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This enables us to check for overlay planes which are located
'below' the primary plane.
Since the alpha value only has an effect when creating surfaces
with an alpha-pixelformat this doesn't affect the regular
XRGB8888 primary surface.
Signed-off-by: Tobias Jakobi <tjakobi@math.uni-bielefeld.de>
Acked-by: Emil Velikov <emil.l.velikov@gmail.com>
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Signed-off-by: Emil Velikov <emil.l.velikov@gmail.com>
Reviewed-by: Alex Deucher <alexander.deucher@amd.com>
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Signed-off-by: Rob Clark <robclark@freedesktop.org>
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The current order (rbg) seems wrong.
Signed-off-by: Joonyoung Shim <jy0922.shim@samsung.com>
[Emil Velikov: Tweak the commit message.]
Reviewed-by: Emil Velikov <emil.l.velikov@gmail.com>
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Provide a more meaningful name, considering what it does.
Signed-off-by: Emil Velikov <emil.l.velikov@gmail.com>
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The modetest application uses libkms to allocate dumb buffers, leading
to overallocation due to the hardcoded 32 bpp value. This can even cause
failures in drivers when the resulting pitch is too large for the
hardware to handle and gets rejected by the driver when creating the
frame buffer.
Fix this by computing the required bpp value and allocating dumb buffers
directly without going through libkms.
Signed-off-by: Laurent Pinchart <laurent.pinchart@ideasonboard.com>
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Make upper-left corner for RGB32 buffers translucent, for testing
blending of AR24 vs XR24.
Signed-off-by: Rob Clark <robclark@freedesktop.org>
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... rather than explicitly redefining HAVE_STDINT_H and _GNU_SOURCE.
Signed-off-by: Emil Velikov <emil.l.velikov@gmail.com>
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Multiple the image height by 1.5 for NV12/NV21 and by 2 for NV16/NV61 to
make room for the chroma plane.
Signed-off-by: Laurent Pinchart <laurent.pinchart@ideasonboard.com>
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The line stride passed to the function is expressed in bytes, there's no
need to multiply it by 2.
Signed-off-by: Laurent Pinchart <laurent.pinchart@ideasonboard.com>
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Enable all standard automake warnings except for -Wpointer-arith (as the
test pattern generation code uses void pointer arithmetics) and fix
them.
Signed-off-by: Laurent Pinchart <laurent.pinchart@ideasonboard.com>
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Render the crosshairs for 565 and x888/a888 formats.
v2: Use the drm format to determine cairo format
Acked-by: Laurent Pinchart <laurent.pinchart@ideasonboard.com>
Signed-off-by: Ville Syrjälä <ville.syrjala@linux.intel.com>
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YUV420 support is trivial to add since the code already supports
YVU420.
But it looks like the YVU420 support is a bit broken. The chroma
planes are passed in the wrong order to the fill functions, so
fix that while were at it.
Signed-off-by: Ville Syrjälä <ville.syrjala@linux.intel.com>
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The fourcc is inside the format_info structure, so if we want to use
it inside the various fill_tiles functions, we need to pass down the
whole format_info, not just the rgb/yuv infos.
Signed-off-by: Ville Syrjälä <ville.syrjala@linux.intel.com>
Acked-by: Laurent Pinchart <laurent.pinchart@ideasonboard.com>
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Signed-off-by: Ville Syrjälä <ville.syrjala@linux.intel.com>
Acked-by: Laurent Pinchart <laurent.pinchart@ideasonboard.com>
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libkms only has the xrgb8888 format, so we're overallocating the bo by
quite a lot in some cases. But we still need to get the pitch from the
libkms since it's the driver that decides how to align it.
Signed-off-by: Ville Syrjälä <ville.syrjala@linux.intel.com>
Acked-by: Laurent Pinchart <laurent.pinchart@ideasonboard.com>
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As the modeset test application is often referred to as an example of
the KMS API usage, move test pattern generation and buffer allocation to
a separate file to keep it simple and clear.
Signed-off-by: Laurent Pinchart <laurent.pinchart@ideasonboard.com>
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