- #1
Fr34k
- 20
- 0
What is it, what does it mean/do and why is it used for? Its defined as:
S(r)=ln(P(r)r^2/(P(r0)r0^2)), where r is distance in atmosphere and P is intensity of detected light.
S(r)=ln(P(r)r^2/(P(r0)r0^2)), where r is distance in atmosphere and P is intensity of detected light.