Distance from light(or other electromagnetic)source

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The discussion focuses on calculating distance from a light source using the UVB band energy values derived from the Planck-Einstein equation. The participant confirms that light intensity can be expressed using the formula E_r = E_0 / (4πr²), where E(r) and E(0) are known values. They propose substituting energy values (in eV) for light radiation to determine distance, utilizing UV sensor readings. The mathematical manipulation to derive the distance formula is provided, emphasizing the use of the positive root since distance cannot be negative. This approach aims to explore a novel method of distance calculation based on energy measurements.
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Hello.I'm doing a research on ultraviolet (mainly on UVB band).
UVB band with the wavelength 280nm~315nm has the energy of 4.43eV~3.94eV
which can be calculated from Plank-Einstein equation.

In visible spectrum,light intensity can be calculated from
E_{r}=\frac{E_{0}}{4\pi r^{2}}
With the above equation,when E(r) and E(0) is known,distance,r can be calculated.
Light radiation is measured in mW/cm^2,and I right?

So,my question is,using the above equation,instead of light radiation,
is it possible to calculate distance by replacing E(r) and E(0) with energy [eV] ?
Where E(r) and E(0) can be obtained from UV sensor readings.
Radiometers do measure UV intensity in mW/cm^2. I'm trying something different.
 
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Yes, of course, that's a simple algebra calculation.

Multiply both sides of the equation by r^2 and divide both sides by E_r to get
r^2= \frac{E_0}{4\pi E_r}
Now take the square root of both sides:
r= \sqrt{\frac{E_0}{4\pi E_r}}
We use the positive root because distance is always positive.
 
It may be shown from the equations of electromagnetism, by James Clerk Maxwell in the 1860’s, that the speed of light in the vacuum of free space is related to electric permittivity (ϵ) and magnetic permeability (μ) by the equation: c=1/√( μ ϵ ) . This value is a constant for the vacuum of free space and is independent of the motion of the observer. It was this fact, in part, that led Albert Einstein to Special Relativity.
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