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| author | Matthew Hoops | 2012-09-19 16:00:27 -0400 |
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| committer | Matthew Hoops | 2012-09-19 16:00:27 -0400 |
| commit | 0677871ea94356e0a4a224840de691c05c05e8c5 (patch) | |
| tree | b23f9094d72ff56ecd236a360154dab4e5862a5f | |
| parent | 173dace75b2cc7c06c9cae46efe51162490f9e40 (diff) | |
| download | scummvm-rg350-0677871ea94356e0a4a224840de691c05c05e8c5.tar.gz scummvm-rg350-0677871ea94356e0a4a224840de691c05c05e8c5.tar.bz2 scummvm-rg350-0677871ea94356e0a4a224840de691c05c05e8c5.zip | |
GRAPHICS: Update YUV410 conversion docs
| -rw-r--r-- | graphics/yuv_to_rgb.h | 5 |
1 files changed, 3 insertions, 2 deletions
diff --git a/graphics/yuv_to_rgb.h b/graphics/yuv_to_rgb.h index 68a0449d2c..0e832be0ec 100644 --- a/graphics/yuv_to_rgb.h +++ b/graphics/yuv_to_rgb.h @@ -82,8 +82,9 @@ public: * * Since the chroma has a very low resolution in 410, we perform bilinear scaling * on the two chroma planes to produce the image. The chroma planes must have - * at least one extra row that can be read from in order to produce a proper - * image (filled with 0x80). This is required in order to speed up this function. + * at least one extra row and one extra column that can be read from in order to + * produce a proper image. It is suggested that you fill these in with the previous + * row and column's data. This is required in order to speed up this function. * * @param dst the destination surface * @param scale the scale of the luminance values |