Left to its own devices, your 90D can do an excellent job of providing the proper exposure for most scenes. But even a camera as smart as the 90D frequently can benefit from intelligent input. For example, when you shoot with the main light source behind the subject, you end up with backlighting, which can result in an overexposed background and/or an underexposed subject. The Canon 90D recognizes backlit situations nicely, and, in most cases, can properly base exposure on the main subject using the default Evaluative metering mode, producing a decent photo.
But, as a creative photographer, there will be many instances where you would rather not have automatic correction for backlighting. What if you want to underexpose the subject to produce a silhouette effect? The 90D does a poor job of exposing intentional silhouettes and will end up producing unwanted detail in what should have been inky black areas of your image. Fortunately, the camera has metering modes and other exposure options that allow you to produce the image you are looking for. If you’re looking for an extensive exposure range, options like the 90D’s built-in Highlight Tone Priority and Auto Lighting Optimizer features can adjust your exposure as you take photos, preserving detail in the highlights and shadows as required. Your Canon 90D also has the capability of fine-tuning exposure separately for each of the metering modes, so you can consistently add or subtract a little exposure to suit your creative tastes.
This chapter discusses using the full range of the camera’s various shooting modes and exposure controls, so you’ll be better equipped to override the default settings when you want to, or need to, and achieve spot-on exposures that produce the exact image you are looking for, every time.
The 90D gives you a great deal of control over all of these, although composition is entirely up to you. You must still frame the photograph to create an interesting arrangement of subject matter, but all the other parameters are basic functions of the camera. You can let your 90D set them for you automatically, you can fine-tune how the camera applies its automatic settings, or you can make them yourself, manually. The amount of control you have over exposure, sensitivity (ISO settings), color balance, focus, and image parameters like sharpness and contrast make the 90D a versatile tool for creating images.
In the next few pages, I’m going to give you a grounding in one of those foundations, and explain the basics of exposure, either as an introduction or as a refresher course, depending on your current level of expertise. When you finish this chapter, you’ll understand most of what you need to know to take well-exposed photographs creatively in a broad range of situations.
This section explains the fundamental concepts that go into creating an exposure. If you already know about the role of f/stops, shutter speeds, and sensor sensitivity in determining an exposure, you might want to skip to the next section, which explains how the 90D calculates exposure.
In the most basic sense, exposure is all about light. Exposure can make or break your photo. Correct exposure brings out the detail in the areas you want to picture, providing the range of tones and colors you need to create the desired image. Poor exposure can cloak important details in shadow or wash them out in glare-filled featureless expanses of white. However, getting the perfect exposure requires some intelligence—either that built into the camera or the smarts in your head—because digital sensors can’t capture all the tones we are able to see. If the range of tones in an image is extensive, embracing both inky black shadows and bright highlights, we often must settle for an exposure that renders most of those tones—but not all—in a way that best suits the photo we want to produce.
As the owner of a Canon EOS 90D, you’re probably well aware of the traditional “exposure triangle” of aperture (quantity of light, light passed by the lens), shutter speed (the amount of time the shutter is open), and the ISO sensitivity of the sensor—all working proportionately and reciprocally to produce an exposure. The trio is itself affected by the amount of illumination that is available to work with. So, if you double the amount of light, increase the aperture by one stop, make the shutter speed twice as long, or boost the ISO setting 2X, you’ll get twice as much exposure. Similarly, you can increase any one of these factors while decreasing one of the others by a similar amount to keep the same exposure.
Working with any of the three controls involves trade-offs. Larger f/stops provide less depth-of-field, while smaller f/stops increase depth-of-field (and potentially at the same time can decrease sharpness through a phenomenon called diffraction). Shorter shutter speeds do a better job of reducing the effects of camera/subject motion, while longer shutter speeds make that motion blur more likely. Higher ISO settings increase the amount of visual noise and artifacts in your image, while lower ISO settings reduce the effects of noise. (See Figure 4.1.)
Exposure determines the look, feel, and tone of an image, in more ways than one. Incorrect exposure can impair even the best-composed image by cloaking important tones in darkness, or by washing them out so they become featureless to the eye. You’ll often need to make choices about which details are important, and which are not, so that you can grab the tones that truly matter in your image. That’s part of the creativity you bring to bear in realizing your photographic vision.
For example, look at two bracketed exposures presented at top in Figure 4.2. For the image at upper left, there is plenty of detail in the interior of this country store/post office, but the exterior visible through the windows is completely washed out. In the version at top right, taken an instant later using a tripod-mounted camera, the scene outside is well exposed, but the store’s interior is murky and dark. The camera’s sensor simply can’t capture detail in both dark areas and bright areas in a single shot.
With digital camera sensors, it’s tricky to capture detail in both highlights and shadows in a single image, because the number of tones, the dynamic range of the sensor, is limited. The solution, in this particular case, was to resort to a technique called High Dynamic Range (HDR) photography, in which the two exposures from Figure 4.2 were combined in an image editor such as Photoshop, or a specialized HDR tool like Photomatix (about $100 from www.hdrsoft.com). The resulting shot is shown at bottom in Figure 4.2. I’ll explain more about HDR photography later in this chapter. For now, though, I’m going to concentrate on showing you how to get the best exposures possible without resorting to such tools, using only the features of your Canon 90D.
To understand exposure, you need to understand the six aspects of light that combine to produce an image. Start with a light source—the sun, an interior lamp, or the glow from a campfire—and trace its path to your camera, through the lens, and finally to the sensor that captures the illumination. Here’s a brief review of the things within our control that affect exposure.
These factors all work proportionately and reciprocally to produce an exposure. That is, if you double the amount of light that’s available, increase the aperture by one stop, make the shutter speed twice as long, or boost the ISO setting 2X, you’ll get twice as much exposure.
If you’re really new to more advanced cameras (and I realize that many soon-to-be-ambitious photographers do purchase the 90D as their first digital SLR), you might need to know that the lens aperture, or f/stop, is a ratio, much like a fraction, which is why f/2 is larger than f/4, just as 1/2 is larger than 1/4. However, f/2 is actually four times as large as f/4. (If you remember your high school geometry, you’ll know that to double the area of a circle, you multiply its diameter by the square root of two: 1.4.)
Lenses are usually marked with intermediate f/stops that represent a size that’s twice as much/half as much as the previous aperture. So, a lens might be marked f/2, f/2.8, f/4, f/5.6, f/8, f/11, f/16, or f/22, with each larger number representing an aperture that admits half as much light as the one before, as shown in Figure 4.3.
Shutter speeds are actual fractions (of a second), but the numerator is omitted, so that 60, 125, 250, 500, 1000, and so forth represent 1/60th, 1/125th, 1/250th, 1/500th, and 1/1000th second. To avoid confusion, Canon uses quotation marks to signify longer exposures: 2”, 2”5, 4”, and so forth representing 2.0-, 2.5-, and 4.0-second exposures, respectively.
One of the most important aspects in this discussion is the concept of equivalent exposure. This term means that exactly the same amount of light will reach the sensor at various combinations of aperture and shutter speed. Whether we use a small aperture (large f/number) with a long shutter speed or a wide aperture (small f/number) with a fast shutter speed, the amount of light reaching the sensor can be exactly the same. Table 4.1 shows equivalent exposure settings using various shutter speeds and f/stops; in other words, any of the combination of settings listed will produce exactly the same exposure.
Most commonly, exposure settings are made using the aperture and shutter speed, followed by adjusting the ISO sensitivity if it’s not possible to get the preferred exposure; that is, the one that uses the “best” f/stop or shutter speed for the depth-of-field (range of sharp focus) or action stopping we want (produced by short shutter speeds, as I’ll explain later).
