If we consider the light emitted from a flashlight to come from a point source, the light flux (Lux) will be inversely proportional to the square of the distance from the light source. This means that if you measure the flux in one direction, you can based on this model calculate the flux at any distance in this direction.
[FONT="]I have earlier presented measurements of the light flux along at a certain distance (1 m) from the flashlight lens. This light flux can be integrated to give the total light output in lumens. Earlier, I measured this light flux as good as I was able to at 1 m distance. For lights with a very concentrated hot spot, this becomes quite difficult, and also it is a problem that my light sensor becomes quite big compared to the light flux gradients. Now I just use the concept from first paragraph, and can then [/FONT][FONT="]measure the light at any distance, and calculate back to the flux at 1 m. This means that I can use a distance of several meter, and get a good measurement of the spot for instance in my Dereelight DBS. After that, I can measure the spill in a much shorter distance, and combine. The result measured and calculated @ 1 m distance, for my Dereelight CL1H 3SD Q5 SMO looks like this
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This is as I can see it, a good way of presenting the light output from a flashlight. You get both the lumens, the max light flux (Lux) and also the distribution.
Since we here have the light distribution out from center, we can calculate the distance to a certain light flux in any direction. This makes it possible to present the area where the light flux is above a certain level. This looks like this:
Here I have used 1 Lux as one limit. This is may be a limit for usable light (about moonlight). As you can see my CL1H gives this light flux just above 100 m. I have also presented 10 Lux which is a quite good light level.
What do you think about this way of presenting the light output?
If any interest, I can also present the output from my DBS in a similar way.
Regards from
Jens
[FONT="]I have earlier presented measurements of the light flux along at a certain distance (1 m) from the flashlight lens. This light flux can be integrated to give the total light output in lumens. Earlier, I measured this light flux as good as I was able to at 1 m distance. For lights with a very concentrated hot spot, this becomes quite difficult, and also it is a problem that my light sensor becomes quite big compared to the light flux gradients. Now I just use the concept from first paragraph, and can then [/FONT][FONT="]measure the light at any distance, and calculate back to the flux at 1 m. This means that I can use a distance of several meter, and get a good measurement of the spot for instance in my Dereelight DBS. After that, I can measure the spill in a much shorter distance, and combine. The result measured and calculated @ 1 m distance, for my Dereelight CL1H 3SD Q5 SMO looks like this
[/FONT]


This is as I can see it, a good way of presenting the light output from a flashlight. You get both the lumens, the max light flux (Lux) and also the distribution.
Since we here have the light distribution out from center, we can calculate the distance to a certain light flux in any direction. This makes it possible to present the area where the light flux is above a certain level. This looks like this:

Here I have used 1 Lux as one limit. This is may be a limit for usable light (about moonlight). As you can see my CL1H gives this light flux just above 100 m. I have also presented 10 Lux which is a quite good light level.
What do you think about this way of presenting the light output?
If any interest, I can also present the output from my DBS in a similar way.
Regards from
Jens