Hello,
Since the inception of photography almost 200 years ago, understanding and mastering light has always been and will always be the fundamental base of photography. Geez, I should be a philosopher!
Technology has always been advancing in the area of exposure estimation and automation. From early Sunny 16 tables to today's advanced multimode predictive super duper nuclear powered multidimensional and time traveling metering, getting the exposure right is the goal. Light metering has come a long way.
One of the earliest types of light meters was the extinction meter in the late 19th century. There were several variations and types but essentially, it consists of an array of calibrated ND filters of different values. The photographer will look at the scene thru it and determine which value still allows light thru and that will be the basis for an exposure calculator to suggest appropriate exposure combinations.
Let me show you an example with this Argus A2B, equipped with an extinction meter/calculator. Argus introduced this type of extinction meter in their cameras in 1939 on the A2B and A2F models.
(You can read more about this camera in this link:
1948 Argus A2B: Entry level 35mm popularization camera - PentaxForums.com)
First of all, this meter is calibrated in Weston sensitivity, Not ASA/ISO
The conversion is:
ASA - Weston
15 --- 12
25 --- 20
50 --- 40
100 ---72
ASA 100 was considered fast in its day
Steps for calculating the exposure:
1. Point the meter to the scene and determine where the light falls off. Dimmest window still letting light go thru
2. Move the slider to match that location
3. Set the sensitivity
4. Set the conditions: Bright, Average, Cloudy, Interior lit room.
Make sure both sliders move together to ensure proper sensitivity. If not, adjust accordingly.
5. Take a reading from the calculator
Examples:
So, next time you complain about the meter in your DSLR, remember those before you that had to use these.
Hope you like this.
Thanks,
Ismael