When the 90D is set for P (Program) mode, the metering system selects the correct exposure for you automatically, but you can change quickly to an equivalent exposure by locking the current exposure, and then spinning the Main Dial until the desired equivalent exposure combination is displayed. You can use this standard Program Shift feature more easily if you remember that you need to rotate the dial toward the left when you want to increase the amount of depth-of-field or use a slower shutter speed; rotate to the right when you want to reduce the depth-of-field or use a faster shutter speed. The need for more/less DOF and slower/faster shutter speed are the primary reasons you’d want to use Program Shift. I’ll explain Program mode exposure shifting options in more detail later in this chapter.
In Aperture-priority (Av) and Shutter-priority (Tv) modes, you can change to an equivalent exposure using a different combination of shutter speed and aperture, but only by either adjusting the aperture in Aperture-priority mode (the camera then chooses the shutter speed) or shutter speed in Shutter-priority mode (the camera then selects the aperture). I’ll cover all these exposure modes and their differences later in the chapter.
In photography parlance, f/stop always means the aperture or lens opening. However, for lack of a current commonly used word for one exposure increment, the term stop is often used. In the past, EV (Exposure Value) served this purpose, and was used as a measure of the total sensitivity range of a device such as a light meter, but exposure value and its abbreviation have since been inextricably intertwined with its use in describing exposure compensation. In this book, when I say “stop” by itself (no f/), I mean one whole unit of exposure, and am not necessarily referring to an actual f/stop or lens aperture. So, adjusting the exposure by “one stop” can mean changing to the next shutter speed increment (say, from 1/125th second to 1/200th second) or the next aperture (such as f/4 to f/5.6). Similarly, 1/3-stop or 1/2-stop increments can mean either shutter speed or aperture changes, depending on the context. Be forewarned.
When using the optical viewfinder, your Canon 90D calculates exposure by measuring the light that passes through the lens and is bounced up by the mirror to a 220,000-pixel RGB plus IR-sensitive metering sensor located near the focusing surface. (Note: In live view, the sensor image is used instead, as I’ll explain later.) Light is evaluated using a pattern you can select (more on that later) and based on the assumption that each area being measured reflects about the same amount of light as a neutral gray card that reflects a “middle” gray of about 12 to 18 percent reflectance. (The photographic “gray cards” you buy at a camera store have an 18 percent gray tone, which does represent middle gray; however, your camera is calibrated to interpret a somewhat darker 12 percent gray; I’ll explain more about this later.) That “average” 12 to 18 percent gray assumption is necessary, because different subjects reflect different amounts of light. In a photo containing, say, a white cat and a dark gray cat, the white cat might reflect five times as much light as the gray cat. An exposure based on the white cat will cause the gray cat to appear to be black, while an exposure based only on the gray cat will make the white cat appear washed out.
This is more easily understood if you look at some photos of subjects that are dark (they reflect little light), those that have predominantly middle tones, and subjects that are highly reflective. The next few figures show a simplified scale with a middle gray 18 percent tone, plus black and white patches, along with a human figure (not a cat) to illustrate how different exposure measurements actually do affect an exposure.
The image shown in Figure 4.4, left, represents how a photograph might appear if you inserted the patches shown at bottom left into the scene, and then calculated exposure by measuring the light reflecting from the middle gray patch, which, for the sake of illustration, we’ll assume reflects approximately 12 to 18 percent of the light that strikes it. The exposure meter in the camera sees an object that it thinks is a middle gray (the middle patch), calculates an exposure based on that, and the patch in the center of the strip is rendered at its proper tonal value. Best of all, because the resulting exposure is correct, the black patch at left and white patch at right are rendered properly as well.
When you’re shooting pictures with your 90D camera, and the meter happens to base its exposure on a subject that averages that “ideal” middle gray, then you’ll end up with similar (accurate) results. The camera’s exposure algorithms are concocted to ensure this kind of result as often as possible, barring any unusual subjects (that is, those that are backlit, or have uneven illumination). The camera has five different metering modes (described in an upcoming section), each of which is equipped to handle certain types of unusual subjects, as I’ll outline.
Figure 4.4, center, shows what would happen if the exposure were calculated based on metering the leftmost, black patch, which is roughly the same tonal value of the darkest areas of the subject’s hair. The light meter sees less light reflecting from the black square than it would see from a gray middle-tone subject, and so figures, “Aha! I need to add exposure to brighten this subject up to a middle gray!” That lightens the “black” patch, so it now appears to be gray.
But now the patch in the middle that was originally middle gray is overexposed and becomes light gray. And the white square at right is now seriously overexposed and loses detail in the highlights, which have become a featureless white. Our human subject is similarly overexposed. You should always be aware when overexposure occurs but note that it’s not always a bad thing. Some slight overexposures add a dreamy look to an image; once you know how the rules are derived, you’ll know how and when to break them.
The third possibility in this simplified scenario is that the light meter might measure the illumination bouncing off the white patch and try to render that tone as a middle gray. A lot of light is reflected by the white square, so the exposure is reduced, bringing that patch closer to a middle-gray tone. The patches that were originally gray and black are now rendered too dark. Clearly, measuring the gray card—or a substitute that reflects about the same amount of light—is the only way to ensure that the exposure is precisely correct. (See Figure 4.4, right.)
As you can see, the ideal way to measure exposure is to meter from a subject that reflects 12 to 18 percent of the light that reaches it. If you want the most precise exposure calculations, the solution is to use a stand-in, such as the evenly illuminated gray card I mentioned earlier. But, because the standard Kodak gray card reflects 18 percent of the light that reaches it and, as I said, your camera is calibrated for a somewhat lighter 12 percent tone, you would need to add about one-half stop more exposure than the value metered from the card. Of course, in most situations, it’s not necessary to do this. Your camera’s light meter will do a good job of calculating the right exposure, especially if you use the exposure tips in the next section. But I felt that explaining exactly what is going on during exposure calculation would help you understand how your camera’s metering system works.
In some very bright scenes (like a snowy landscape or a lava field), you won’t have a mid-tone to meter. Another substitute for a gray card is the palm of a human hand (the backside of the hand is too variable). But a human palm, regardless of ethnic group, is even brighter than a standard gray card, so instead of one-half stop more exposure, you need to add one additional stop. That is, if your meter reading is 1/500th of a second at f/11, use 1/500th second at f/8 or 1/200th second at f/11 instead. (Both exposures are equivalent.)
Or you might want to resort to using an evenly illuminated gray card mentioned earlier. Small versions are available that can be tucked in a camera bag. Place it in your frame near your main subject, facing the camera, and with the exact same even illumination falling on it that is falling on your subject. Then, use the Spot metering function (described in the next section) to calculate exposure.
In serious photography, you’ll want to choose the metering mode (the pattern that determines how brightness is evaluated) and the exposure mode (determines how the appropriate shutter speed and aperture is set). I’ll describe both aspects in later sections.
Why are so many photographers under the impression that camera light meters are calibrated to the 18 percent “standard,” rather than the true value, which may be 12 to 14 percent, depending on the vendor? You’ll find this misinformation in an alarming number of places. I’ve seen the 18 percent “myth” taught in camera classes; I’ve found it in books, and even been given this wrong information from the technical staff of camera vendors. (They should know better—the same vendors’ engineers who design and calibrate the cameras have the right figure.)
The most common explanation is that during a revision of Kodak’s instructions for its gray cards in 1977, the advice to open up an extra half stop was omitted, and a whole generation of shooters grew up thinking that a measurement off a gray card could be used as-is. Kodak restored the proviso in 1997 during the next update of the instructions but by then it was too late.
