GR-raytracing/usage.md

Rendering guide

See README.md for the project overview and a first 2MASS render, and build.md for compilation. Commands below run from the repository root and use the default Release binaries. Run a binary with --help for its complete option list and defaults.

Catalog input

Use --all-sky-catalog assets/2mass/processed/all_sky for the tiled 2MASS catalog, or --catalog PATH for a single processed CSV. Acquisition and processing are documented in assets/2mass/README.md. 2MASS blackbody amplitudes need a much larger display exposure than the synthetic test catalog; --exposure 1e15 is a starting point, to be adjusted for the field and camera.

Schwarzschild camera

schwarzschild_sky uses an analytic Schwarzschild metric in Cartesian ingoing Kerr–Schild coordinates, with mass M=1. The default camera is static at coordinate radius 30. --look-ra-deg and --look-dec-deg set the direction from the camera to the hole; the camera is placed on the opposite side of the origin and points radially inward. --observer-radius R requires R > 2. --observer-inward-speed V applies a local inward boost relative to the static observer, with 0 <= V < 1 and default 0.

The analytic setup uses escape radius 256 and capture radius 1.5, inside the horizon at r=2. These are current demonstration settings; they do not establish termination criteria for future numerical-relativity data.

Movie image sequences

Movie mode reads an observer-track CSV containing coordinate time, proper time, Cartesian position, and a full four-by-four tetrad (21 columns). The track must cover the requested frame times. The following generates a sample accelerating Minkowski trajectory and renders it against the 2MASS sky:

mkdir -p output/imgs
./build/Release/minkowski_sky --write-minkowski-accel-track output/minkowski_accel_2s.csv \
  --duration 2 --fps 30 --proper-acceleration 1.52
./build/Release/minkowski_sky --observer-track output/minkowski_accel_2s.csv \
  --all-sky-catalog assets/2mass/processed/all_sky \
  --frames-dir output/imgs --frames-prefix minkowski_accel \
  --start-time 0 --duration 2 --fps 30 --exposure 1e15

The inclusive time interval produces frames minkowski_accel_000000.png through minkowski_accel_000060.png. Exposure may need adjustment as Doppler shifts change the brightness. The trajectory generator is a flat-spacetime example; other camera motions are supplied through observer-track CSVs. Output is an image sequence; video encoding is a separate step.

Movie rays from all frames share a newest-to-oldest coordinate-time sweep. --slab-duration sets its time-slab width (default 64). The current analytic backends use logical slabs without metric I/O; Nmesh metric loading remains future work.

Reuse a completed lens map

--lens-map-output FILE saves the finalized inverse-lens mesh after tracing and refinement, while also rendering the image normally. It stores the geometry, frequency shifts, terminal statuses, triangle topology, and frame metadata in a versioned .grlens file. This allows later catalog, PSF, and exposure changes without repeating ray tracing.

mkdir -p output/imgs output/maps
./build/Release/schwarzschild_sky \
  --all-sky-catalog assets/2mass/processed/all_sky \
  --width 640 --height 360 --coarse-cell-pixels 8 --fov-deg 60 \
  --refine-max-level 2 --exposure 1e15 \
  --lens-map-output output/maps/schwarzschild.grlens \
  --output output/imgs/schwarzschild_trace.png
./build/Release/schwarzschild_sky \
  --lens-map-input output/maps/schwarzschild.grlens \
  --all-sky-catalog assets/2mass/processed/all_sky \
  --psf-fwhm-pixels 6 --psf-moffat-beta 3 --exposure 1e15 \
  --output output/imgs/schwarzschild_restyled.png

Import and export are mutually exclusive. Imported maps retain their original pixel dimensions, horizontal FOV, and mesh resolution; they cannot be refined on import. Explicit conflicting dimensions or FOV are rejected. The reader checks the format version, finite values, unit directions, triangle indices, and per-frame CRCs.

A movie export stores all final frame meshes in one file. To render it again, pass --lens-map-input FILE, the catalog, --frames-dir DIR, and --frames-prefix NAME; no observer track is needed on import.

Adaptive image mesh refinement

Adaptive refinement is disabled by default (--refine-max-level 0), so the existing coarse-mesh renders remain unchanged. When enabled, its defaults are an absolute direction error of 1e-3 degrees, relative error 0.1, minimum long edge 0.5 pixels, minimum area 0.25 pixel-squared, and a provisional minimum discrete-Jacobian magnitude of 1e-3. Each value can be overridden independently:

--refine-max-level N
--refine-angle-abs-deg D
--refine-angle-rel R
--refine-jacobian-min J
--refine-min-edge-pixels P
--refine-min-area-pixels2 A

N caps the triangle refinement level. Let e be the angle between the traced longest-edge midpoint direction and the normalized endpoint interpolation, and let s be the angle between those two endpoint camera directions. Both are evaluated internally in radians; the absolute CLI threshold D is specified in degrees and converted before comparison. s is the angular geometric size of the image triangle's test edge, not a source-sky/lens-map length. A locally escaped triangle is split only when both e > D_rad (the converted --refine-angle-abs-deg D) and e / max(s, 1e-15) > --refine-angle-rel. P and A prevent selecting a leaf already at or below the requested image-plane long-edge and area scales. Triangles whose three vertices disagree between capture and escape are split independently of the direction-error thresholds, allowing the mesh to follow a shadow boundary.

