Showing posts with label Light. Show all posts
Showing posts with label Light. Show all posts

Thursday, January 14, 2010

18%


Here's a winter tip from your friendly photographer buddy, me. Many of you already know this, but you may not know the why of it.

The exposure meter in your camera, that sensor and logic that tells the camera how to expose your picture based on the current conditions, assumes that every scene will reflect an average amount of light. Experimentation has shown that an average scene reflects about 18% of the light that hits it. It's a generalized number and it works great for most scenes.

But if the scene you are photographing reflects more or less light than this on average, the exposure your camera calculates will be wrong.

Fresh snow is very bright white. And the reason it is very bright is that it reflects most of the light that hits it - that is WHY we see it as bright.

You probably see where this is going.

When you photograph snow, your camera does like it always does: it measures the light coming in from the scene and assumes the light it sees is the 18% reflection off the scene. But because snow reflects so much more than 18% of the light that strikes it, this calculated exposure will produce an underexposed image. Your camera has been fooled.

This will be more noticeable if most or all of your scene is snow, because the calculation is typically some kind of average for the scene.

And THAT, my friends, is why your snow always looks gray in your pictures when you can plainly see that it is most certainly NOT gray, it is pure white.

Your snow is simply underexposed.

So what to do? The solution is simple - you need to tell your camera to overexpose the scene. Yes, as crazy as it sounds when you are staring at a field of blinding white powder as far as the eye can see, you have to OVERexpose snow to make it look correct in your picture.

The trick is to dial in just enough added exposure to bring the snow up to white without pushing it so far that it becomes completely stark white and you lose picture information. Incidentally, this is called "blowing your highlights". No jokes now, we're all adults here. I usually overexpose by about 2 stops, but just try it and see what works.

Incidentally, 1 stop is a halving (-1 stop) or doubling (+1 stop) of light reaching the sensor or film. A 2 stop underexposure error by the camera is HUGE. It is 4 times less light than a correct exposure would be. Unless you are shooting and editing your pictures in the "raw" format of your camera (.DNG, .CRW, .CR2, .NEF, .NRW, etc.) or on film, you will not be able to correct that kind of error after the picture is taken. A .JPG file simply doesn't have that kind of dynamic range. That's why this can be very important.

There are also scenes that can fool your camera in the other direction, some scenes reflect very little light and can make your camera overexpose as it tries to get the scene's average brightness up to 18%. Lots of dull vegetation in a picture seems to do this.

So why don't they make cameras smarter? It's not that easy. Many cameras allow you to control which part of the scene is used for the 18% average by switching metering modes. Common modes are "Center Weighted Average", "Evaluative", and "Spot" metering, all of which can be useful in certain circumstances.

But remember one important fact as you think about this: many scenes do not have one "correct" exposure across the frame. There are many times when a scene may contain dark shadows underneath some subject, or a very bright patch of sky in one corner. In these cases the camera has to make a snap decision on which part of the scene will be exposed correctly. And although modern cameras have dizzyingly complex algorithms to help make this choice, they cannot account for all eventualities and they sometimes just fall flat on their faces.

In 1941 Ansel Adams and Fred Archer developed an elegant and sophisticated methodology called The Zone System, which used "tone mapping" to establish the dynamic range of a scene across a gray scale in great detail, and allowed the photographer to chose exposure based on exactly how he wanted the various shades to render in the final image. And if you've ever seen the work of Ansel Adams, you know how good The Zone System works in choosing exposure in a complicated scene.

Now, while you may not want to invest that much time in one picture, you do still have control and if you use your eyes and the histogram on the preview screen of your camera, you can often get very close. I've guessed exposures at shoots before when my light meter wasn't working and everything came out fine. Don't be afraid to experiment with exposure, you will not break your camera. In fact, setting your camera on "M" can be one of the most liberating experiences you can have with an electronic appliance.

Ok, NOW you can crack jokes.

Monday, January 11, 2010

Relationships


"The studio photographer is a master of light. The outdoor photographer is slave to it."

Thursday, December 17, 2009

Speed Bumps

"Even the very wise cannot see all ends" - Gandalf the Grey

Sometimes with progress comes setback. For many many years, incandescent bulbs were used in traffic lights. They were inefficient, not very bright (hence the big sun shields on them), didn't last long, and were very difficult and dangerous to replace.

But with the incredible advances in Light Emitting Diode (LED) technology we have seen these past five years, it didn't take long to figure out that the savings of moving traffic lights to the new technology would be huge. While an LED light costs more to make than an incandescent bulb does, they last almost forever (incandescents last about a year, while the first LEDs installed ten years ago are still going strong and will probably last at least 25 years unless they are physically damaged), use far less power, and they're very durable to boot. Heck, the color is even more vibrant. Win-win situation, right?

Well, not entirely. And here's why...

Remember, LED lights are very efficient. What that means is, they use less electricity. More than 90% less. That's the definition of efficiency here: more light per unit of energy. LEDs convert more energy to light so less goes to waste heat, as compared to incandescents.

See the problem yet? LEDs don't get hot. And in the winter, in states with significant snowfall, this turns out to be a big problem. LED streetlights do not melt the snow off of themselves! This has apparently led to many accidents and at least one death is blamed on it.

You can do your best, but there always seems to be one eventuality that slips through your analysis. So the LED engineers are back to the proverbial drawing board, devising a fix for this problem: a system that acts like a rear-window defroster, only when needed, that will cost a little more energy in the winter but still nowhere near as much as the old lights gobble.

Another hiccup, but the inexorable march of progress continues...

Saturday, June 20, 2009

A Pisa Lisa


Happy Birthday, Lisa

Monday, February 2, 2009

Somewhere & Somewhen


One of my favorite apps for my iPhone is an astronomy program I have called "Star Walk". It's an interactive visual map of the approximately 10,000 stars and "Messier Objects" in our sky that have an "apparent magnitude" of 6.5 or brighter (the lower, the brighter)*.

Basically, that's everything visible to the naked eye.

Since I do not own a telescope, it's perfect for me. Ever wonder where Vega is, or where in the sky you can find Cetus the Whale at a given time? Or when Venus is going to rise? It's in there! You can see the great spiral galaxy in Andromeda, M31, with it's hundreds of billions of suns, shining away and looking by eye just like a single star (it has an apparent magnitude of 4.5 from here, because it's more than 2 million light-years away!).

You can also go back or forward in time to see what the sky looked like "somewhen" else. And since the program is location-aware, the view you get is correct for the exact spot you are in, or any other you wish to choose.

So I've gone back in time to April 14th 1912, in the North Atlantic, to see that the new moon did indeed make it a very dark night for seeing icebergs.

The picture shows what the eastern sky looked like at the moment of my birth, as seen from the location of Mt. Carmel Hospital in Detroit. Looks like Venus, Jupiter, and Mercury were all there to check me out :)

* The magnitude scale is logarithmic, a first magnitude star is 100 times as bright as a sixth magnitude star. Amazingly, the Hubble Space Telescope can resolve objects down to an apparent magnitude of 30!

If you happen to have a big telescope or extreme curiosity, and easily visible stars don't cut it, try the USNO-B1.0 catalog. It is the most complete full-sky database, including more than a billion objects in various optical bands. It is considered accurate down to magnitude 21, far far below what we could ever see unaided.