The light meters built into your 90D are calibrated at the factory. But if you use a handheld incident or reflective light meter, you can calibrate it, using the instructions supplied with your meter. Because a handheld meter can be calibrated to the 18 percent gray standard (or any other value you choose), my rant about the myth of the 18 percent gray card doesn’t apply.
Another essential concept when discussing exposure, ISO control allows you to change the sensitivity of the camera’s imaging sensor. Sometimes photographers forget about this option, because the common practice is to set the ISO once for a particular shooting session (say, at ISO 100 or 200 for bright sunlight outdoors, or ISO 800 or 1600 when shooting indoors) and then forget about ISO. Or some shooters simply leave the camera set to ISO Auto. That enables the camera to change the ISO it deems necessary, setting a low ISO in bright conditions or a higher ISO in a darker location. That’s fine, but sometimes you’ll want to set a specific ISO yourself. That will be essential sometimes, since ISO Auto cannot set the highest ISO levels that are available when you use manual ISO selection.
TIPWhen shooting in the Program (P), Aperture-priority (Av), and Shutter-priority (Tv) modes, all discussed soon, changing the ISO does not change the exposure. If you switch from using ISO 100 to ISO 1600 in Av mode, for example, the camera will simply set a different shutter speed. If you change the ISO in Tv mode, the camera will set a different aperture, and in P mode, it will set a different aperture and/or shutter speed. In all of these examples, the camera will maintain the same exposure. If you want to make a brighter or a darker photo in P, Av, or Tv mode, you will need to set + or – exposure compensation, as discussed later.
However, when you use the Manual (M) mode, changing the ISO also changes the exposure, as discussed shortly.
The camera provides the best possible image quality in the ISO 100 to 400 range. We use higher ISO levels such as ISO 1600 in low light and ISO 6400 in a very dark location because it allows us to shoot at a faster shutter speed. That’s often useful for minimizing the risk of blurring caused by camera shake, which can occur even with lenses that include image stabilization (IS). And, of course, you must also contend with movement of the subject, which no amount of image stabilization will fix.
Although you can set a desired ISO level yourself, the 90D also offers an ISO Auto option. When enabled, the camera will select an ISO that should be suitable for the conditions: a low ISO on a sunny day and a high ISO in a dark location.
Over the past few years, there has been something of a competition among the manufacturers of digital cameras to achieve the highest ISO ratings. The highest announced ISO numbers have been rising annually, from 1600 to 3200 and 6400; a few cameras even allow you to choose a sensitivity setting that tops 3.2 million. Canon is a bit more conservative, but the 90D offers all the ISO options you’re ever likely to need, up to 25600, expandable to H, the equivalent of ISO 51200. Obviously, the loftiest numbers come at the cost of increased contrast and grain.
To calculate exposure automatically, you need to tell the 90D where in the frame to measure the light (this is called the metering method) and what controls should be used (aperture, shutter speed, or both) to set the exposure. That’s called exposure mode and includes Program (P), Shutter-priority (Tv), Aperture-priority (Av), or Manual (M) options, plus Auto and Creative Auto. I’ll explain all these next.
But first, I’m going to introduce you to the four metering methods. You can select any of the four if you’re working with P, Tv, Av, or M exposure modes; if you’re using Auto or Creative Auto, Evaluative metering is selected automatically and cannot be changed.
In either case, the individual zones used are linked to the autofocus points currently in use. The camera evaluates the data, giving extra emphasis to the metering zones that indicate sharp focus to make an educated guess about what kind of picture you’re taking, based on examination of thousands of different real-world photos. For example, if the top sections of a picture are much lighter than the bottom portions, the algorithm can assume that the scene is a landscape photo with lots of sky.
You’ll find four Creative Zone methods for choosing the appropriate shutter speed and aperture: Program (P), Shutter-priority (Tv), Aperture-priority (Av), and Manual (M). To select one of these modes, just spin the Mode Dial (located at the top-left side of the camera) to choose the method you want to use. You can also select from the Basic Zone exposure methods, which provide much less control.
Your choice of which exposure method is best for a given shooting situation will depend on things like your need for lots of (or less) depth-of-field, a desire to freeze action or allow motion blur, or how much noise you find acceptable in an image. Each of the 90D’s exposure methods emphasizes one of those aspects of image capture or another. This section introduces you to all of them.
When using Basic Zone modes, you have little control over exposure. In any of these modes, the 90D sets Evaluative metering for you, and chooses the shutter speed and aperture automatically. Indeed, when using Scene modes, you can’t change any of the other shooting settings (other than image quality).
In Scene Intelligent Auto mode, the 90D selects an appropriate ISO sensitivity setting, color (white) balance, Picture Style, color space, noise reduction features, and use of the Auto Lighting Optimizer. (All of these will be discussed in Chapter 7.)
In Av mode, you specify the lens opening used, and the 90D selects the shutter speed. Aperture-priority is especially good when you want to use a particular lens opening to achieve a desired effect. Perhaps you’d like to use the smallest f/stop possible to maximize depth-of-field in a close-up picture. Or you might want to use a large f/stop to throw everything except your main subject out of focus, as in Figure 4.9. Maybe you’d just like to “lock in” a particular f/stop smaller than the maximum aperture because it’s the sharpest available aperture with that lens. Or, you might prefer to use, say, f/2.8 on a lens with a maximum aperture of f/1.4, because you want the best compromise between speed and sharpness.
Aperture-priority can even be used to specify a range of shutter speeds you want to use under varying lighting conditions, which seems almost contradictory. But think about it. You’re shooting a soccer game outdoors with a telephoto lens and want a relatively high shutter speed, but you don’t care if the speed changes a little should the sun duck behind a cloud. Set your 90D to Av, and adjust the aperture until a shutter speed of, say, 1/1000th second is selected at your current ISO setting. (In bright sunlight at ISO 400, that aperture is likely to be around f/11.) Then, go ahead and shoot, knowing that your 90D will maintain that f/11 aperture (for sufficient DOF as the soccer players move about the field), but will drop down to 1/750th or 1/500th second if necessary should the lighting change a little.
A blinking 30 or 8000 in the viewfinder indicates that the 90D is unable to select an appropriate shutter speed at the selected aperture and that over- and underexposure will occur at the current ISO setting. That’s the major pitfall of using Av: you might select an f/stop that is too small or too large to allow an optimal exposure with the available shutter speeds. For example, if you choose f/2.8 as your aperture and the illumination is quite bright (say, at the beach or in snow), even your camera’s fastest shutter speed might not be able to cut down the amount of light reaching the sensor to provide the right exposure. Or, if you select f/8 in a dimly lit room, you might find yourself shooting with a very slow shutter speed that can cause blurring from subject movement or camera shake. Aperture-priority is best used by those with a bit of experience in choosing settings. Many seasoned photographers leave their 90D set on Av all the time.
When to use Aperture-priority:
If you use Av mode and select an aperture like f/11 or f/16, it’s your responsibility to make sure the shutter speed selected is fast enough to avoid losing detail to camera shake, or that the 90D is mounted on a tripod. One thing that new landscape photographers fail to account for is the movement of distant leaves and tree branches. When seeking the ultimate in sharpness, go ahead and use Aperture-priority, but boost ISO sensitivity a bit, if necessary, to provide a sufficiently fast shutter speed, whether shooting handheld or with a tripod.
