Hi all,
Need to calibrate my light meter and I keep reading about gray card use, which seem unnecessary for what I'm after.
Pls tell me where I'm missing something.
So, I have an old light meter requiring calibration (Luna Pro in my case, but the discussion applies to any such generic
device allowing calibration). I'll be using Nikon D-200 DSLR's internal metering as a reference. I'm not interested in
knowing exact absolute number of Lux hitting the sensor, converting it to EV or any of that (may be that's what a gray
card is used for). All I need is to point D-200 to any uniformly lit object (a flat wall would be ideal), and illuminate it with
variable light source, dialing light intensity such that D-200 shows, say 1/25" with F/5.6 @ ISO=100 (or any combination
for that matter). The "whiter" the wall, the less illumination it will require to achieve this level of exposure, certainly no
need for the wall to be gray. I then turn adjustments on my light meter to show the same numbers on it. Next, I'll arbitrarily
increase light intensity to achieve next readout point, say, 1/200" @ F/5.6 @ the same ISO=100. Adjust my meter to match
that. Increment lighting a couple of more times to get additional measurement points, I may go back and forth a couple of
times, until Luna Pro readings match those of the D-200 for given lighting. Again, note, I don't care what is actual illumination
in Lux or what EV number is - the meter will sure show me that, but my objective is to just match un-calibrated hardware with
calibrated one - whatever EV happens to be in those steps. This the procedure doesn't care what color the wall is, it certainly
does not have to be gray and in fact doesn't have to be a wall at all - can be any object I can artificially illuminate and point
both meters to. Looks like no need for gray cards of any sort for such calibration. What am I missing?
Hi all,
Need to calibrate my light meter and I keep reading about gray card use, which seem unnecessary for what I'm after.
Pls tell me where I'm missing something.
So, I have an old light meter requiring calibration (Luna Pro in my case, but the discussion applies to any such generic
device allowing calibration). I'll be using Nikon D-200 DSLR's internal metering as a reference. I'm not interested in
knowing exact absolute number of Lux hitting the sensor, converting it to EV or any of that (may be that's what a gray
card is used for). All I need is to point D-200 to any uniformly lit object (a flat wall would be ideal), and illuminate it with
variable light source, dialing light intensity such that D-200 shows, say 1/25" with F/5.6 @ ISO=100 (or any combination
for that matter). The "whiter" the wall, the less illumination it will require to achieve this level of exposure, certainly no
need for the wall to be gray. I then turn adjustments on my light meter to show the same numbers on it. Next, I'll arbitrarily
increase light intensity to achieve next readout point, say, 1/200" @ F/5.6 @ the same ISO=100. Adjust my meter to match
that. Increment lighting a couple of more times to get additional measurement points, I may go back and forth a couple of
times, until Luna Pro readings match those of the D-200 for given lighting. Again, note, I don't care what is actual illumination
in Lux or what EV number is - the meter will sure show me that, but my objective is to just match un-calibrated hardware with
calibrated one - whatever EV happens to be in those steps. This the procedure doesn't care what color the wall is, it certainly
does not have to be gray and in fact doesn't have to be a wall at all - can be any object I can artificially illuminate and point
both meters to. Looks like no need for gray cards of any sort for such calibration. What am I missing?
Doing a one point photometric calibration by matching an unknown light meter to a known and correct light meter inspires confidence in getting good exposure information.
I've done this procedure but I still got some exposures wrong. My problem involved a camera with a good TTL meter, Pentax ME-Super, matched to a good Gossen Luna Pro hand held meter.
Faced with a normal outdoor landscape the Pentax would give three different meter readings depending on framing the scene with a bit of sky, 1/2 sky, or a lot of sky. How do I know which reading is correct?
Only one reading is right and I can get it by turning the exposure compensation dial. But this involves either well practiced judgement born of long experience or outright guess work supported by exposure bracketing. Not so easy.
Alternatively how should I deploy the Luna Pro meter to find this "correct" reading? Is it meter the ground and forget the sky, meter the sky and give two stops more, or is it meter land and sky and strike an average?
Again the decision depends on long experience or, failing that, more guesswork. The one point calibration told me that the TTL camera and hand held meter were not contradictory but they do see the world in different ways.
And I still have to make a judgement call about exposure settings.
Some things seem to be that obvious people forget. If you take a picture of a 18% grey card and your film development and light meter are functioning properly you will get a negative that wil transmit 18% of the light. If you print that negative you will get a print that reflects 18%. That’s the way a photographic can be calibrated.
As usual, we certainly have gotten far afield. All 336v wants to do is calibrate his light meter so that it works correctly. He thought of comparing it to the results from his camera -- which is one way -- but it's much simpler to calibrate it to match the f16 rule. No camera or gray card or average scene or gymnastics of any kind are needed.
In fact if you calibrate for the f/16 rule you will indeed need the gray card.
As usual, we certainly have gotten far afield. All 336v wants to do is calibrate his light meter so that it works correctly. He thought of comparing it to the results from his camera -- which is one way -- but it's much simpler to calibrate it to match the f16 rule. No camera or gray card or average scene or gymnastics of any kind are needed.
But the Sunny 16 rule of thumb is only an APPROXIMATION on any given day, and one could be 'calibrating' one's meter outside the actual range of exposures specifiied by the ISO standard formula!
stability of 'sunny 16'
I normally see a 1/2 to full stop between a reflective and incident and meters depending on the scene, how much sky, or very bight and large reflective surfaces may be present. It is my understanding that Nikon optimized their version of matrix or evaluative meting for slides, not sure if true...www.photrio.com
...so you know your meter is 'approximately right' if depending upon Sunny 16.
Add up an approximate meter reading, and an approximate f-stop setting, and an approximate shutter speed accuracy, and an approximate ISO rating and you can forget about getting to home plate! You're lucky to land in the ball park.
I thought the point of a light meter was to have something to blame when the exposure's wrong!
Since the print can be made over a range of enlarger time choices, this seems like a circular argument. Any negative transmitting any percentage can be printed to the print of 18% reflection. what am I missing?
I thought the point of a light meter was to have something to blame when the exposure's wrong!
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