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For now, however, we will confine ourselves to the range of printable values in a straight print, Zones 0 to 9. I have mentioned several times that by doubling the exposure, you can jump from one zone to the next higher one; but how do you double the exposure? Simple! A quick glance at your camera shows that the shutter speeds are (in fractions of a second) 1, ½, ¼, , , , , , , , and perhaps . Each speed is half the exposure of the previous one. If you go the other way, each is twice the speed of the previous one. Thus, if your exposure is second, you double the exposure by going to second. If your exposure is ¼ second, you double it by going to ½ second. So the camera’s shutter speeds tie in immediately with the zones.

There is another way to open up or close down a zone: by closing the aperture (i.e., the opening) of the lens. Look at the aperture settings, also known as the f/stops. They are f/2, f/2.8, f/4, f/5.6, f/8, f/11, f/16, f/22, and perhaps f/32, f/45, and f/64. Each of these numbers represents a halving of the aperture from the previous setting. Thus, f/5.6 admits half the light that f/4 admits. F/16 allows only half the light through the lens that f/11 allows. The higher the number, the smaller the aperture and the less light passes through the lens. Again, the camera and the zone system work together in harmony

The photograph contains a full range of tonalities from black to white, yet there appear to be no jarring contrasts. There are small amounts of dodging and burning, but no extensive alterations.

Figure 8-2. Stairway to Cittá Alta, Bergamo, Italy

Table 8-1. Negative density and print tonal scale

Negative Density and Print Tonal Scale

THE NEGATIVE

ZONES

THE PRINT

12

13

Double the exposure of Zone

11

12

Paper Base white

Double the exposure of Zone

10

11

Paper Base white

Double the exposure of Zone

9

10

Paper Base white

Double the exposure of Zone

8

9

Paper Base white

Double the exposure of Zone

7

8

Very light gray—no visible textures, but tonally darker than pure white

Double the exposure of Zone

6

7

Light gray—clearly visible light textures

Double the exposure of Zone

5

6

Medium light gray

Double the exposure of Zone

4

5

Medium gray—the 18% gray card

Double the exposure of Zone

3

4

Medium dark gray

Double the exposure of Zone

2

3

Dark gray—clearly visible textures

Double the exposure of Zone

1

2

Very dark gray—no visible textures, but tonally lighter than black

First obvious density

1

Black (no real difference from Zone 0)

No density—film base fog

0

Maximum black

The other confusion comes from the fact that the f/stop number is actually a ratio of the lens opening to the focal length of the lens, so we are really dealing with an inverse amount, or ¼, , , , , , , , etc. This is how we end up with the rule, “The bigger the number, the smaller the hole,” i.e., the larger the f/stop number, the smaller the aperture.

The two methods of doubling or halving the exposure, via aperture or shutter speed, point out a very important relationship: one zone is equal to one stop. When you “open up a stop—for example from f/11 to f/8—you are at the same time giving one zone more exposure. In the same way, when you change the shutter speed from, say, second to second, you are also “opening up one stop” or giving one stop greater exposure.

Now that you know what the zones are and how you can jump from one to another with your camera, set that information aside for a while as we look at the workings of the light meter. By combining the knowledge of the zones with an understanding of the light meter, the zone system becomes immediately clear.

Note

As a brief technical aside, it is worth explaining aperture numbers, which seem so arbitrary and senseless at first. The formula for the area of a circle is A=πr2, where A is the area of the circle, r is its radius, and π=3.14159. If you square each of the aperture numbers (i.e., multiply it by itself) and plug them into the formula as r2, they form a simple geometric progression: 4, 8, 16, 32, 64, 128, 256, 512, etc., so that each opening is half or double the previous one.

The Light Meter—How it Works

In order to fully understand the light meter, let’s refer to it by a different name for awhile. The name “light meter” is a bit confusing. We’ll call it a “gray meter” because its only function is to tell the proper exposure for medium gray, or Zone 5. All gray meters do the same thing: they average light within the viewing angle of the meter and give you a reading of the proper exposure for Zone 5. That is the only thing they do!

Note

All gray meters do the same thing: they average light within the viewing angle of the meter and give you a reading of the proper exposure for Zone 5. That is the only thing they do!

The gray meter has no idea what it’s pointed towards. It could be a dark coat in a hallway, a field of snow under bright sun, a person’s face under overcast skies, or anything else you can think of. All it knows is the amount of light that impinges on its lightsensitive cells. Since it has no idea what it’s looking at, it cannot give the proper exposure for the item, so it gives the Zone 5 exposure! For this reason, it should logically be called a gray meter.

Zone 5 may be just the right exposure for many things—perhaps a person’s face under overcast skies (though it seems a bit too dark to me)—but it surely is not the proper exposure for sunlit snow! The difference between you and the gray meter is that you can think! Recognizing that the meter always gives a Zone 5 reading, you can supply your knowledge of the tonal scale to determine the proper exposure.

Let’s take the case of sunlit snow. If the snow has modulations—small hills and valleys—and perhaps even some shadows, you may want it somewhere between Zone 7 (easily seen light gray textures) and Zone 8 (very light gray, almost white—no real textures). Even though snow is white, you probably want to avoid a blank white area lacking in detail. Suppose the gray meter reads f/16 @