Shutter-priority (Tv) is the inverse of Aperture-priority: you choose the shutter speed you’d like to use, and the camera’s metering system selects the appropriate f/stop. Perhaps you’re shooting action photos and you want to use the absolute fastest shutter speed available with your camera; in other cases, you might want to use a slow shutter speed to add some blur to a ballet photo that would be mundane if the action were completely frozen. Shutter-priority mode gives you some control over how much action-freezing capability your digital camera brings to bear in a particular situation, as you can see in Figure 4.10.
You’ll also encounter the same problem as with Aperture-priority when you select a shutter speed that’s too long or too short for correct exposure under some conditions. I’ve shot outdoor soccer games on sunny fall evenings and used Shutter-priority mode to lock in a 1/1000th second shutter speed, which triggered the blinking warning, even with the lens wide open.
Like Av mode, it’s possible to choose an inappropriate shutter speed. If that’s the case, the maximum aperture of your lens (to indicate underexposure) or the minimum aperture (to indicate overexposure) will blink.
When to use Shutter-priority:
Program mode (P) uses the 90D’s built-in smarts to select the correct f/stop and shutter speed using a database of picture information that tells it which combination of shutter speed and aperture will work best for a particular photo. If the correct exposure cannot be achieved at the current ISO setting, the shutter speed or aperture indicator in the viewfinder will blink, indicating under- or overexposure. You can then boost or reduce the ISO to increase or decrease sensitivity.
The 90D’s recommended exposure can be overridden if you want. Use the EV setting feature (described later, because it also applies to Tv and Av modes) to add or subtract exposure from the metered value. And, as I mentioned earlier in this chapter, you can change from the recommended setting to an equivalent setting (as shown in Table 4.1) that produces the same exposure, but using a different combination of f/stop and shutter speed. To accomplish this:
Your adjustment remains in force for a single exposure; if you want to change from the recommended settings for the next exposure, you’ll need to repeat those steps.
When to use Program mode priority:
Part of being an experienced photographer comes from knowing when to rely on your 90D’s automation (including Scene Intelligent Auto or P mode), when to go semi-automatic (with Tv or Av), and when to set exposure manually (using M). Some photographers actually prefer to set their exposure manually, as the 90D will be happy to provide an indication of when its metering system judges your settings provide the proper exposure, using the analog exposure scale at the bottom of the view-finder and on the status LCD.
Manual exposure can come in handy in some situations. You might be taking a silhouette photo and find that none of the exposure modes or EV correction features give you exactly the effect you want. For example, when I photographed the sunset shot in Figure 4.11, there was no way any of my 90D’s exposure modes would be able to interpret the scene the way I wanted to shoot it, even with Spot metering, which didn’t have a narrow enough field-of-view from my position. So, I took a couple test exposures, and set the exposure manually using the exact shutter speed and f/stop I needed. You might be working in a studio environment using multiple flash units. The additional flash are triggered by slave devices (gadgets that set off the flash when they sense the light from another flash, or, perhaps from a radio or infrared remote control). Your camera’s exposure meter doesn’t compensate for the extra illumination, and can’t interpret the flash exposure at all, so you need to set the aperture manually.
Depending on your proclivities you might not need to set exposure manually very often, but you should still make sure you understand how it works. Fortunately, the 90D makes setting exposure manually very easy. Just set the Mode Dial to M, turn the Main Dial to set the shutter speed, and rotate the Quick Control Dial to adjust the aperture. Press the shutter release halfway or press the AE lock button, and the exposure scale in the viewfinder shows you how far your chosen setting diverges from the metered exposure.
When to use Manual exposure:
Another way of adjusting exposures is by changing the ISO sensitivity setting. Sometimes photographers forget about this option, because the common practice is to set the ISO once for a particular shooting session (say, at ISO 100 or 200 for bright sunlight outdoors, or ISO 800 when shooting indoors) and then forget about ISO. ISOs higher than ISO 100 or 200 are seen as “bad” or “necessary evils.” However, changing the ISO is a valid way of adjusting exposure settings, particularly with the Canon EOS 90D, which produces good results at ISO settings that create grainy, unusable pictures with some other camera models.
Indeed, I find myself using ISO adjustment as a convenient alternate way of adding or subtracting EV when shooting in Manual mode, and as a quick way of choosing equivalent exposures when in Auto or semi-automatic modes. For example, I’ve selected a Manual exposure with both f/stop and shutter speed suitable for my image using, say, ISO 200. I can change the exposure in full-stop increments by pressing the ISO button on top of the camera and spinning the Main Dial one click at a time. Rotating to the right increases the ISO sensitivity; to the left reduces it; and spinning all the way to the left selects Auto ISO. The difference in image quality/noise at the base setting of ISO 200 is negligible if I dial in ISO 100 to reduce exposure a little or change to ISO 400 to increase exposure. I keep my preferred f/stop and shutter speed, but still adjust the exposure.
Or, perhaps, I am using Tv mode and the metered exposure at ISO 200 is 1/500th second at f/11. If I decide on the spur of the moment, I’d rather use 1/500th second at f/8, I can press the ISO button and spin the Main Dial to switch to ISO 100. Of course, it’s a good idea to monitor your ISO changes, so you don’t end up at ISO 25600 accidentally. ISO settings can, of course, also be used to boost or reduce sensitivity in particular shooting situations. The 90D can use ISO settings from ISO 100 up to 1600. You can also activate ISO expansion in the ISO Speed Settings entry of the Shooting 2 menu (as described in Chapter 7) to enable settings up to H (ISO 25600 equivalent).
With the 90D, Canon has given you a great deal of control over the ISO settings available for manual or automatic selection:
You can select Auto for shutter speed selection; press SET and then rotate the Main Dial to choose Slower (up to –3) or Faster (up to +3). At the middle (0) value, the minimum shutter speed will be the reciprocal of the lens focal length, i.e., 1/30th second with a 30mm zoom setting. Each value plus or minus 1 to 3 specifies a shutter speed one stop faster or slower, respectively.
Choose Manual, instead, and you can select a minimum shutter speed from 1 second to 1/8000th second using the Main Dial.
When ISO Auto is enabled, the camera can adjust the ISO automatically as appropriate for various lighting conditions. In Basic Zone modes, ISO is normally set between ISO 100 and ISO 6400, except in Landscape mode, where only ISO 100 to ISO 1600 is used, and Handheld Night Scene mode, which uses ISO 100 to ISO 12800.
When using flash, Auto ISO produces a setting of ISO 400 automatically, except when overexposure would occur (as when shooting subjects very close to the camera), in which case a lower setting (down to ISO 100) will be used. If you have an external dedicated flash attached, the 90D can set ISO in the range of 400 to 1600 automatically when using Creative Auto, Portrait, Landscape, Close-Up, Sports, or P exposure modes. That capability can be useful when shooting outdoor field sports at night and other “long distance” flash pictures, particularly with a telephoto lens, because you want to extend the “reach” of your external flash as far as possible (to dozens of feet or more), and boosting the ISO does that. Remember that if the Auto ISO ranges aren’t suitable for you, individual ISO values can also be selected in any of the Creative Zone modes.
TIPFind yourself locked out of ISO settings lower than 200 or higher than 12800? You’ve probably set Highlight Tone Priority to Enable in the Shooting 2 menu, as described in Chapter 7.
Visual image noise is that random grainy effect that some like to use as a special effect, but which, most of the time, is objectionable because it robs your image of detail even as it adds that “interesting” texture. Noise is caused by two different phenomena: high ISO settings and long exposures.
