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| author | Jean-Michel Hautbois <jeanmichel.hautbois@ideasonboard.com> | 2021-11-19 07:56:12 +0100 |
|---|---|---|
| committer | Jean-Michel Hautbois <jeanmichel.hautbois@ideasonboard.com> | 2021-11-29 20:41:38 +0100 |
| commit | fea85f84c2ac940f1e149d1382216ab3da0b7703 (patch) | |
| tree | a1df8afaaa766cb7dff4c0b5da8c24dd57cea667 /src/v4l2/v4l2_camera_file.cpp | |
| parent | af7f70b69ac9c8127e14557a8f2d9618a054da59 (diff) | |
ipa: rkisp1: Introduce AGC
Now that we have IPAContext and Algorithm, we can implement a simple AGC
based on the IPU3 one. It is very similar, except that there is no
histogram used for an inter quantile mean. The RkISP1 is returning a 5x5
array (for V10) of luminance means. Estimating the relative luminance is
thus a simple mean of all the blocks already calculated by the ISP.
Signed-off-by: Jean-Michel Hautbois <jeanmichel.hautbois@ideasonboard.com>
Reviewed-by: Laurent Pinchart <laurent.pinchart@ideasonboard.com>
Reviewed-by: Kieran Bingham <kieran.bingham@ideasonboard.com>
Diffstat (limited to 'src/v4l2/v4l2_camera_file.cpp')
0 files changed, 0 insertions, 0 deletions