Lee L said:Yesterday I looked up the information I have on TMY in two astrophotography books for a friend here on APUG. They give Schwarzschild factors of 0.80 and 0.81 for TMY, both derived from the same test method. I'll not go into the method here unless you request it, but the method relies on exposure tests.
To use this factor, you plug it into the formula T=(t+1)^(1/p)-1...etc.
Pat,gainer said:The best fit I have found to experimental data for long exposures is:
T = Tm + a * (Tm ^ 1.42)
where Tm is the exposure time read from the light meter's calculator and a is constant for any given film. For TMY or TMX you may use 0.06.
c6h6o3 said:Way too complicated. Just use Kodak's charts. .
That wasn't the only one of my boo-boos. The part that plots as a straight line on log-log paper is the right hand side of:Lee L said:Pat,
I'm just headed out the door, but I wanted to note that you might have a typo here. Isn't the last number 1.62 rather than 1.42? I recall it was the golden mean, Fibonacci ratio, or whatever you want to call 1.618....
Lee
jp80874 said:The problem with just using Kodak's charts is that the Kodak chart ends at a metered exposure of 100 seconds.
gainer said:You still have to be able to correct exposure without changing f-stop. When you change the f-stop, you change the effective measured time. The correction of 2 stops would be unacceptable to the view camera user who sets the f-stop without concern for its effect on exposure, then sets the exposure time to suit the f-stop.
I calculate a corrected exposure time of 5346 seconds when the metered time is 1000 seconds. That is a change from 16.7 minutes to 89.1 minutes. If you open 2 stops, the metered time would drop to 250 seconds. I would calculate the correct exposure time to be 710 seconds, or 11.8 munutes, not 1000 seconds or 16.7 minutes. It would be 1/2 stop overexposed at 1000 seconds. This may or may not be acceptable exposure error, but opening from f/64 to f/32 or from f/32 to f/16 might change the picture quite a bit.
Lee L said:Ka Tai,
I noticed that some of the tables you are using are from Bruce Barnbaum's empirical tests or from Photo Techniques, a magazine that he often writes for. IIRC, Gainer's formula is designed to fit data from Howard Bond, derived empirically and published in Photo Techniques.
The numbers I gave are from empirical tests as well, but show p=0.88 for TMX. These are derived from tests shots of a gray scale with no filter at 1/8 second, then with a 1000x ND filter and exposures of 128 seconds at bracketed f-stops. The Schwarzschild factor is then calculated from the adjustment needed in f-stops to render the gray scale as close to the 1/8 second exposure as possible.
If you don't find that doing exponential equations in your head clears your head and puts you in a receptive, zen-like state, you can always plug the formula I gave (which is a Michael Covington derivation from the standard Schwarzschild formula) into a spreadsheet and work up your own pocket chart that converts metered times to reciprocity corrected times.
There is another long thread on this topic with more information and a number of charts here on APUG. (there was a url link here which no longer exists)
Lee
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