro lens or suitable bellows extension. It is a departure from a standard way of exposing film for sensitometric analysis by means of a sensitometer. One of the factors that varies across these two methods is the presence of flare. This made me think of the Jones and Condit (1941) paper.
It reminded me of the distinction that Jones and Condit make ( Loyd A. Jones and H. R. Condit, "The Brightness Scale of Exterior Scenes and the Computation of Correct Photographic Exposure*," J. Opt. Soc. Am. 31, 651-678 (1941)) between "negative material" (henceforth curve 1) and a "particular negative" (henceforth curve 2). They made it very clear that "If for any purpose it is desired to determine the magnitude of a negative density difference, delta Dn, corresponding to some object brightness difference, delta log Bo, curve 2 must be used. Thus, in dealing with tone reproduction problems which involve a consideration of gradients, curve 2 gives the desired information."
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In that particular paper, the authors referred to the object as "Bo" or "brightness scale of the object" but, the term "object luminance" was also used, particularly, in later work. Curve 2 is derived by incorporating a flare factor, which is defined as the ratio of the brightness scale of the object to the illumination scale of the
image. In the classic tone reproduction theory, the more common representation of flare light is as a plot of log subject luminance to log image luminance, but in the paper above, we have both scene and image luminance plotted against negative density, i.e., a characteristic curve. This can be somewhat confusing, but I am just going to leave it at that, as, otherwise, I'd need to write a few paragraphs, and, besides, most of you already know this stuff really well.
What I do want to focus on is the fact that the proposed method for deriving curve 2 is rather involved. First of all, you need to know the actual brightness scale of the object, including the exact minimum and maximum values, which are related to the minimum and maximum negative densities related to that scene. You also need to, separately, expose a step tablet in a sensitometer, i.e., without flare, and plot it using the actual, rather than relative, exposure values. To derive curve 2, you also need to construct a separate log Bo scale (along the top of the plot in Fig. 4), and then measure displacement calculated from the brightness and flare information. It can be done, but it's rather tedious.
An alternative approach is to use the notion of flare light as "flare density," as suggested by Dorst ( Paul W. Dorst, "A Novel Graphical System for Representing Tone Reproduction Data," J. Opt. Soc. Am. 34, 597-600 (1944)) and others. The advantage of this approach is that you do not need to know the object brightness scale before the value of image density corresponding to any intermediate value of object density can be computed. In other words, it is possible to construct curve 2, without the complicated method proposed by Jones and Condit. You can even do it without knowing actual exposure values, by just using a relative LogE scale. That way, we can simulate a characteristic curve of the "particular negative" and compare it to the curve of the "negative material" rather simply. In my attempt to implement these two methods computationally, I obtained very similar results. They are not identical, and you can, of course, criticize the "flare density" model as not being "correct" but this might be a compromise that is worth making, particularly for the sake of simplicity. The chief distinction is that the "curve density" method is more of a simulation, whereas the "curve factor" method obtains actual measurements of parameters related to the negative in question. Since Jones and Condit tried to produce a large body of empirical data of actual scenes and actual negatives and prints, they, obviously, had to use the flare factor approach.
I synthesized a curve 1 (blue) to be similar to that in Fig. 4 above to make the comparison easier. I then used a flare ratio algorithm to derive curve 2 (red) and a flare density model to derive another curve 2 (green). Because the flare ratio method uses separation, the resulting curve 2 (red) becomes asymptotic past the point representing an object of zero brightness. The flare density curve 2, on the other hand, extends only as far as curve 1.
My point is not to argue that one model is better than the other. I am simply trying to find the simplest, but still reasonably accurate, method of deriving curve 2 for the purpose of analyzing gradients and simulating the mapping of negative density onto object brightness. I am curious to see what you guys think of these methods and how they compare. I am also curious to hear whether this type of analysis (i.e., curve 1 vs curve 2) is useful for ordinary film testing?
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Great questions! Here's my understanding of the concept. Maybe others will chime in to make it a more complete description.Again, without knowing how an EI is determined, I'm only guessing, but I suspect a disconnect between the empiric data from "panel of viewers" and "best print." Or I guess the question is "what is the connection?"
I do know that Delta-X connects 0.1log D to 0.3G via Delta-D and the parabola below. But what is the connection between this Exposure Index and 0.3G?
So, to conclude, one can choose from a number of different methods of determining their personal EI (or effective speed), including the fractional gradient method. It's a matter of personal choice. Film manufacturers, however, usually use the current ISO standard.
The statistical psychophysical evaluation or print speed represents the most accurate method of determining film speed. Jones and Nelson compared the results obtained using various sensitometric methods to the print speeds as described in "A Study of Various Sensitometric Criteria of Negative Film Speeds." Obviously the psychophysical method would be "much too complicated and laborious to permit of its application in practice and that for such a purpose it is desirable or, in fact, imperative to find a sensitometric method which will yield results in close agreement with those obtained by the direct psychophysical method." It was concluded the fractional gradient method agreed most closely to the print speeds over the greatest number of films and situations. The Delta-X Criterion is the modern equivalent. It uses the same concept of the shadow gradient in determining the minimum useful exposure point and not density (a point that Jones greatly emphasized). The method has stood the test of time and why it is part of the current ISO standard.
One could say there is only one film speed and that is the speed at the fractional gradient point. Everything else is EI. In JOSA 1943, American Standard Method for Determining Photographic Speed and Speed Number, makes a distinction between "speed", meaning the fractional gradient speed, 1 / E, and "Speed Number", which is Speed / 4. Speed was "not intended for use with ordinary exposure meters or exposure calculators. The speed number was used as the published film speed. I believe they later became ASA Speed and ASA Film Exposure Index. While the published film speeds to be used in conjunction with an exposure meter aren't the actual speed determined at the fractional gradient speed point, they are tethered to the only method that has a legitimate connection to the subjective evaluation of quality. All other methods of film speed determination don't have that relationship and are compromised. My feeling is why go to the trouble of testing just to use an inferior method.
This is a very ingenious method. Thank you for suggesting it. I have read about the black box with a hole, but not about the top hat. It should work even better than the box, especially if it's made of matte black felt, or similar fabric.I’d carry a top hat out with me and set it on its side in a scene. Take a close-up meter reading from inside the hat and base the exposure on that reading, placing it at the lowest shadow value you can think of.
You ‘know’ the inside of the hat should have ‘no’ net density in the resulting negative except that because of actual flare there will be some density.
Plot that resulting density reading of the inside of the hat on the finished negative… on the curve from that film/development combination.
The displacement on the x-axis from where you placed it … to where it landed… defines the flare.
Convert the data points of the Log E scale of the graph to arithmetic numbers. Convert the difference (difference in Log E from where you placed the exposure to where density fell) to an arithmetic number and add this number to every exposure number and convert them back to Log.
Then find the density above each Log E result and plot that density above the original data point Log E position.
You’ll get the second curve from this exercise.
Having said that, I cannot help but also be impressed by photographers creating amazing art by using methods that, from the point of view of theory, seem haphazard, at best. People develop film in coffee and beer, digitize film with a DSLR, and still get great results. On the other hand, I test my materials as meticulously as I am able, and still end up with a roll of badly exposed frames from time to time. I just wasted two hours and three sheets of expensive paper trying to print from a badly exposed negative. I did get a decent print, but nowhere near good or even satisfactory.
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