Do many people apply that extra exposure? To all formats, or just LF? Why would I notice an effect in LF and not in 35 mm?
Thanks,
Tim
Are you compensating for bellows factor? That is the #1 source of exposure confusion for most people when they begin working with a bellows-focusing camera. Of course, at infinity focus, it shouldn't be an issue. The other sort of "new" exposure issue that comes up in LF which you may not have noticed before is falloff and/or image circle limitations. I am assuming you don't mean that.
I am not sure I understand what you mean by "the neg was quite dark"... do you mean thick? Thin? When you say a neg is dark that sounds like it is too "thick" which means overexposed not under. Perhaps you mean the print is dark?
I do not add additional exposure on top of the filter factor- I just round up for simplicity if the factor is not in full stops. Almost always better to err on the side of slight overexposure with neg film.
I use B+W orange & red filters for 35mm & MF. I have found, from experience, that I need to add a stop extra exposure more than the stated filter factor for the orange using Delta 400 & FP4 to get simlar neg densities to unfiltered shots. This is with TTL reflective or incident metering.I've read on a number of occasions that additional exposure should be added on top of a filter factor, originally suggested by Gordon Hutchings- 1 extra stop for an orange #16 and 2 extra stops for a red #25. ...
Do many people apply that extra exposure? To all formats, or just LF? Why would I notice an effect in LF and not in 35 mm?
Thanks,
Tim
Tim,
How long are your exposures averaging, with the filters and stuff?
This one negative in particular was shot in bright daylight at Red Canyon. I can't remember what the settings were offhand (they may be in my notes at home), but I don't think the time was over 1 second, which is the cutoff for FP4+. I was using tilt to keep as wide an aperture as possible. I figured a red filter in red canyon against a blue sky would really lighten up the rocks while darkening the blue sky to really bring out the contrast. Everything ended up dark on the contact print. I haven't tried printing the neg otherwise, but it's obviously underexposed. I'm pretty sure I would have adjusted for reciprocity, but who knows- I've been known to forget to close my aperture before pulling my darkslide too!
It sounds like nobody follows the advice given by Hutchings here, adding that extra exposure. The table is reproduced in Steve Simmons' book. My understanding is that a red #25 (ff 3 stops) is advised to get 5 stops total extra on top of metered reading, and an orange (ff 2 stops) should get 4 stops extra total (as a general rule, not taking time of day, shadow coverage, or zone system adjustment into account).
Tim
It sounds like nobody follows the advice given by Hutchings here, adding that extra exposure. The table is reproduced in Steve Simmons' book. My understanding is that a red #25 (ff 3 stops) is advised to get 5 stops total extra on top of metered reading, and an orange (ff 2 stops) should get 4 stops extra total (as a general rule, not taking time of day, shadow coverage, or zone system adjustment into account).
Tim
I have recently been exchanging email's with Schneider Optics regarding B+W filter factors and Wratten filter numbers.
Schneiders' position is that a Factor is a Factor is a Factor! It makes no difference what emulsion you are using. T-grain emulsions are factored exactly as conventional emulsions. If your results are disappointing it is due to operator error, not the filter factor.
I was thinking reciprocity might be the culprit, but it sounds like you have a handle on that. What speed are you rating the FP4 at, and what developer are you using and what is your processing and times?
Tim, I would go with the basic filter factor + reciprocity + some fudge factor for response of the film. "Fudge factor" depends on the kind of light you're getting (e.g. morning, noon... spring or summer or winter... clear or fogged...) and the spectral sensitivity of your film and your filter cutoff. The fudge factor can be as little as zero or as large as several stops. Extreme cases:
*** You're shooting in the canyon in late summer and there are high clouds or mist or Santa Ana / LA crap blowing over the canyon. You know there is significant scatter of higher wavelengths and IR because of the clouds... the scene looks "bluer" than normal. In this case I would pick a fudge factor of at least one extra stop or two. Yeah, I know without precise metering it's not so scientific, but.... this is how I would rationalize my confidence in my exposure and hence my need to bracket.
***Other extreme case: really clear, spring weather over the canyon, no LA crap, no high clouds, the scene looks its normal pure, reddish colour. Fudge factor = zero. No real need to bracket the exposure.
I adopted this idea of a spectral sensitivity fudge factor when I started doing IR. I found that in the canyon, in the early summer, it was surprisingly hard to get a decent IR exposure because of the LA crap and high clouds. I got home, developed my negs, and found them to be lacking at least 2 or 3 stops. I think that would affect your reds in an analogous way because the spectral sensitivity of the film + the cutoff of the filter is fairly constant across deep red / near IR. And the LA crap does scatter well into the visible reds.
Tim, I think if you're working at either extreme end of the visible spectrum (blue or red) or indeed beyond that (UV or IR) then this "fudge factor" I mention can become very important. A really robust way to deal with this would be to use a digital sensor and to plug in a sensitivity curve that mimicks your film sensitivity + the filter's transmission curve. But most of the time you don't need to go to that level to get a good exposure.
Atmospheric conditions matter a lot when it comes to determining how much light in a given wavelength range makes it to your film, especially through a narrow filter. When you red filter you of course select out a particular narrow band of reddish wavelengths. If the reds are underrepresented in your illumination due to atmospheric conditions, then the appropriate exposure comp value can be something quite large. The filter factor concept is a rather dangerous one: it is merely a recommendation, and one that can be waaay off if the illumination isn't "ideal" and the film doesn't have broad and fairly uniform spectral sensitivity.
Haze appears less in IR exposure because the relevant atmospheric scattering goes as lambda^4 (lambda=wavelength), so IR light scatters much less in the atmosphere than bluer light. Hence the perceived better sharpness and contrast in IR. But notice, visible red light scatters quite a bit more than IR... the dependence is to the fourth power, after all. So I allege that I can wave my hands around several stops difference when shooting a scene like the canyon.
Metering through a filter has the obvious problem that the standard meter doesn't know the sensitivity curve of your film. Sometimes that is an issue. I think the very safest way to proceed is to learn how to estimate how much "spread" (uncertainty) there is in your exposure estimate and bracket accordingly. That doesn't mean that you have to bracket every damn shot, which would be expensive in LF. You could just bracket a representative scene and develop a bracket for that one shot, and determine how you will alter the rest of your development, if necessary. This is the practice that I have most recently been trying to adopt, in lieu of a fancy meter into which I can program a sensitivity curve.
T-grain emulsions are factored exactly as conventional emulsions.
They don't know what they're talking about.I have recently been exchanging email's with Schneider Optics regarding B+W filter factors and Wratten filter numbers.
Schneiders' position is that a Factor is a Factor is a Factor!
They don't know what they're talking about.
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