High ISO noise commonly first appears when you raise your camera’s sensitivity setting above ISO 800. With Canon cameras, which are renowned for their good ISO noise characteristics, noise may become visible at ISO 1600, and it is usually fairly noticeable at ISO 3200. At the H setting (ISO 25600 equivalent), noise is usually quite bothersome, which is why that lofty sensitivity rating is disabled by default and must be activated using an option in the ISO Speed Settings entry of the Shooting 2 menu (discussed again in Chapter 7). This kind of noise appears as a result of the amplification needed to increase the sensitivity of the sensor. While higher ISOs do pull details out of dark areas, they also amplify non-signal information randomly, creating noise.
A similar noisy phenomenon occurs during long time exposures, which allow more photons to reach the sensor, increasing your ability to capture a picture under low-light conditions. However, the longer exposures also increase the likelihood that some pixels will register random phantom photons, often because the longer an imager is “hot,” the warmer it gets, and that heat can be mistaken for photons. There’s also a special kind of noise that CMOS sensors like the one used in the 90D are potentially susceptible to. With a CCD, the entire signal is conveyed off the chip and funneled through a single amplifier and analog-to-digital conversion circuit. Any noise introduced there is, at least, consistent. CMOS imagers, on the other hand, contain millions of individual amplifiers and A/D converters, all working in unison. Because all these circuits don’t necessarily process in precisely the same way all the time, they can introduce something called fixed-pattern noise into the image data.
Fortunately, Canon’s electronics geniuses have done an exceptional job minimizing noise from all causes in the 90D. Even so, you might still want to apply the optional long exposure noise reduction. This type of noise reduction involves the 90D taking a second, blank exposure, and comparing the random pixels in that image with the photograph you just took. Pixels that coincide in the two represent noise and can safely be suppressed. This noise reduction system, called dark frame subtraction, effectively doubles the amount of time required to take a picture, and is used only for exposures longer than one second. Noise reduction can reduce the amount of detail in your picture, as some image information may be removed along with the noise. So, you might want to use this feature with moderation. Some types of images don’t require noise reduction, because the grainy pattern tends to blend into the overall scene.
To activate your 90D’s long exposure noise reduction features, go to the Shooting 4 menu, as explained further in Chapter 7.
You can also apply noise reduction to a lesser extent using Photoshop, and when converting RAW files to some other format, using your favorite RAW converter, or an industrial-strength product like Noise Ninja (www.picturecode.com) to wipe out noise after you’ve already taken the picture.
Sometimes you’ll want more or less exposure than indicated by the 90D’s metering system. Perhaps you want to underexpose to create a silhouette effect or overexpose to produce a high-key look. It’s easy to use the 90D’s Exposure Compensation system to override the exposure recommendations, available in any Creative Zone mode except Manual. There are two ways to make exposure value (EV) changes with the 90D. One method is fast but limited to display of plus/minus three stops of compensation. The second method is slower but allows setting up to 5 stops of compensation in either 1/3- or full-stop increments.
Activate the exposure meters by tapping the shutter release button. Then, rotate the QCD while looking through the viewfinder or at the back-panel LCD monitor when the Quick Control screen is visible (press the INFO. button to cycle to it, if necessary). Spin to the right to make the image brighter (add exposure), and to the left to make the image darker (subtract exposure). The exposure scale in the viewfinder and on the LCD indicates the EV change you’ve made. The EV change you’ve made remains for the exposures that follow, until you manually zero out the EV setting with the AV button + Main Dial. EV changes are ignored when using M or any of the Basic Zone modes. (If you’re unable to make an adjustment, you may have set the Lock switch to the locked position. Rotate it downward to reactivate the Quick Control Dial.)
You can also use the second method for making EV changes with the 90D. It can be a little slower but allows you to set up to plus/minus five stops of adjustment. You also have the option of setting exposure bracketing at the same time:
Bracketing is a method for shooting several consecutive exposures using different settings, as a way of improving the odds that one will be exactly right. Before digital cameras took over the universe, it was common to bracket exposures, shooting, say, a series of three photos at 1/125th second, but varying the f/stop from f/8 to f/11 to f/16. In practice, smaller than whole-stop increments were used for greater precision. Plus, it was just as common to keep the same aperture and vary the shutter speed, although in the days before electronic shutters, film cameras often had only whole increment shutter speeds available. Figure 4.14 shows a typical bracketed series.
Today, cameras like the 90D can bracket exposures much more precisely, and bracket white balance as well (using the WB Shift/Bkt entry found in the Shooting 3 menu and described in Chapter 7). While WB bracketing is sometimes used when getting color absolutely correct in the camera is important, autoexposure bracketing (AEB) is used much more often. When this feature is activated, the 90D takes three (and only three) consecutive bracketed photos (immediately if continuous shooting is enabled; otherwise, one at a time as you press the shutter release). It takes one photo at the metered “correct” exposure, one with less exposure, and one with more exposure, using an increment of your choice up to plus 2/minus 2 stops. (Choose between increments by setting Custom Function (C.Fn) I-1 to 0 [1/3 stop] or 1 [1/2 stop].) In Av mode, the shutter speed will change, while in Tv mode, the aperture will change.
The final relevant entry in the C.Fn I: Exposure menu is 3: Bracketing Auto Cancel. When you activate bracketing (in the Shooting 2 menu, described shortly), the 90D continues to shoot bracketed exposures until you manually turn the bracket feature off, assuming you have this setting disabled. That’s a good thing. If you’re out shooting a series of bracketed exposures (especially for HDR), it’s convenient to have your bracket setting be “sticky” and still be active even if you turn your camera off. Some shooters like to bracket virtually everything and like to leave bracketing on routinely.
However, much of the time you’ll want to turn bracketing off, and you may not want to visit the Shooting 2 menu to deactivate it manually. Set Bracketing Auto Cancel to On, and bracketing is cancelled when you turn the 90D off, change lenses, use the flash, or change memory cards. When this setting is set to Off, bracketing remains in effect until you manually turn it off or use the flash. The flash still cancels bracketing, but your settings are retained.
Also in the Custom Function menu, you’ll find the C.Fn I-4: Bracketing Sequence entry, which allows you to specify the order in which the autoexposure bracketing series are exposed. Your choice will depend both on personal preference, and what you intend to do with the bracketed shots. The options include:
The C.Fn I-5: Number of Bracketed Shots entry allows you to elect to bracket 2, 3, 5, or 7 shots:
You can choose the size of the jump between each of the bracketed exposures. To do that, you’ll need to visit the Expo. Comp/AEB entry in the Shooting 2 menu. There, you can select from plus/minus 1/3 to 3 full stops in 1/3-stop increments, by rotating the Main Dial. The next section provides instructions for producing a bracketed set.
Using AEB is trickier than it needs to be, but it has been made more flexible than it was with earlier models. With the 90D you can now choose to bracket only overexposures or underexposures—a very useful improvement! Just follow these steps:
When the three bracket indicators aren’t separated, using the left/right multi-controller buttons simply, in effect, adds or subtracts exposure compensation. You’ll be shooting a “bracketed” set of one picture, with the zero point placed at the portion of the scale you indicated. Until you rotate the Main Dial to separate the three bracket indicators by at least one indicator, this screen just supplies EV adjustment. Also keep in mind that the increments shown will be either 1/3 stop or 1/2 stop, depending on how you’ve set C.Fn I-1.
NOTEAEB is disabled when you’re using Multi Shot Noise Reduction, taking long time exposures with the Bulb setting, or have enabled the Auto Lighting Optimizer in the Shooting 2 menu (in which case the optimizer will probably override and nullify bracketing).
High dynamic range (HDR) photography is quite the rage these days, and entire books have been written on the subject. It’s not really a new technique—film photographers have been combining multiple exposures for ages to produce a single image of, say, an interior room while maintaining detail in the scene visible through the windows.
