mrcal-stereo(1)

OPTIONAL ARGUMENTS

will be made available with time.

OPTIONAL ARGUMENTS

  -h, --help            show this help message and exit
  --az-fov-deg AZ_FOV_DEG
                        The field of view in the azimuth direction, in
                        degrees. There's no auto-detection at this time, so
                        this argument is required (unless --already-rectified)
  --el-fov-deg EL_FOV_DEG
                        The field of view in the elevation direction, in
                        degrees. There's no auto-detection at this time, so
                        this argument is required (unless --already-rectified)
  --az0-deg AZ0_DEG     The azimuth center of the rectified images. "0" means
                        "the horizontal center of the rectified system is the
                        mean forward direction of the two cameras projected to
                        lie perpendicular to the baseline". If omitted, we
                        align the center of the rectified system with the
                        center of the two cameras' views
  --el0-deg EL0_DEG     The elevation center of the rectified system. "0"
                        means "the vertical center of the rectified system
                        lies along the mean forward direction of the two
                        cameras" Defaults to 0.
  --pixels-per-deg PIXELS_PER_DEG
                        The resolution of the rectified images. This is either
                        a whitespace-less, comma-separated list of two values
                        (az,el) or a single value to be applied to both axes.
                        If a resolution of >0 is requested, the value is used
                        as is. If a resolution of <0 is requested, we use this
                        as a scale factor on the resolution of the first input
                        image. For instance, to downsample by a factor of 2,
                        pass -0.5. By default, we use -1 for both axes: the
                        resolution of the input image at the center of the
                        rectified system.
  --rectification {LENSMODEL_PINHOLE,LENSMODEL_LATLON}
                        The lens model to use for rectification. Currently two
                        models are supported: LENSMODEL_LATLON (the default)
                        and LENSMODEL_PINHOLE. Pinhole stereo works badly for
                        wide lenses and suffers from varying angular
                        resolution across the image. LENSMODEL_LATLON
                        rectification uses a transverse equirectangular
                        projection, and does not suffer from these effects. It
                        is thus the recommended model
  --already-rectified   If given, assume the given models and images already
                        represent a rectified system. This will be checked,
                        and the models will be used as-is if the checks pass
  --clahe               If given, apply CLAHE equalization to the images prior
                        to the stereo matching. If --already-rectified, we
                        still apply this equalization, if requested. Requires
                        --force-grayscale
  --force-grayscale     If given, convert the images to grayscale prior to
                        doing anything else with them. By default, read the
                        images in their default format, and pass those
                        posibly-color images to all the processing steps.
                        Required if --clahe
  --viz {geometry,stereo}
                        If given, we visualize either the rectified geometry
                        or the stereo results. If --viz geometry: we construct
                        the rectified stereo system, but instead of continuing
                        with the stereo processing, we render the geometry of
                        the stereo world; the images are ignored in this mode.
                        If --viz stereo: we launch an interactive graphical
                        tool to examine the rectification and stereo matching
                        results; the Fl_Gl_Image_Widget Python library must be
                        available
  --axis-scale AXIS_SCALE
                        Used if --viz geometry. Scale for the camera axes. By
                        default a reasonable default is chosen (see
                        mrcal.show_geometry() for the logic)
  --title TITLE         Used if --viz geometry. Title string for the plot
  --hardcopy HARDCOPY   Used if --viz geometry. Write the output to disk,
                        instead of making an interactive plot. The output
                        filename is given in the option
  --terminal TERMINAL   Used if --viz geometry. The gnuplotlib terminal. The
                        default is almost always right, so most people don't
                        need this option
  --set SET             Used if --viz geometry. Extra 'set' directives to pass
                        to gnuplotlib. May be given multiple times
  --unset UNSET         Used if --viz geometry. Extra 'unset' directives to
                        pass to gnuplotlib. May be given multiple times
  --force, -f           By default existing files are not overwritten. Pass
                        --force to overwrite them without complaint
  --outdir OUTDIR       Directory to write the output into. If omitted, we
                        user the current directory
  --tag TAG             String to use in the output filenames. Non-specific
                        output filenames if omitted
  --disparity-range DISPARITY_RANGE DISPARITY_RANGE
                        The disparity limits to use in the search, in pixels.
                        Two integers are expected: MIN_DISPARITY
                        MAX_DISPARITY. Completely arbitrarily, we default to
                        MIN_DISPARITY=0 and MAX_DISPARITY=100
  --valid-intrinsics-region
                        If given, annotate the image with its valid-intrinsics
                        region. This will end up in the rectified images, and
                        make it clear where successful matching shouldn't be
                        expected
  --range-image-limits RANGE_IMAGE_LIMITS RANGE_IMAGE_LIMITS
                        The nearest,furthest range to encode in the range
                        image. Defaults to 1,1000, arbitrarily
  --stereo-matcher {SGBM,ELAS}
                        The stereo-matching method. By default we use the
                        "SGBM" method from OpenCV. libelas isn't always
                        available, and must be enabled at compile-time by
                        setting USE_LIBELAS=1 during the build
  --sgbm-block-size SGBM_BLOCK_SIZE
                        A parameter for the OpenCV SGBM matcher. If omitted, 5
                        is used
  --sgbm-p1 SGBM_P1     A parameter for the OpenCV SGBM matcher. If omitted,
                        the OpenCV default is used
  --sgbm-p2 SGBM_P2     A parameter for the OpenCV SGBM matcher. If omitted,
                        the OpenCV default is used
  --sgbm-disp12-max-diff SGBM_DISP12_MAX_DIFF
                        A parameter for the OpenCV SGBM matcher. If omitted,
                        the OpenCV default is used
  --sgbm-pre-filter-cap SGBM_PRE_FILTER_CAP
                        A parameter for the OpenCV SGBM matcher. If omitted,
                        the OpenCV default is used
  --sgbm-uniqueness-ratio SGBM_UNIQUENESS_RATIO
                        A parameter for the OpenCV SGBM matcher. If omitted,
                        the OpenCV default is used
  --sgbm-speckle-window-size SGBM_SPECKLE_WINDOW_SIZE
                        A parameter for the OpenCV SGBM matcher. If omitted,
                        the OpenCV default is used
  --sgbm-speckle-range SGBM_SPECKLE_RANGE
                        A parameter for the OpenCV SGBM matcher. If omitted,
                        the OpenCV default is used
  --sgbm-mode {SGBM,HH,HH4,SGBM_3WAY}
                        A parameter for the OpenCV SGBM matcher. Must be one
                        of ('SGBM','HH','HH4','SGBM_3WAY'). If omitted, the
                        OpenCV default (SGBM) is used
  --write-point-cloud   If given, we write out the point cloud as a .ply file.
                        Each point is reported in the reference coordinate
                        system, colored with the nearest-neighbor color of the
                        camera0 image. This is disabled by default because
                        this is potentially a very large file
  --jobs, -j JOBS       parallelize the processing JOBS-ways. This is like
                        Make, except you're required to explicitly specify a
                        job count. This applies when processing multiple sets
                        of images with the same set of models