Independently of the midpoint geometry test, an all-escaped triangle also computes the discrete lens Jacobian J = Omega_source / Omega_image. Both signed solid angles use 2 atan2(dot(a, cross(b,c)), 1 + dot(a,b) + dot(b,c) + dot(c,a)), with the ordered camera directions for Omega_image and their traced infinity directions for Omega_source. A J-driven split requires both a shared image edge whose incident triangles have opposite nonzero signs of J and min(abs(J_left), abs(J_right)) < --refine-jacobian-min. It then requests that shared edge on both leaves. Thus |J| bounds the fold selection instead of widening it as a standalone critical-curve band. A negative sign is physical parity and is retained. The 1e-3 default is deliberately provisional and should be tuned with the small Schwarzschild refinement diagnostic before being treated as a production threshold.

For a small mesh diagnostic using the synthetic catalog:

./build/Release/schwarzschild_sky --catalog assets/sky_grid_5deg.csv \
  --width 48 --height 48 --coarse-cell-pixels 24 --fov-deg 40 \
  --refine-max-level 1 --refine-angle-abs-deg 0.001 \
  --refine-angle-rel 0.001 --refine-jacobian-min 0.001 \
  --refine-min-edge-pixels 1 \
  --refine-min-area-pixels2 1 --draw-mesh \
  --output output/imgs/schwarzschild_refinement.png

For movies, each refinement generation completes the full newest-to-oldest time-slab sweep before any probe becomes a mesh vertex. Newly added vertices are therefore traced only by the next generation; the renderer never returns to a slab that has already been released. At the start of every generation, newly inserted vertices and geometry-only longest-edge probes for its new leaves are collected together, so both ray sets use the same parallel RayPool pass.

Camera directions and optics

Catalog directions and --look-ra-deg/--look-dec-deg use standard right-handed ICRS Cartesian axes: +X is RA 0 degrees/Dec 0 degrees, +Y is RA 90 degrees/Dec 0 degrees, and +Z is the north celestial pole. The local camera axes are forward, celestial north, and celestial west, so an image with north up has decreasing RA to the right. The defaults preserve the original -Z view. --exposure converts a catalog's physical flux normalization to the prototype HDR scale. The current synthetic catalog is calibrated for default exposure 1e-3; a 2MASS blackbody normalization in steradians requires a much larger display exposure such as the example above. The optics path integrates each fitted Planck spectrum through CIE 1931 color-matching functions and converts the resulting radiance to linear sRGB; it does not use an empirical color-temperature RGB approximation.

Point sources use a flux-normalized circular Moffat PSF by default (--psf-fwhm-pixels 2.7 --psf-moffat-beta 4.5). The FWHM matches the former 1.15-pixel Gaussian core while the Moffat wings remain continuous; both values are display/optics calibration parameters.

The default renderer builds one immutable, process-wide 64-by-64 sub-pixel Moffat lookup kernel. Its weights are pixel-area integrals and are bilinearly interpolated between phase tables. The renderer reports its build time and cached/direct-fallback image counts. Pass --psf-direct to use the slower 8-point quadrature reference evaluator for regression comparisons; an image whose required HDR-tail support exceeds the cache radius selects that reference path automatically.

--psf-relative-tail R controls the maximum omitted PSF tail fraction per image; it defaults to 1e-8. Larger values intentionally shorten the Moffat support and rebuild the immutable cache at the corresponding radius, which is useful when a faster, lower-fidelity render is acceptable.

--psf-min-y Y defaults to 0 (disabled). A positive value is a linear-HDR luminance cutoff: a PSF stops where its continuous Moffat Y profile falls below Y, and an image whose central value is already below Y is omitted. The final PSF report counts such omitted events and emits a warning when any occur.

For bounded preview renders, --max-cache-psf-flux F (default 1) allows images with 1 < flux <= F to use the existing cache instead of the direct evaluator. This does not rebuild or enlarge the cache: the image retains its true core flux, color, and sub-pixel position, while its Moffat wing is clipped at the existing cache radius. Images above F retain the direct fallback. --max-magnification M (default unlimited) caps the per-triangle rendering magnification before flux is formed; it is an explicit preview approximation.

Progress and diagnostics

The PSF-cache completion line is printed before tracing and catalog splatting begin. For long renders, pass --verbose to print catalog-prefetch state, splat-worker local heartbeats (8, 16, 32, ... completed triangles per worker), and image-write boundaries. The worker heartbeats use neither global progress accounting nor cross-worker synchronization. Verbose ray-trace output reports the initial mesh trace and refinement stages for single frames; movie mode additionally reports each generation's sample count and each time slab's activation and terminal-ray summary. Movie renders always print one summary per time slab; --verbose also prints the ray counts before each slab is loaded.

Pass --draw-mesh to alpha-composite image-plane triangle edges as one-pixel-wide 0.5 linear-gray diagnostic lines at 0.5 opacity. The line rasterizer uses coverage-based antialiasing.

HDR output

To preserve a single-frame render for later exposure and tone-mapping work, build with ENABLE_HDR=1 as described in build.md. This produces build/Release/schwarzschild_sky, which accepts --hdr-output. This switch writes the HDR file next to the ordinary output, replacing its extension with _HDR.fits; for example, --output output/imgs/ring.png --hdr-output writes output/imgs/ring_HDR.fits. It writes the pre-tone-mapping RGB framebuffer as a three-plane, 32-bit float FITS image. Values remain linear HDR at the renderer's arbitrary scale; no tone mapping or per-frame normalization is applied. The ordinary binaries do not contain this option or writer.

The FITS header describes a synthetic 8640-by-5760, 36-by-24 mm full-frame sensor with 4.1667 um pixels. Each render records its active centered crop and derives FOCALLEN from that render's width and horizontal --fov-deg; these camera fields support plate-solving workflows but do not calibrate flux.