Ysarex
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Ysarex said:Outside, the Sunny 16 rule, and variations, works well. Indoors, which is what the OP mentioned, it is much harder. Photographers took to meters for a reason.
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The OP mentioned both, "Where I'm at right now is that I'll walk into a room or outside..." For many decades before meters existed photographers managed to successfully take photos both outdoors and indoors. Erich Salomon's Ermanox wasn't equipped with a light meter in the 1920s. It is likewise possible to train oneself to reasonably judge the level of interior brightness, but yes it is more difficult than doing the same outside.
Not suggesting abandoning a meter if you have one -- just answering the OP's question.
I applaud the OP for the question and the effort to learn. There's advantage to having a good understanding of the photographic process. Another story: Again early in my career I worked selling Pro gear. I remember a fashion photographer who had to spend a lot of money paying for a re-shoot because he blew the original shoot. He brought me his light meter which we determined was at fault for his debacle. It had broken as was reading more than 5 stops off. How do you miss an equipment failure like that?
Joe
Joe,
Do you recall the circular calculator system that was sold for a time, mail-order mostly, in which lighting levels and exposures were tied to a simple X-value system, which began with the Sunny 16 rule as the Zero-X baseline, and then added exposure in one-stop or one-X increments? I read about it in Popular Photography magazine, but it never got off the ground really. Sort of similar to Fred Parker's Ultimate Exposure Computer, but a bit different, and I would say, better conceptualized. Parker's Ultimate Exposure computer is shown as an EV value chart that is directly associated with real-world lighting scenarios, like EV 16 which is light that is one exposure value brighter than Sunny 16, meaning EV 16 is "Subjects in bright daylight on sand or snow". The Sunny 16 rule means light that is E.V. 15 in brightness.
The EV System is fine as a framework, but it is almost always presented merely as a charted set of numbers and f/stop and shutter speed times, with no verbal or illustrated linkage to actual shooting scenarios or common types of scenes. We can say "EV 14! EV 15!", but without a kind of scene, a type of location, or some kind of general description, the saying of the two words, "EV fifteen" means...nothing to most people.
The X-System, as it was called (to the best of my recollection) began as I said, at Sunny 16 at let's just say, ISO 100 film speed, so f/16 at 1/100 second. Keep in mind, the Sunny 16 settings refer to an EV light value rating of 15. The X-system began there, as "O-X", or Baseline. As the light level grew dimmer, another "X" was added, meaning the lens was opened up one more stop, or the shutter slowed by one stop value, or any combination of both.
So...beginning at Zero-X,the X-system was like this:
The Full moon or weak, hazy sunlight was +1-X.
Cloudy-bright with no shadow light was +2-X.
Heavy Overcast or Open Shade lighting was +3-X.
Sunsets and Deep Shade was +4-X.
Landscapes and City Skylines just after sundown was +5-X.
Neon Lights,Landscapes, Skylines, 10 mins after sunset +6-X
Las Vegas, TImes Square,campfires,bonfires,ice shows, baseball, football, bright interiors with florescent light +7-x.
Indoor sports, circuses, bottom of rainforest canopy, +8-x.
This continued to Moonlight, at +20-X for moonlit landscapes, and ended at +21-X, starlighted landscapes.
The Minus-X stuff was all crazy-bright stuff, like "Welding Arc flame at work surface" and so on.
This system had basically 21 different scene brightness levels to work with in normal, everyday situations. The advantage it offered was that it began right at the Sunny 16 rule, and was based on the simple idea like, okay, some light clouds come out, I need to go Plus-1 "X". A little bit darker but still daylight, plus 2-X. Heavy Overcast or Open Shade, plus 3-X. So, basically, there are about 21 different exposure brightness values that a person could use for most of a lifetime, and only 12 of them which take you down in brightness (but "up" in X-value) to "Fireworks".
That sounds vaguely familiar -- I am aware of Parker's exposure calculator.
"The EV System is fine as a framework, but it is almost always presented merely as a charted set of numbers and f/stop and shutter speed times, with no verbal or illustrated linkage to actual shooting scenarios or common types of scenes. We can say "EV 14! EV 15!", but without a kind of scene, a type of location, or some kind of general description, the saying of the two words, "EV fifteen" means...nothing to most people."
Yes, so often when EV values are referred to a lot is assumed in the background. But this background assuming often muddies the meaning of the EV values. EV 15 is correct exposure for ISO 100 in direct sunshine -- there's no reason other than convention for that to be some kind of standard. If you spent your years in the 60s and 70s shooting Tri-X then EV 17 was the sunny day standard and for us Kodachrome shooters it was EV 14. By itself an EV number is not a brightness level or a film/sensor exposure.
All the EV number really does is take the two variables of shutter speed and f/stop and combine them into a single value which is then a constant. At a fixed EV the camera "light pipe" is set to a fixed value. That value doesn't identify a brightness level. Thinking "light pipe" again the shutter and f/stop are like the hot and cold handles to a sink faucet. How much water get's through is a function of both the size of the opening set on the faucet as well as the water pressure. In our case (photo) the EV value plus the intensity of the ambient light (water pressure) determine the exposure brightness. Exposure being a function of ambient light intensity plus shutter speed plus f/stop: exposure = light intensity + EV.
That still doesn't work in ISO. Back to the water faucet analogy ISO is the size of the glass you're holding under the faucet. Ideally you want to fill it.
Joe