mirror of https://github.com/mpv-player/mpv
242 lines
10 KiB
Plaintext
242 lines
10 KiB
Plaintext
Video Filters
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=============
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video filters are plugin-like code modules implementing the interface
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defined in vf.h
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basically it means video output manipulation, ie. these plugins can
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modify the image and the image properties (size, colorspace etc) between
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the video decoders (vd.h) and output layer (libvo or video encoders)
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the actual API is a mixture of the video decoder (vd.h) and libvo
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(video_out.h) APIs.
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the main differences:
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- vf plugins may be "loaded" multiple times, with different parameters
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and context - it's new in mplayer, old APIs weren't reentrant
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- vf plugins don't have to implement all functions - all funcs has
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'fallback' version, so the plugins only override these if want
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- each vf plugin has its own get_image context, and they can interchange
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images/buffers using these get_image/put_image calls.
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API details:
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-- TO DO -- (see vf.h fpr API and vf_*.c for examples)
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Current plugins:
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================
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-vf crop[=w:h:x:y]
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Simple cropping plugin.
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w,h (cropped width,height) defaults to original width,height
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x,y (position of cropped subimage on the original image) defaults to center
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MPI: EXPORT only, using stride manipulation
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-vf expand[=w:h:x:y:o]
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Expanding _and_ (optional) OSD rendering plugin.
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w,h (expanded width,height) defaults (-1) to original width,height
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x,y (position of original image on the expanded image) defaults (-1) to center
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o (0=disable/1=enable SUB/OSD rendering) defaults (0) to disabled
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MPI: DR (if possible) or copy
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Special: mpcodecs core uses it to solve stride restrictions between filters
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mencoder uses (autoload) it to render SUB/OSD
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-vf flip
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Flips image upside-down (vertical mirroring)
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No parameters.
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MPI: DR (if possible) or EXPORT, using stride manipulation
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Special: dec_video autoloads it when flipping is required and libvo can't do
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-vf mirror
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Horizontal mirroring
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No parameters.
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MPI: TEMP
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-vf rectangle[=w:h:x:y]
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Draw a rectangle. Useful for testing crop plugin parameters.
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w,h (rectangle's width and height) defaults (-1) to maximum
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possible width while keeping the boundaries visible.
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x,y (rectangle's top left corner position) defauts (-1) to upper
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left most position.
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The plugin responds to the input.conf directive "change_control"
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that takes two parameters. The first parameter can be 0 for w, 1
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for h, 2 for x or 3 for y. The second parameter is the amount to
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change the designated rectangle boundary.
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MPI: TEMP, accepts stride
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-vf rotate[=x]
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Rotate image +/- 90 degrees
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Optional 'x' parameter (0..3) controls horizontal and vertical mirroring
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MPI: TEMP
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-vf scale[=w:h[:c[:p]]]
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Software scaling (zoom) _and_ yuv<->rgb colorspace conversion
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w,h (new width/height after scaling) defaults to original width,height
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note: if -zoom is used, and underlaying filters (including libvo)
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uncapable of scaling, then it defaults to d_width/d_height !
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note 2: w/h values -1 means original width/height, 0 means scaled
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d_width/d_height. -2/-3 means calculating w or h using the other
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dimension and the original (-3) or prescaled (-2) aspect ratio.
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c chroma skipping
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0 -> use all available input lines for chroma
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1 -> use only every 2. input line for chroma
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2 -> use only every 4. input line for chroma
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3 -> use only every 8. input line for chroma
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p scaling parameter (depends upon the used scaling method)
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for -sws 2 (bicubic) its sharpness (0 (soft) - 100 (sharp))
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for -sws 7 (gaussian) its sharpness (0 (soft) - 100 (sharp))
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for -sws 9 (lanczos) its filter length (1 - 10)
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MPI: TEMP, accepts stride
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Special: dec_video and mpcodecs core autoloads it for colorspace conv.
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-vf yuy2
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Forced software YV12/I420 -> YUY2 conversion
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(usefull for video cards/drivers with slow YV12 but fast YUY2 support)
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MPI: TEMP, accepts stride
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-vf rgb2bgr[=swap]
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RGB 24/32 <-> BGR 24/32 colorspace conversion (default) or
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RGB 24/32 <-> RGB 24/32 conversion with R<->B swapping ('swap' option)
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MPI: TEMP, accepts stride
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-vf palette
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RGB/BGR 8 -> RGB/BGR 15/16/24/32 colorspace conversion using palette
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MPI: TEMP, accepts stride
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-vf format[=fourcc]
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_restrict_ the list of supported colorspaces (query-format()) to a single,
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given fourcc. The 'fourcc' option defaults to 'yuy2', but may be any
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format name, like rgb15, bgr24, yv12 etc...
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note again, it does NOT do any conversion, it just limits the _next_
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plugins format list.
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MPI: passthru
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-vf pp=[<filterName>[:<option>[:<option>...]][/[-]<filterName>[:<option>...]]...]
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Postprocessing filter. (usefull for codecs without built-in
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postprocessing, like libmpeg12 or libavcodec)
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see `mplayer -vf pp=help`
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MPI: DR (if possible) or TEMP
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Special: dec_video autoloads it if -pp option used but codec can't do pp.
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-vf lavc[=quality:fps]
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Fast software YV12->MPEG1 conversion, usefull for dxr3/dvb drivers
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It uses libavcodec. Currently faster and better quality than -vf fame!