Suppose you wanted to photograph a dimly lit room that had a bright window showing an outdoors scene. Proper exposure for the room might be on the order of 1/60th second at f/2.8 at ISO 200, while the outdoors scene probably would require f/11 at 1/400th second. That’s almost a 7 EV step difference (approximately 7 f/stops) and well beyond the dynamic range of any digital camera, including the Canon 90D.
Until camera sensors gain much higher dynamic ranges (which may not be as far into the distant future as we think), special tricks like Highlight Tone Priority and HDR photography will remain basic tools. With the Canon 90D, you can create in-camera HDR exposures, or shoot HDR the old-fashioned way—with separate bracketed exposures that are later combined in a tool like Photomatix, the Nik HDR Efex Pro 2 (part of DxO’s Nik Collection), or Adobe’s Merge to HDR Pro image-editing feature. I’m going to show you how to use both methods.
Here are some tips for using this built-in feature, found in the Shooting 3 menu:
Access HDR mode from the Shooting 4 menu, and you’ll be taken to a menu with four entries:
The 90D’s in-camera HDR Backlight Control feature, available as a Special Scene option when the Mode Dial is in the SCN position, is simple, not particularly flexible, but still surprisingly effective in creating high dynamic range images. It’s also remarkably easy to use. It combines three images to create a single HDR photograph, and it’s not as effective as the HDR mode feature already discussed, or as powerful as the manual HDR method I’ll describe in the section after this one.
Figure 4.16 shows you a typical situation in which you might want to use this setting. When the exposure is set for the interior of the cathedral, the beautiful backlit stained-glass windows (top left) are washed out and have no detail. When the exposure is adjusted to produce detail in the glass panes (top right), the rest of the cathedral goes dark. The quickie solution is to use the 90D’s HDR Backlight Control. It captures three consecutive images, including similar to the two at top, plus a third with an exposure between the two, and then merges them to preserve both highlight and shadow detail, as you can see at bottom in the figure, which has a much fuller range of tones.
Here are some tips for using this feature (these also apply to the Handheld Night Scene mode, which also merges multiple shots to create a single improved image):
Creating HDR images manually is not difficult. You simply shoot individual images either by manually bracketing or using the camera’s auto bracketing modes, described earlier in this chapter.
Although my goal in this book is to show you how to take great photos in the camera rather than how to fix your errors in Photoshop, the Merge to HDR Pro feature in Adobe’s flagship image editor (and a variation also found in Photoshop Elements) is too cool to ignore. The ability to have a bracketed set of exposures that are identical except for exposure is key to getting good results with this Photoshop feature, which allows you to produce images with a full, rich dynamic range that includes a level of detail in the highlights and shadows that is almost impossible to achieve with digital cameras.
When you’re using Merge to HDR Pro, you’d take several pictures, some exposed for the shadows, some for the middle tones, and some for the highlights. The exact number of images to combine is up to you. Four to seven is a good number. Then, you’d use the Merge to HDR Pro command to combine all the images into one HDR image that integrates the well-exposed sections of each version. Here’s how.
The images should be as identical as possible, except for exposure. So, it’s a good idea to mount the camera on a tripod, use a remote release, and take all the exposures in one burst. Just follow these steps:
You can use auto bracketing or manually change the exposure between shots. In Manual mode, make sure Auto ISO is off, and you adjust exposures only by changing the shutter speed. You should be very careful when you make the adjustment to avoid jostling the camera.
How do you choose the number of EV/stops to separate your exposures? You can use histograms, described at the end of this chapter, to determine the correct bracketing range. Take a test shot and examine the histogram. Reduce the exposure until dark tones are clipped off at the left of the resulting histogram. Then, increase the exposure until the lighter tones are clipped off at the right of the histogram. The number of stops between the two is the range that should be covered using your bracketed exposures. Note that if you want to override the +/- 3-stop limitation of auto bracketing, you can add or subtract exposure compensation. That will bias the exposures in the direction you choose. For example, if autobracketing in Aperture-priority mode would produce exposures of 1/125th, 1/250th, and 1/500th second, you can set EV to –2 and get 1/30th, 1/60th, and 1/125th second exposures instead.
The next steps show you how to combine the separate exposures into one merged high dynamic range image.
If you do everything correctly, you’ll end up with a full-range high dynamic range photo, like the one shown at right in Figure 4.17. What if you don’t have the opportunity, inclination, or skills to create several images at different exposures, as described? If you shoot in RAW format, you can still use Merge to HDR, working with a single original image file. What you do is import the image into Photoshop several times, using Adobe Camera Raw to create multiple copies of the file at different exposure levels.
For example, you’d create one copy that’s too dark, so the shadows lose detail, but the highlights are preserved. Create another copy with the shadows intact and allow the highlights to wash out. Then, you can use Merge to HDR to combine the two and end up with a finished image that has the extended dynamic range you’re looking for. (This concludes the image-editing portion of the chapter. We now return you to our alternate sponsor: photography.)
Your 90D’s histograms are a simplified display of the numbers of pixels at each of 256 brightness levels, producing an interesting mountain range effect. As I mentioned in Chapter 3, the 90D lets you designate either an RGB version or brightness-only version of the histogram as your “main” histogram display, using the Histogram Display entry in the Playback 3 menu, and shown in Figure 4.18. Or you can display both types at once, as seen in Figure 4.19, by scrolling down in the main histogram display screen using the up/down directional controls. The 90D also provides an optional “live” histogram on the screen as you frame and shoot when using Live View mode.
Although your camera may offer separate charts for brightness and the red, green, and blue channels, when you first start using histograms, you’ll want to concentrate on the brightness histogram, which represents a composite of all red, green, and blue tones using a white histogram. Each vertical line in the graph represents the number of pixels in the image for each brightness value, from 0 (black) on the left to 255 (white) on the right. The vertical axis measures that number of pixels at each level.
Histograms help you adjust the tonal range of an image, the span of dark to light tones, from a complete absence of brightness (black) to the brightest possible tone (white), and all the middle tones in between. Because all values for tones fall into a continuous spectrum between black and white, it’s easiest to think of a photo’s tonality in terms of a black-and-white or grayscale image, even though you’re capturing those tones in three separate color layers of red, green, and blue.
Because your images are digital, the tonal “spectrum” isn’t really continuous: it’s divided into discrete steps that represent the different tones that can be captured. Figure 4.20 may help you understand this concept. The gray steps shown range from 100 percent gray (black) at the left, to 0 percent gray (white) at the right, with 20 gray steps in all (plus white).
Along the bottom of the chart are the digital values from 0 to 255 recorded by your sensor for an image with 8 bits per channel. (8 bits of red, 8 bits of green, and 8 bits of blue equal a 24-bit, full-color image). Any black captured would be represented by a value of 0, the brightest white by 255, and the midtones would be clustered around the 128 marker. The actual scale may be “finer” and record say, 0 to 4,094 for an image captured when the 90D is capturing RAW images with 14 bits per channel.
Grayscale images (which we call black-and-white photos) are easy to understand. Or, at least, that’s what we think. When we look at a black-and-white image, we think we’re seeing a continuous range of tones from black to white, and all the grays in between. But that’s not exactly true. The blackest black in any photo isn’t a true black, because some light is always reflected from the surface of the print, and if viewed on a screen, the deepest black is only as dark as the least-reflective area a computer monitor can produce. The whitest white isn’t a true white, either, because even the lightest areas of a print absorb some light (only a mirror reflects close to all the light that strikes it), and, when viewing on a computer monitor, the whites are limited by the brightness of the display’s LCD or LED picture elements. Lacking darker blacks and brighter, whiter whites, that continuous set of tones doesn’t cover the full grayscale tonal range.
