I read that for metering sun sets one points the spot meter about 6 solar diameters off the sun, this has worked very well for me at least. The difference between this and night shots is that with night shots your exposure meter simply says "there is no light at all" when an 1 hour exposure confirms the opposite. It may even be useful for estimating maximum useful exposure time for star trail shots, before the back ground brightness registers on my film.This did remind me though of the method my father taught me for metering sunsets: Point the meter straight up vertically. I can remember trying it once but can't recall how successful it was.
Interesting idea. Which direction do you use for the offset? Is that recommendation designed to be metered on clear sky?I read that for metering sun sets one points the spot meter about 6 solar diameters off the sun, this has worked very well for me at least.
Google for The Ultimate Exposure Computer...very, very accurate for a variety of situations.
Thanks. I believe you'll find that the EOS 3 has a 2.4% spot meter. The viewing angle of the metering area in degrees will change with the focal length with an in camera TTL spot meter. That's why I assumed from your description that you were using a handheld spot meter.@Lee: The 6 diameters rule is not a scientifically verified law but just a rule of thumb which I apply for sun set shots with silhuettes and with which I have gotten excellent results on slide film so far. I don't know about dedicated spot meters, as my EOS 3 does this job very well with its 1° spot measurement function.
@PVia: The ultimate exposure guide just lists a number of light situations together with an exposure estimate for them. It does, unfortunately not tell me how long I can expose star trails before the back ground turns grey or how long to expose a very dark forrest or landscape (this is also where the in camera meter of my SLR falls short). For good negative film it's not a big deal if you are one or two stops off, for slide film being 2 stops off kills the image.
@wiltw: sure, reciprocity failure needs to be taken into account, but that's something you measure only once for every film (or look up numbers online). As long as I did night time exposures with negative film the results looked great, although I just guestimated the exposure time. Unfortunately slide film isn't that forgiving, so I started looking for a measurement device for extremely low light.
Sorry for my confusion. You are correct, the spot meter of my EOS 3 covers 2.4% of the view finder screen, so it covers about 20mm^2 on the film. This corresponds to a circle with a diameter of 5mm. With my 70-210 F/4 I get angular coverage across the diameter of the spot metering circle of about 1.4°.Thanks. I believe you'll find that the EOS 3 has a 2.4% spot meter. The viewing angle of the metering area in degrees will change with the focal length with an in camera TTL spot meter. That's why I assumed from your description that you were using a handheld spot meter.
The Ultimate Exposure Guide is a list of typical exposure situations, not a meter, and shouldn't be mistaken for one. IMHO it's exactly these kinds of guides and the need for bracketing which drove so many night shooters into the digital camp. My aim is to employ a device specifically made for measuring extremely low light szenarios for my photographic purposes. Bracketing is no fun if your exposures take hours.Actually it does, it essentially provides you a zone 5 setting/reading, like all incident meters try to.
It's up to you where to place the zones in your shot from there.
My aim is a device which tells me (directly or through conversion tables) what exposure an ideal film sans reciprocity failure would require for a zone 5 exposure. Adding or subtracting stops for specific purposes is trivial, and facturing in reciprocity failure should require much fewer failed shots than guestimating szene illumination with my bare eyes.Like reciprocity, the camera setting you might like for a given effect in a given lighting situation is only necessary once.
I guess I'll just try it out and report ...
The Ultimate Exposure Guide is a list of typical exposure situations, not a meter, and shouldn't be mistaken for one. IMHO it's exactly these kinds of guides and the need for bracketing which drove so many night shooters into the digital camp. My aim is to employ a device specifically made for measuring extremely low light szenarios for my photographic purposes. Bracketing is no fun if your exposures take hours.
Obviously some vocal converts may be driven more by ample supply of marketing dollars than by real photographic benefits. Some of the problems with quickly discharging batteries and excessive noise have been overcome years ago (battery grips, image stacking), while analog shooters still resort to bracketing once our light meters prove too insensitive for the task. I wasn't looking for a magic bullet which makes my shots better, just for a metering device for extremely low light situations. If I can see details in a scenery with my bare eyes, a sensitive light meter should be able to deliver accurate numbers.IMHO there are no magic bullet devices and the digi converts probably moved for other reasons because they face real limits for night use; their sensors and batteries tend to die or simply won't do what is asked when a truly long exposure, hours, is needed.
It's reading corresponds do star magnitude per square arc second. Someone could calculate how this corresponds to exposure values, but I rather let the spot meter of my camera find this out for me (compare spot meter reading of a moderately dark spot to the reading of the SQM). One star magnitude is about a factor of 2.5 (it's a logarithmic measure), so I could put together a table very quickly.Back to the original question: I can't find a sensitivity (stellar magnitude or whatever) given for that device.
Could this help me estimate accurate exposure times for night shots as well?
Once I got the exposure nailed I can deal with color casts (in the worst case in a hybrid work flow, my scanner does much much better with slides than negs). Right now I look at pics with bright white mountains in front of white sky and dim star trails on light grey sky. And very short star trails on black sky. I'd rather spend 10 minutes measuring light and thinking it through than spray&pray.Maybe this could give you some data, but EV may not be the whole, nor even the biggest issue with your slide film providing poor results.
What is the difference between the real color of the scene and the way you want to render it?
How are you going to judge your filtering to get all three color layers exposed properly for the result you want?
Since it's used to estimate observability of stars with human eyes (bare or through a telescope) I assume it's mostly sensitive to the wave lengths we see. I don't have this thing yet but if I get it I can try shining some IR diodes at it and see whether it gets fooled by them. I asked my question not in an attempt to advertise some gadgetery but to find out whether other folks have already tried this.Is your film sensitive to a broader or narrower set light wavelengths than the meter?
I was not aware that scene contrast would be narrow, in my experience I had to battle excessive contrast as soon as artificial lighting exists in small parts of the view. Moon light should yield similar contrast levels to sun light.One other question here is; how you plan to adjust the development to correct for the narrow scene contrast?
Once I got the exposure nailed I can deal with color casts (in the worst case in a hybrid work flow
, my scanner does much much better with slides than negs). Right now I look at pics with bright white mountains in front of white sky and dim star trails on light grey sky.
I was not aware that scene contrast would be narrow, in my experience I had to battle excessive contrast as soon as artificial lighting exists in small parts of the view. Moon light should yield similar contrast levels to sun light.
I was at a workshop a week ago and we were all shooting a landscape scene late afternoon and over cast, the total SBR was about 3 stops when we arrived even shooting toward the horizon and measured by a variety of spot meters. That dropped to as little as 1 stop SBR before we left and it wasn't even dark yet.
Excluding point sources a night landscape may have an SBR well under 0.5. This is where I think your white mountain gray sky issue is rooted.
Could you go into more detail as to how you made these measurements?
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