Guide NumberThere are a number of scientific units for light intensity, but they are too specific to be applied easily to photography. So in photography a “helper unit” is used, the Guide Number (GN). The guide number specifies the distance of an object to be exposed correctly with a flash unit, using ISO 100 film and an aperture of f/1.0. The GN is expressed in meters or feet, because it's a distance unit (I will use meters here). It basically describes the intensity of a flash pulse required to correctly expose the object.
The simplified formula for flash exposure at ISO 100 is:
GN = aperture × distanceor
distance = GN / aperture
Manual FlashA flash unit is a near-point light source. The light that the flash unit emits illuminates a larger area the farther you're away from the flash. Specifically, the intensity of the light decreases with the square of the distance from the flash. This is because the flash illuminates the surface area of a (virtual) sphere with the flash at its center, and, as we've learned in school, the surface area of a sphere increases with the square of the radius. So when you increase the distance from the light source by a factor of 1.4, the light intensity will be only 1/2 of the original. If you double the distance, light intensity decreases to 1/4, and so on.
When we use a fully manual flash system, we can calculate the required flash intensity when we know the film's sensitivity, the distance between flash and subject and the effective aperture. For example, when the subject is 10 meters away from the flash, we use ISO 100 film and we shoot at f/2.8, the required GN for correct exposure would be 30 m (f/2.8 is 3 stops slower than f/1.0, so we need three times the light intensity for the same exposure).
With manual flash you adjust flash output exactly in this way. You first calculate the required guide number. Then you set up the flash unit to emit such a burst. Most flash units can not be adjusted in such fine steps, so you choose the closest setting and fine-tune with either flash distance or aperture. After that's done, you can shoot, and the object will be exposed correctly.
The nice thing about manual flash is what is not relevant:
- Shutter speed (that's the case with all flash systems, as long as you stay below the x-sync speed of the camera)
- Brightness or reflectivity of the object
However, using manual flash is also very tedious. You have to measure the distance, factor in the film speed and aperture, factor in everything else that influences either flash output (diffusors, concentrators) or effective aperture (filters, extension tubes), adjust the flash unit and probably do some fine-tuning. This is not only very complicated, but also quite slow. With quick-changing situations you will not want to use manual flash.
Correct Flash ExposureWhen I said “correct exposure” above, I meant the technical definition of “correct”. This means that a mid-toned object (eg. a grey card) will also appear mid-toned in the image. Sometimes you intentionally increase this exposure to get more details in the shadows of the image, or you decrease it to get details in the highlights. This is a different aspect of exposure, and I will concentrate on the technical aspects here.
© 2008 Michael Hohner; This page was last changed on 2011-09-29
The current Minolta AF/Sony Alpha flash system has grown quite complex, and it is not very well covered in the manuals. That's because this would involve to cover some very basic concepts, and there are many combinations of cameras and flash units with different capabilities that would have to be documented. What I try here is to explain how the Minolta flash system works in detail. This compendium assumes that you have some basic knowledge of photography, ie. you know that an aperture is and you know how a shutter works. Sony has taken over further development of the Minolta A mount (now Sony Alpha mount) and has also kept the Minolta AF flash system with their new DSLRs. When this compedium says "Minolta", the same is true for "Sony Alpha", too, except when noted otherwise.