Differences
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isp:brightness [2023/09/10 20:56] – [Algorithm] Igor Yefmov | isp:brightness [2023/09/10 21:01] – [Calculation reference] Igor Yefmov | ||
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To calculate luminosity we just find the max and min of the triplet and get a simple average: | To calculate luminosity we just find the max and min of the triplet and get a simple average: | ||
\[L = \frac{min(R, | \[L = \frac{min(R, | ||
+ | |||
+ | Brightness adjustment is a trivial addition, clamping the value to its proper limits: | ||
+ | |||
+ | \[ | ||
+ | L` = L + br \\ | ||
+ | L` \in [0..4095] | ||
+ | \] | ||
The slope \(k_R\) for the red component calculation depends on whether \(L\) is above or below the middle: | The slope \(k_R\) for the red component calculation depends on whether \(L\) is above or below the middle: | ||
Line 30: | Line 37: | ||
\] | \] | ||
- | Brightness adjustment is a trivial addition, clamping | + | Finding |
+ | \[ | ||
+ | R = | ||
+ | \begin{cases} | ||
+ | k_R * 2047 & \text{if} \; L \leq 2047 \\ | ||
+ | 255 - k_R * 2047 & \text{if} \; L > 2047 | ||
+ | \end{cases} | ||
+ | \] | ||
+ | If we are crossing the middle luma boundary as the result of this adjustment - flip the slope: | ||
\[ | \[ | ||
- | L` = L + br \\ | + | k_R = 2 - k_R |
- | L` \in [0..4095] | + | |
\] | \] | ||