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| author | Niklas Haas <git@haasn.dev> | 2023-09-20 02:09:05 +0200 |
|---|---|---|
| committer | Niklas Haas <github-daiK1o@haasn.dev> | 2023-09-20 17:07:38 +0200 |
| commit | c172a650c41a28d77d14de4af398cfd90caaa805 (patch) | |
| tree | 856a05303f6c315cf7ba2f4921edec0de12eeb77 /video | |
| parent | 87baed0b0f774940fbcc2a8d0298b525e2a28faf (diff) | |
| download | mpv-c172a650c41a28d77d14de4af398cfd90caaa805.tar.bz2 mpv-c172a650c41a28d77d14de4af398cfd90caaa805.tar.xz | |
vo_gpu: default to dscale=hermite
This new filter is slightly sharper, and significantly faster, than
mitchell. It also tends to preserve detail better. All in all, there is
no reason not to use it by default, especially from a performance PoV.
(In vo_gpu_next, hermite is implemented efficiently using hardware
accelerated bilinear interpolation)
See-Also: https://code.videolan.org/videolan/libplacebo/-/commit/75b3947b2c07803456483ec6976c037bad91b5dd
Diffstat (limited to 'video')
| -rw-r--r-- | video/out/gpu/video.c | 2 |
1 files changed, 1 insertions, 1 deletions
diff --git a/video/out/gpu/video.c b/video/out/gpu/video.c index 8618e8c6ef..3c8c6bae39 100644 --- a/video/out/gpu/video.c +++ b/video/out/gpu/video.c @@ -304,7 +304,7 @@ static const struct gl_video_opts gl_video_opts_def = { .scaler = { {{"lanczos", .params={NAN, NAN}}, {.params = {NAN, NAN}}, .cutoff = 0.001}, // scale - {{"mitchell", .params={NAN, NAN}}, {.params = {NAN, NAN}}, + {{"hermite", .params={NAN, NAN}}, {.params = {NAN, NAN}}, .cutoff = 0.001}, // dscale {{NULL, .params={NAN, NAN}}, {.params = {NAN, NAN}}, .cutoff = 0.001}, // cscale |