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Param quality: fixed qscale (1<=quality<32) or bitrate (32<=quality KBits)
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Param fps: force output fps (float value). If not give, or 0, it's
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autodetected based on height (240,480->29.97fps, others -> 25fps)
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MPI: EXPORT special
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-vf fame
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Fast software YV12->MPEG1 conversion, usefull for dxr3/dvb drivers
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It uses libfame.
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MPI: EXPORT special
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-vf dvbscale[=aspect]
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Setup scaling to the optimal values for the DVB card.
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(use HW for X-scaling, calc sw Y scaling to keep aspect)
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The 'aspect' parameter controls aspect ratio, it should be calculated
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as aspect=DVB_HEIGHT*ASPECTRATIO, default is 576*(4/3)=768
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(for 16:9 TV set it to 576*(16/9)=1024)
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It's only usefull together with expand+scale:
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-vf dvbscale,scale=-1:0,expand=-1:576:-1:-1:1,lavc
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MPI: passthru
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-vf cropdetect[=limit]
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It's a special filter, it doesn't alter the image itself, but detects
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(using some kind of heuristics) the black borders/bands of the image,
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and prints the optimal -vf crop= parameters to the stdout/console.
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It calculates the average value of pixel luminances for a line, and
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depending on the result it's either black band (result<=limit) or
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picture (result>limit). Optional parameter 'limit' defaults to 24.
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MPI: EXPORT
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-vf test[=first frame number]
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generate various test patterns
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MPI: TEMP, accepts stride
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-vf noise[=lumaNoise[u][t|a][h]:chromaNoise[u][t|a][h]
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add noise
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0<= lumaNoise, chromaNoise <=100
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u uniform noise (gaussian otherwise)
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t temporal noise (noise pattern changes between frames)
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a averaged temporal (smoother, but a lot slower)
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h high quality (slightly better looking, slightly slower)
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p mix random noise with a (semi)regular pattern
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MPI: DR (if possible) or TEMP, accepts stride
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-vf eq[=brightness:contrast]
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software equalizer, for use with cards that don't support
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brightness and contrast controls in hardware. It might also be
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useful with mencoder, either for fixing poorly captured movies, or
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for slightly reducing contrast to mask artifacts and get by with
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lower bitrates. Initial values in the range -100..100 may be
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given on the command line, and the eq filter is controllable
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interactively just like with normal hardware equalizer controls.
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-vf eq2[=gamma:contrast:brightness:saturation:r_gamma:g_gamma:b_gamma]
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advanced software equalizer, for use with cards that don't support
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brightness/contrast/saturation and channel gamma controls in hardware.
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Initial values in the range -2.0 .. 2.0 may be given on the command line,
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and the eq2 filter is controllable interactively just like with normal
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hardware equalizer controls or -vf eq. Defaults: 1:1:0:1:1:1:1
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This filter uses MMX only if available and all gamma == 1.0, otherwise
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LUT (look-up table) is being used.
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-vf unsharp=l|cWxH:amount[:l|cWxH:amount]
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unsharp mask / gaussian blur.
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l apply effect on luma component
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c apply effect on chroma components
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WxH width and height of the matrix, odd sized in both directions
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min = 3x3, max = 13x11 or 11x13
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usually you will use somthing between 3x3 and 7x7
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amount relative amount of sharpness / blur to add to the image
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amount < 0 = blur, amount > 0 = sharpen
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usually you will use something between -1.5 and 1.5
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MPI: DR (if possible) or TEMP, accepts stride
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-vf swapuv
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swap U & V plane
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MPI: EXPORT
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-vf il=[d|i][s][:[d|i][s]]
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(de)interleaves lines
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d deinterleave
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i interleave
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s swap fields (exchange even & odd lines)
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The goal of this filter to add ability of processing interlaced images
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pre-field without deinterlacing it. You can filter your interlaced dvd
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and playback on TV without breaking the interlacing.
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While deinterlacing (with the post processing filter) removes permamently
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the interlacing (by smoothing averaging etc) deinterleaving splits the
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frame into 2 fields (so called half pictures), so you can process (filter)
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them independently and then re-interleave them.
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MPI: TEMP, accepts stride
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-vf boxblur=radius:power[:radius:power]
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radius size of the filter
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power how often the filter should be applied
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MPI: TEMP, accepts stride
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-vf sab=radius:prefilter:colorDiff[:radius:prefilter:colorDiff]
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radius blur filter strength (~0.1-4.0) (slower if larger)
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prefilter prefilter strength (~0.1-2.0)
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colorDiff how different the pixels are allowed to be to be considered (~0.1-100.0)
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-vf smartblur=radius:stregth:threshold[:radius:stregth:threshold]
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radius blur filter strength (~0.1-5.0) (slower if larger)
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strength (0.0-1.0) -> blur, (-1.0-0.0) -> sharpen
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threshold 0 -> filter all, (0-30) -> filter flat areas, (-30-0) -> filter edges
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-vf perspective=x0:y0:x1:y1:x2:y2:x3:y3:t
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x0,y0,... coordinates of the topleft, topright, bottomleft, bottomright corners
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t 0-> linear, 1->cubic resampling
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-vf denoise3d=[luma:chroma:time]
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luma spatial luma strength (default = 4)
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chroma spatial chroma strength (default = 3)
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time temporal strength (default = 6)
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This filter aims to reduce image noise producing smooth images and
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making stills realy still. (it should enhance compressibility)
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Can be given from 0 to 3 parameters. Parameters not given will be
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infered from the given ones. (ie: providing only one of them acts as an
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"scale factor")
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