METERING, SENSITIVITY AND WHITE BALANCE
Metering, sensitivity and white balance are three key aspects of the way your image looks once you press the shutter button, irrespective of the focus, sharpness or number of pixels you throw at it. Here we will look at key components of the DSLR that make an image look right in terms of colour, image noise and exposure
Sensitivity
A camera’s ISO setting defi nes its sensitivity to light. The higher the ISO, the more sensitive it becomes and vice versa. But
a downside of higher sensitivities is the introduction of image noise (analogous to grain in fi lm) that can adversely affect a shot. Think of noise as interference, just like the ‘snow’ in a badly tuned TV picture. It appears because increasing sensitivity is actually turning up the gain on the sensor. Things that can affect noise include internal electrical interference from camera components, heat and the amount of light. The light is the good signal, everything else is noise, and hence a
good signal to noise ratio is important: the HIGH ISO more light the less noise. This is why noise
becomes more evident in
images, try to use the lowest possible setting for the shot at hand. Set it to ISO 100 or its lowest setting for best overall results. Set your camera’s noise reduction (it’ll be there in the
Here is a ready reckoner for the use of a particular ISO (sensitivity) and why, based upon typical DSLR sensitivity settings...
LOW ISO | MATRIX OR EVALUATIVE | |
These are many small (in some cases over | ||
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| 200) metering ‘zones’ around the frame that | |
| are used to intelligently assess and measure | |
| light from all locations within the frame (based | |
| on | |
| balanced exposure. This mode is ideal for | |
| general photography or broader subjects | |
| such as landscapes or subjects where there | |
| are no tricky | |
| CENTRE WEIGHTED | |
| A central portion of the frame (the size of this | |
| zone can be adjusted on some DSLRs) is | |
| ‘weighted’ to simply measure the average of | |
| light | |
| any adjustments. Ideal for where you want | |
| to bias the exposure to the central area, in | |
| backlit subjects for example. It’s also useful | |
| in that you can predict how it will react to a | |
| scene and when it will be fooled, so you can | |
| more easily compensate for it. | |
| SPOT | |
| A very small area of the frame | |
| frame, depending on the camera) that is ideal | |
| for measuring light from a very specifi c area | |
| in a scene. Ideal for macro | |
| or for portraits (metering from a skin tone) or | |
| for | |
| bright highlights/deep shadows (or meter | |
| from both and apply an average). |
White balance
Your DSLR offers a variety of White Balance (WB) or colour temperature settings to combat colour casts from differing light sources. Whether in menus or accessed via an external control it is not always a good idea to leave your camera set to its ‘Auto WB’ setting. The colours may not be rendered as accurately in a shot as needed. To help get the most from any shot, use the correct WB setting for the job at hand: daylight setting for daylight and so on. Moreover, if you are not sure, use the custom setting; DSLRs enable you to tailor the WB quickly and simply to any lighting type.
The typical settings available will include all or some of those set out in the box below, indicated using small icons, text or both. Some DSLRs have
ISO 100
Bright daylight, sunny conditions,
ISO 200
Where faster shutter speeds are required or slightly longer lenses, or where you need extra fl exibility with apertures/shutter speeds.
ISO 400
For indoor or overcast conditions; or if you want to avoid using fl ash, or need a fast shutter speed/aperture to shoot
ISO 800
For overcast or dark indoor shooting, sports or action photography where you need to freeze the motion and some noise is okay.
ISO 1600
Night time,
ISO 3200
For
Metering
DSLRs come with a |
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or ‘metering’ to ensure your shots are |
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properly exposed; not too light, and not too |
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dark, for example. The system is designed |
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to measure light refl ected from your subject |
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from either the entire frame (Matrix or Evalu- |
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ative metering) a |
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of the scene (Centre Weighted), or from a |
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small spot, usually in the middle of the frame |
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(Spot metering). You can set the camera to |
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use whatever metering method you require |
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to achieve a |
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task, but its effect can be altered to suit the |
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subject (or your preference) by controlling the |
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aperture and shutter speeds in the manual |
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modes, for example. |
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Importantly, many DSLRs have their |
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focusing zones linked directly to the metering |
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system, thus providing a very accurate |
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bias in the metering to whichever AF point |
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(or points) are in use. This makes accurate |
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metering from specifi c (often tiny) areas in |
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a scene possible and provides a great level |
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of extra control should it be required, if, say, |
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the camera’s main metering systems are not |
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cutting the mustard. | Above: One stop over |
Typical auto white balance settings
•Auto: General scenes/mixed lighting but colours may not be accurate in some lighting.
•Direct Sunlight: Ideal for bright, sunlit daylight.
•Shade: Best for shade or shots in deeper shadow.
•Cloud: Use for overcast daylight shots.
•Flash: Use with fl ash photos including fi
•Incandescent: Use for atmospheric candlelit images.
•Fluorescent: Use when shooting photos using light from kitchen- style strip lights.
•Tungsten: Ideal for household bulb/lamplight shots and shots taken indoors.
•Custom: User set (see text above) to whatever ambient light is present in any conditions for most accurate colour rendition.
a Kelvin scale for even fi ner tuning as well as the custom mode. The latter allows you to set WB specifi cally for the current ambient light; typically this involves taking a shot (in the custom WB set- up screen) of something plain, fi lling the frame and you know to be white: paper, anything. It does not even have to be in focus. Using the custom method of WB control means no matter what the ambient light, you will always have white whites!
Here is a quick guide to colour temperature using the Kelvin scale and the corresponding (typical) light source. The lower the Kelvin
figure, the warmer (or redder) the colour is going to be. The higher the Kelvin fi gure, the hotter the light source is and bluer the colour.
1,700-1,800k = Match fl ame
6 | 7 |