The full scale of tones becomes useful when you have an image that has large expanses of shades that change gradually from one level to the next, such as areas of sky, water, or walls. Think of a picture taken of a group of campers around a campfire. Since the light from the fire is striking them directly in the face, there aren’t many shadows on the campers’ faces. All the tones that make up the features of the people around the fire are compressed into one end of the brightness spectrum—the lighter end.
Yet, there’s more to this scene than faces. Behind the campers are trees, rocks, and perhaps a few animals that have emerged from the shadows to see what is going on. These are illuminated by the softer light that bounces off the surrounding surfaces. If your eyes become accustomed to the reduced illumination, you’ll find that there is a wealth of detail in these shadow images.
This campfire scene would be a nightmare to reproduce faithfully under any circumstances. If you are an experienced photographer, you are probably already wincing at what is called a high-contrast lighting situation. Some photos may be high in contrast when there are fewer tones and they are all bunched up at limited points in the scale. In a low-contrast image, there are more tones, but they are spread out so widely that the image looks flat. Your digital camera can show you the relationship between these tones using a histogram.
As I mentioned earlier, your 90D’s histograms are a simplified display of the numbers of pixels at each of 256 brightness levels. Although separate charts may be provided for brightness and the red, green, and blue channels, when you first start using histograms, you’ll want to concentrate on the brightness histogram.
Each vertical line in the graph represents the allocation of pixels in the image for each brightness value, from 0 (black) on the left to 255 (white) on the right. Although histograms are most often used to fine-tune exposure, you can glean other information from them, such as the relative contrast of the image. Figure 4.21, top, is a simplified rendition of a histogram of an image having normal contrast. In such an image, most of the pixels are spread across the image, with a healthy distribution of tones throughout the midtone section of the graph. That large peak at the right side of the graph represents all those light tones in the sky. A normal-contrast image you shoot may have less sky area, and less of a peak at the right side, but notice that very few pixels hug the right edge of the histogram, indicating that the lightest tones are not being clipped because they are off the chart.
With a lower-contrast image, like the one shown in Figure 4.21, center, the basic shape of the previous histogram will remain recognizable, but gradually will be compressed together to cover a smaller area of the gray spectrum. The squished shape of the histogram is caused by all the grays in the original image being represented by a limited number of gray tones in a smaller range of the scale.
Instead of the darkest tones of the image reaching into the black end of the spectrum and the whitest tones extending to the lightest end, the blackest areas of the scene are now represented by a light gray, and the whites by a somewhat lighter gray. The overall contrast of the image is reduced. Because all the darker tones are actually a middle gray or lighter, the scene in this version of the photo appears lighter as well.
Going in the other direction, increasing the contrast of an image produces a histogram like the one shown in Figure 4.21, bottom. In this case, the tonal range is now spread over the entire width of the chart, but, except for the bright sky, there is not much variation in the middle tones; the mountain “peaks” are not very high. When you stretch the grayscale in both directions like this, the darkest tones become darker (that may not be possible) and the lightest tones become lighter (ditto). In fact, shades that might have been gray before can change to black or white as they are moved toward either end of the scale.
The effect of increasing contrast may be to move some tones off either end of the scale altogether, while spreading the remaining grays over a smaller number of locations on the spectrum. That’s exactly the case in the example shown. The number of possible tones is smaller, and the image appears harsher.
The important thing to remember when working with the histogram display in your 90D is that changing the exposure does not change the contrast of an image. The curves illustrated in the previous three examples remain exactly the same shape when you increase or decrease exposure. I repeat: The proportional distribution of grays shown in the histogram doesn’t change when exposure changes; it is neither stretched nor compressed. However, the tones as a whole are moved toward one end of the scale or the other, depending on whether you’re increasing or decreasing exposure. You’ll be able to see that in some illustrations that follow.
So, as you reduce exposure, tones gradually move to the black end (and off the scale), while the reverse is true when you increase exposure. The contrast within the image is changed only to the extent that some of the tones can no longer be represented when they are moved off the scale.
To change the contrast of an image, you must do one of four things:
Of the four of these, the third—changing the contrast of the scene—is the most desirable, because attempting to fix contrast by fiddling with the tonal values is unlikely to be a perfect remedy. However, adding a little contrast can be successful because you can discard some tones to make the image more contrasty. However, the opposite is much more difficult. An overly contrasty image rarely can be fixed, because you can’t add information that isn’t there in the first place.
What you can do is adjust the exposure so that the tones that are already present in the scene are captured correctly. Figure 4.22, top, shows the histogram for an image that is badly underexposed. You can guess from the shape of the histogram that many of the dark tones to the left of the graph have been clipped off. There’s plenty of room on the right side for additional pixels to reside without having them become overexposed. So, you can increase the exposure (either by changing the f/stop or shutter speed or by adding an EV value) to produce the corrected histogram shown in Figure 4.22, center.
Conversely, if your histogram looks like the one shown in Figure 4.22, bottom, with bright tones pushed off the right edge of the chart, you have an overexposed image, and you can correct it by reducing exposure. In addition to the histogram, the 90D has its Highlights and Zebra options, which, when activated, shows areas that are overexposed with flashing tones (often called “blinkies”). Depending on the importance of this “clipped” detail, you can adjust exposure or leave it alone. For example, if all the dark-coded areas in the review are in a background that you care little about, you can forget about them and not change the exposure, but if such areas appear in facial details of your subject, you may want to make some adjustments.
In working with histograms, your goal should be to have all the tones in an image spread out between the edges, with none clipped off at the left and right sides. Underexposing (to preserve highlights) should be done only as a last resort, because retrieving the underexposed shadows in your image editor will frequently increase the noise, even if you’re working with RAW files. A better course of action is to expose for the highlights, but, when the subject matter makes it practical, fill in the shadows with additional light, using reflectors, fill flash, or other techniques rather than allowing them to be seriously underexposed.
A traditional technique for optimizing exposure is called “expose to the right” (ETTR), which involves adding exposure to push the histogram’s curve toward the right side but not far enough to clip off highlights. The rationale for this method is that extra shadow detail will be produced with a minimum increase in noise, especially in the shadow areas. It’s said that half of a digital sensor’s response lies in the brightest areas of an image, and so require the least amount of amplification (which is one way to increase digital noise). ETTR can work, as long as you’re able to capture a satisfactory amount of information in the shadows.
It’s easier to understand exposing to the right if you mentally divide the histogram into fifths. And, for the sake of simplicity and smaller numbers, assume you’re shooting in 14-bit RAW. Any 14-bit image can record a maximum of 16,383 different tones per channel. However, each fifth of the histogram does not encompass 3,277 tones (one-fifth of 16,383).
Instead, the right-most fifth, the highlights, shown in Figure 4.23, accounts for fully half, or 50 percent of the tones; the next fifth accounts for 1/4 (25 percent); and so on, with 1/8th, 1/16th, and 1/32nd assigned to the remaining fifths. These “fifths” are fuzzy rather than hard boundaries. But note that in the left-most area, approximately only 512 different tones are captured. When processing your RAW file, there are only 512 tones to recover in the shadows, which is why boosting/amplifying them increases noise. (The effect is most noticeable in the red and blue channels; your sensor’s Bayer array has twice as many green-sensitive pixels as red or blue.)
