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authorNiklas Haas <git@nand.wakku.to>2016-06-28 14:28:32 +0200
committerwm4 <wm4@nowhere>2016-06-28 19:48:29 +0200
commitdc9a5cbfd7c30d4f0597ec0aad91dadf63defbba (patch)
tree2bb156f5f84643068e34e4817860597f73c262dc
parent65499d863a41cd7403302b8b635e18b764d4f9eb (diff)
downloadmpv-dc9a5cbfd7c30d4f0597ec0aad91dadf63defbba.tar.bz2
mpv-dc9a5cbfd7c30d4f0597ec0aad91dadf63defbba.tar.xz
vo_opengl: revise the transfer curve logic
Instead of hard-coding a big list, move some of the functionality to csputils. Affects both the auto-guess blacklist and the peak estimation. Also update the comments.
-rw-r--r--video/csputils.c25
-rw-r--r--video/csputils.h2
-rw-r--r--video/out/opengl/video.c27
3 files changed, 37 insertions, 17 deletions
diff --git a/video/csputils.c b/video/csputils.c
index 65b26acb3a..d419152e2c 100644
--- a/video/csputils.c
+++ b/video/csputils.c
@@ -437,6 +437,31 @@ struct mp_csp_primaries mp_get_csp_primaries(enum mp_csp_prim spc)
}
}
+// Get the relative peak of a transfer curve, that is: (source reference /
+// display reference), or 0 if there is none (i.e. source has an absolute peak)
+float mp_csp_trc_rel_peak(enum mp_csp_trc trc)
+{
+ switch (trc) {
+ case MP_CSP_TRC_SMPTE_ST2084: return 0.0; // This has a fixed peak
+ case MP_CSP_TRC_ARIB_STD_B67: return 12.0;
+ case MP_CSP_TRC_V_LOG: return 46.0855;
+ }
+
+ return 1.0;
+}
+
+bool mp_trc_is_hdr(enum mp_csp_trc trc)
+{
+ switch (trc) {
+ case MP_CSP_TRC_SMPTE_ST2084:
+ case MP_CSP_TRC_ARIB_STD_B67:
+ case MP_CSP_TRC_V_LOG:
+ return true;
+ }
+
+ return false;
+}
+
// Compute the RGB/XYZ matrix as described here:
// http://www.brucelindbloom.com/index.html?Eqn_RGB_XYZ_Matrix.html
static void mp_get_rgb2xyz_matrix(struct mp_csp_primaries space, float m[3][3])
diff --git a/video/csputils.h b/video/csputils.h
index 047b109d2b..274b548381 100644
--- a/video/csputils.h
+++ b/video/csputils.h
@@ -219,6 +219,8 @@ int mp_chroma_location_to_av(enum mp_chroma_location mploc);
void mp_get_chroma_location(enum mp_chroma_location loc, int *x, int *y);
struct mp_csp_primaries mp_get_csp_primaries(enum mp_csp_prim csp);
+float mp_csp_trc_rel_peak(enum mp_csp_trc trc);
+bool mp_trc_is_hdr(enum mp_csp_trc trc);
/* Color conversion matrix: RGB = m * YUV + c
* m is in row-major matrix, with m[row][col], e.g.:
diff --git a/video/out/opengl/video.c b/video/out/opengl/video.c
index fff41a1b91..519857f7f9 100644
--- a/video/out/opengl/video.c
+++ b/video/out/opengl/video.c
@@ -2206,31 +2206,24 @@ static void pass_colormanage(struct gl_video *p, float peak_src,
}
if (trc_dst == MP_CSP_TRC_AUTO) {
+ // Most people seem to complain when the image is darker or brighter
+ // than what they're "used to", so just avoid changing the gamma
+ // altogether by default. The only exceptions to this rule apply to
+ // very unusual TRCs, which even hardcode technoluddites would probably
+ // not enjoy viewing unaltered.
trc_dst = p->image_params.gamma;
- // Avoid outputting linear light or HDR content "by default"
- if (trc_dst == MP_CSP_TRC_LINEAR ||
- trc_dst == MP_CSP_TRC_SMPTE_ST2084 ||
- trc_dst == MP_CSP_TRC_ARIB_STD_B67 ||
- trc_dst == MP_CSP_TRC_V_LOG)
- {
+ // Avoid outputting linear light or HDR content "by default". For these
+ // just pick gamma 2.2 as a default, since it's a good estimate for
+ // the response of typical displays
+ if (trc_dst == MP_CSP_TRC_LINEAR || mp_trc_is_hdr(trc_dst))
trc_dst = MP_CSP_TRC_GAMMA22;
- }
}
if (!peak_src) {
// If the source has no information known, it's display-referred
// (and should be treated relative to the specified desired peak_dst)
- peak_src = peak_dst;
-
- // Exception: ARIB STD-B67's nominal peak is exactly 12 times the
- // target's reference peak
- if (p->image_params.gamma == MP_CSP_TRC_ARIB_STD_B67)
- peak_src = 12 * peak_dst;
-
- // Similar deal for V-Log
- if (p->image_params.gamma == MP_CSP_TRC_V_LOG)
- peak_src = 46.0855 * peak_dst;
+ peak_src = peak_dst * mp_csp_trc_rel_peak(p->image_params.gamma);
}
// All operations from here on require linear light as a starting point,