There are several factors that influence the brightness of an image:
1. The brightness of the light
2. The reflective properties of the subject
3. The aperture
4. The shutter speed
5. The ISO
The first and most important is the brightness of the incident light. It can be quantified as Light Value (LV). For example, the brightness of full sunlight during the middle of the day in temperate or tropical latitudes can be considered nearly constant. For reasons that will soon be apparent, letβs assign it a value of 15.
* Taken from the Wikipedia article on Exposure value where you can find additional information.
The second factor is the reflective properties of the objects in the scene, how much of the incident light is reflected. This ranges from very high (for snow, white clouds, white paint or white feathers it can be 90% or more) to very low (a pile of coal might reflect 10% or less). But you
want to render these subjects as bright and dark. Your camera's meter will try to render them as middle gray. That would be wrong.
Here is how we end up at LV=15.
Shutter speeds starting at 1 second are given a value of 0. Each doubling of the shutter speed increases that value by one:
For longer shutter speeds the value becomes negative.
Apertures starting at f/1 are given a value of 0.
When you combine the value for the shutter speed with the value for the aperture you get the Exposure Value (EV):
ISO values starting at ISO 100 are given a value of 0.
When you combine exposure value with value for the ISO you get the Light Value (LV).
LV 15 is substantially in agreement with Sunny 16 which recommends 1/ISO sec @ f/16 - LV=14.67.
Since the value for ISO 100 is 0, the exposure value table for ISO 100 can be used as a light value table.
Knowing all of this you can learn to set your ISO and exposure without looking at your meter.