To expose to the right, you want to add exposure—as long as you don’t push highlights off the right edge of the histogram—to brighten the shadows. Because there are approximately 8,192 tones available in the highlights, even if the RAW image looks overexposed, it’s possible to use your RAW converter’s Exposure slider (such as the one found in Adobe Camera Raw) to bring back detail captured in that surplus of tones in the highlights. This procedure is the exact opposite of what was recommended for film of the transparency variety—it was fairly easy to retrieve detail from shadows by pumping more light through them when processing the image, while even small amounts of extra exposure blew out highlights. You’ll often find that the range of tones in your image is so great that there is no way to keep your histogram from spilling over into the left and right edges, costing you both highlight and shadow detail. Exposing to the right may not work in such situations. A second school of thought recommends reducing exposure to bring back the highlights, or “exposing to the left.” You would then attempt to recover shadow detail in an image editor, using tools like Adobe Camera Raw’s Exposure slider. But remember, above all, that this procedure will also boost noise in the shadows, and so the technique should be used with caution. In most cases, exposing to the right is your best bet.
The more you work with histograms, the more useful they become. One of the first things that histogram veterans notice is that it’s possible to overexpose one channel even if the overall exposure appears to be correct. For example, flower photographers soon discover that it’s really, really difficult to get a good picture of a red rose. The exposure looks okay—but there’s no detail in the rose’s petals. (See Figure 4.24, left.) The image’s histogram will show you why: typically, you’ll find a peak at the right edge that indicates that highlight information has been lost. In fact, the green channel is often blown, too, and so the green parts of the flower also lack detail. Only the blue channel’s histogram may be entirely contained within the boundaries of the chart, and, on first glance, the white luminance histogram at top of the column of graphs may appear to be fairly normal.
Any of the primary channels—red, green, or blue—can blow out all by themselves, although bright reds seem to be the most common problem area. More difficult to diagnose are overexposed tones in one of the “in-between” hues on the color wheel. Overexposed yellows (which are very common) will be shown by blowouts in both the red and green channels. Too-bright cyans will manifest as excessive blue and green highlights, while overexposure in the red and blue channels reduces detail in magenta colors. As you gain experience, you’ll be able to see exactly how anomalies in the RGB channels translate into poor highlights and murky shadows.
The only way to correct for color channel blowouts is to reduce exposure. As I mentioned earlier, you might want to consider filling in the shadows with additional light to keep them from becoming too dark when you decrease exposure. In practice, you’ll want to monitor the red channel most closely, followed by the blue channel, and slightly decrease exposure to see if that helps. Because of the way our eyes perceive color, we are more sensitive to variations in green, so green channel blowouts are less of a problem, unless your main subject is heavily colored in that hue. If you plan on photographing a frog hopping around on your front lawn, you’ll want to be extra careful to preserve detail in the green channel, using bracketing or other exposure techniques outlined in this chapter.
The final factor in the exposure equation is one that your 90D offers little control over: Basic Zone modes. Your 90D includes Basic Zone shooting modes that can automatically make all the basic settings needed for certain types of shooting situations, such as Portraits, Landscapes, Close-ups, Sports, and Night Portraits. They are especially useful when you suddenly encounter a picture-taking opportunity and don’t have time to decide exactly which Creative Zone mode you want to use. Instead, you can spin the Mode Dial to Scene Intelligent Auto (with the green A+ icon), or to the SCN position, where you can choose an appropriate SCN mode, and fire away, knowing that at least you have a fighting chance of getting a good or usable photo.
Basic Zone modes are also helpful when you’re just learning to use your 90D. Once you’ve learned how to operate your camera, you’ll probably prefer one of the Creative Zone modes that provide more control over shooting options. The Basic Zone scene modes may give you few options or none at all. The AF mode, drive mode, and metering mode are all preset for you. However, you’ll see a screen that shows you which of the settings you can change. I’ll describe those options in the next section. For now, I’m going to tell you about each of the Basic Zone modes.
I’ve previously described how to use the Quick Control screen when working with Creative Zone modes, to change many settings, such as ISO, shutter speed, aperture, and other parameters. When using Basic Zone modes, your options are different. In each case, you can activate the Quick Control screen by pressing the Quick Control button. Then, one of several different screens will appear on your LCD. I’ll describe your options for the different modes next.
In this mode, autofocus, brightness, and color tones are set for you based on the particular Scene mode the camera selects. Press the Q button, and a screen appears that allows you to navigate to the Drive mode, Built-in Flash, and Creative Assist icons at the bottom. (See Figure 4.25.) Highlight one of these three parameters and press SET to make adjustments (in Live View, read the message and select OK to proceed):
Canon previously used the term Ambience for these settings in earlier EOS models, but switched to Creative Assist to avoid confusion with the more common term ambient light. In practice, this option allows you to apply changes to the look of your image in a variety of ways, ranging from brightness and contrast, richness of the colors, and amber/blue or green/magenta color bias. You can also adjust “background” blur, which is simply a way of saying varying the depth-of-field to make the background sharper or blurrier.
When you press the Q button, highlight Creative Assist, and press SET, a screen like the one shown in Figure 4.26 appears. Arrayed along the bottom are tabs labeled Preset, Background Blur, Brightness, Contrast, Saturation, Color Tone 1, Color Tone 2, and Monochrome (you must scroll right to see the settings after Contrast).
If you highlight Preset and press SET, you can select from 12 canned presets, plus any “User” settings you may have saved. These presets are something like the Picture Styles in the Shooting menu that I’ll describe in detail in Chapter 7.
If you want to bypass the presets and make your adjustments directly, just scroll past the Preset tab to highlight Background Blur, Brightness, Contrast, Saturation, Color Tone 1, Color Tone 2, and Monochrome. Note that with the Monochrome parameter, you can only choose Off, B/W, Sepia, Blue, Purple, or green. The other parameters are not available.
If you don’t store your settings using the Apply to Register option, any changes you make to Background Blur, Brightness, Contrast, Saturation, Color Tone 1, Color Tone 2, or Monochrome settings will be reset to their default values when you power down the 90D. If you’d like to retain them, say, temporarily (but don’t want to register them to one of the three USER slots), choose Enable/On in the Retain Creative Assist Data option in the version of the Shooting 2 menu that appears when the mode dial is set to the Auto+ position.
One useful feature of the 90D is the ability to apply Creative Filters to images as you take the picture. However, you can also apply these effects to images you’ve already taken using the Creative Filters entry in the Playback menu (as I’ll describe in Chapter 7). The advantage of applying the filters as you shoot is that you can preview their effect before shooting during live view; the advantage of applying them to a shot that you’ve already taken is that the modified image is saved alongside the original, which is not changed.
You can apply any of these Creative Filters when using the optical viewfinder (although you can’t preview the effects) and when shooting using live view. Just rotate the Mode Dial to the Creative Filters position, located between the SCN and C1 positions. Press the Q button, and you can scroll through a list that includes Grainy B/W, Soft Focus, Fish-eye, Water Painting, Toy Camera, Miniature Effect, and HDR Art (Standard, Vivid, Bold, and Art Embossed). Figure 4.30 shows four of the effects. I’ll explain the individual effects as they are applied after the photo is taken in additional detail in the discussion of Playback menu entries in Chapter 7.
When you highlight one of the effects and press SET, a screen with available adjustments for that effect appears. All of them, except the four HDR choices, allow you to specify Drive mode and Built-in Flash controls. (The HDR modes only allow Drive mode changes.)
Five of the choices allow you to modify the effect by pressing the up directional button and pressing left/right controls to increase/decrease parameters: Grainy B/W (Contrast), Soft Focus, Fish-eye (Strength of the effect), Water Painting (Color Density), and Toy Camera (Warm, Neutral, Cool color tone).
When you press the Q button when a Scene mode is active, you can change some combination of brightness, drive mode, built-in flash settings, or modify the Scene mode’s effect itself. Here are your options.
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