On Thu, 15 Jan 2015, Vittorio Giovara wrote:

---
libswscale/input.c                  | 5 ++---
tests/ref/fate/filter-pixfmts-scale | 2 +-
2 files changed, 3 insertions(+), 4 deletions(-)

diff --git a/libswscale/input.c b/libswscale/input.c
index f575b7b..e806bce 100644
--- a/libswscale/input.c
+++ b/libswscale/input.c
@@ -596,12 +596,11 @@ static void planar_rgb_to_y(uint8_t *dst, const uint8_t 
*src[4], int width)
    }
}

-static void planar_rgb_to_a(uint8_t *_dst, const uint8_t *src[4], int width)
+static void planar_rgb_to_a(uint8_t *dst, const uint8_t *src[4], int width)
{
-    uint16_t *dst = (uint16_t *)_dst;
    int i;
    for (i = 0; i < width; i++)
-        dst[i] = src[3][i] << 6;
+        dst[i] = src[3][i];
}

static void planar_rgb_to_uv(uint8_t *dstU, uint8_t *dstV, const uint8_t 
*src[4], int width)
diff --git a/tests/ref/fate/filter-pixfmts-scale 
b/tests/ref/fate/filter-pixfmts-scale
index 712754c..408644b 100644
--- a/tests/ref/fate/filter-pixfmts-scale
+++ b/tests/ref/fate/filter-pixfmts-scale
@@ -12,7 +12,7 @@ bgr565be            922a2503767036ae9536f4f7823c04ee
bgr565le            3a514a298c6161a071ddf9963c06509d
bgr8                7f007fa6c153a16e808a9c51605a4016
bgra                a5e7040f9a80cccd65e5acf2ca09ace5
-gbrap               08ea11431bc436d788494d678b3edc6f
+gbrap               7df4fd8da27245788cb422794e03acd4
gbrp                205c50f8359cb4ba2827a7711dea2cc6
gbrp10be            30b7f9d5ef5da474fb794743146236aa
gbrp10le            2e9949a01fe4c38774728e34795165cc
--
1.9.3 (Apple Git-50)

Ok - I'm not familiar enough to comment much on the swscale internals, but this makes the output consistent on bigendian, and actually makes at least a fully opaque alpha plane stay that way after scaling, so ok as far as I can see.

Karma points for scaling a picture with actual alpha (not just 255 for all pixels) and checking that it turns out right after scaling.

// Martin
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