GitLab

Summary:
Adds `grid_scatter` op that is similar to `grid_sample` but the grid points to the destination location instead of the source.

`grid_scatter` is indeed dual to `grid_sample`. Forward of `grid_scatter` is backward of `grid_sample` and backward of  `grid_scatter` is forward of `grid_sample` (with the exception for the gradient with respect to grid) which is reflected in the reference implementation in `drtk/grid_scatter.py`.

```python
def grid_scatter(
    input: th.Tensor,
    grid: th.Tensor,
    output_height: int,
    output_width: int,
    mode: str = "bilinear",
    padding_mode: str = "border",
    align_corners: Optional[bool] = None,
) -> th.Tensor:
```

Where :
* `input` [N x C x H x W]: is the input tensor values from which will be transferred to the result.
* `grid` [N x H x W x 2]: is the grid tensor that points to the location where the values from the  input tensor should be copied to. The `W`, `H` sizes of grid should match the corresponding sizes of the `input` tensor.
*  `output_height`, `output_width`: size of the output, where output will be: [N x C x `output_height` x `output_width`]. In contrast to `grid_sample`, we can no longer rely on the sizes of the `grid` for this information.
* `mode`, `padding_mode`, `align_corners` same as for the `grid_sample`, but now for the reverse operation - splatting (or scattering).

At the moment does not support "nearest" mode, which is rarely needed. Maybe will add later.

Ideally, we would also want to support autocast mode where the `input` and output tensors are float16 while the `grid` is float32. This is not the case at the moment, but I'll add that later.

## Example usage

Let's assume that we loaded mesh into `v, vi, vt, vti`, have defined `image_width, image_height`, `cam_pos`, `cam_rot`, `focal`, `princpt`, and computed normals for the mesh `normals`. We also define a shading function, e.g.:

```lang=python
def shade(
    vn_img: th.Tensor,
    light_dir: th.Tensor,
    ambient_intensity: float = 1.0,
    direct_intensity: float = 1.0,
    shadow_img: Optional[th.Tensor] = None,
):
    ambient = (vn_img[:, 1:2] * 0.5 + 0.5) * th.as_tensor([0.45, 0.5, 0.7]).cuda()[
        None, :, None, None
    ]
    direct = (
        th.sum(vn_img.mul(thf.normalize(light_dir, dim=1)), dim=1, keepdim=True).clamp(
            min=0.0
        )
        * th.as_tensor([0.65, 0.6, 0.5]).cuda()[None, :, None, None]
    )
    if shadow_img is not None:
        direct = direct * shadow_img
    return th.pow(ambient * ambient_intensity + direct * direct_intensity, 1 / 2.2)
```

And we can render the image as:

```lang=python
v_pix = transform(v, cam_pos, cam_rot, focal, princpt)
index_img = rasterize(v_pix, vi, image_height, image_width)
_, bary_img = render(v_pix, vi, index_img)

# mask image
mask: th.Tensor = (index_img != -1)[:, None]

# compute vt image
vt_img = interpolate(vt.mul(2.0).sub(1.0)[None], vti, index_img, bary_img)

# compute normals
vn_img = interpolate(normals, vi, index_img, bary_img)

diffuse = (
    shade(vn_img, th.as_tensor([0.5, 0.5, 0.0]).cuda()[None, :, None, None]) * mask
)
```

 {F1801805545}

## Shadow mapping

We can use  `grid_scatter` to compute mesh visibility from the camera view:

```lang=python
texel_weight = grid_scatter(
    mask.float(),
    vt_img.permute(0, 2, 3, 1),
    output_width=512,
    output_height=512,
    mode="bilinear",
    padding_mode="border",
    align_corners=False,
)
threshold = 0.1  # texel_weight is proportional to how much pixel are the texel covers. We can specify a threshold of how much covered pixel area counts as visible.
visibility = (texel_weight > threshold).float()
```
 {F1801810094}

Now we can render the scene from different angle and use the visibility mask for shadows:

```lang=python
v_pix = transform(v, cam_pos_new, cam_rot_new, focal, princpt)
index_img = rasterize(v_pix, vi, image_height, image_width)
_, bary_img = render(v_pix, vi, index_img)

# mask image
mask: th.Tensor = (index_img != -1)[:, None]

# compute vt image
vt_img = interpolate(vt.mul(2.0).sub(1.0)[None], vti, index_img, bary_img)

# compute v image (for near-field)
v_img = interpolate(v, vi, index_img, bary_img)

# shadow
shadow_img = thf.grid_sample(visibility, vt_img.permute(0, 2, 3, 1), mode="bilinear", padding_mode="border", align_corners=False)

# compute normals
vn_img = interpolate(normals, vi, index_img, bary_img)

diffuse = shade(vn_img, cam_pos[:, :, None, None] - v_img, 0.05, 0.4, shadow_img) * mask
```
 {F1801811232}

## Texture projection

Let's load a test image:

```lang=python
import skimage
test_image = (
    th.as_tensor(skimage.data.coffee(), dtype=th.float32).permute(2, 0, 1)[None, ...].mul(1 / 255).contiguous().cuda()
)

test_image = thf.interpolate(test_image, scale_factor=2.0, mode="bilinear", align_corners=False)
```

{F1801814094}

We can use `grid_scatter` to project the image onto the uv space:

```lang=python
camera_image_extended = (
    th.cat([test_image, th.ones_like(test_image[:, :1])], dim=1) * mask
)

texture_weight = grid_scatter(
    camera_image_extended,
    vt_img.permute(0, 2, 3, 1),
    output_width=512,
    output_height=512,
    mode="bilinear",
    padding_mode="border",
    align_corners=False,
)

texture = texture_weight[:, :3] / texture_weight[:, 3:4].clamp(min=1e-4)
```

{F1801816367}

And if we render the scene from a different angle using the projected texture:

 {F1801817130}

Reviewed By: HapeMask

Differential Revision: D61006613

fbshipit-source-id: 98c83ba4eda531e9d73cb9e533176286dc699f63

Summary:
For unused warps we always write zeros to `bary_img_grad`.
However it is possible that the warp is used, but only portion of the threads are used. In this case, for unused threads we do not write zeros to `bary_img_grad`.

For efficiency, `bary_img_grad` is created with `at::empty`, thus  those before mentioned entries, will still have uninitialized values.

This is not an issue, because the `render` function will never read those entries, however it is possible that the uninitialized values will coincide with `nan` and it will trigger a false positive detection in auto grad anomaly detection.  Please see more details in D60904848 about the issue.

Differential Revision: D60912474

fbshipit-source-id: 6eda5a07789db456c17eb60de222dd4c7b1c53d2

Summary:
Apply fisheye62 distortion to HQLP camera renders.

Visualization of results. 4 rows are in order: HMC, drtk render, pixel render, pinhole img.

https://www.internalfb.com/manifold/explorer/codec-avatars-scratch/tree/hmc_nvs/20240516_rosetta_nearfield/runs/TEST_run_hqlp_rosetta_render_ojwang_v0719_002/dome_hmc_nvs_render/MLU130_20220509--0000_codec/vrs_comparison/000002__MLU130-brows_lowered-2022-05-09-16-08-12.png

Debug distortion document, tracked the work: https://docs.google.com/document/d/1nSnFMrGWXVoICDEstpL9JZAnRtiuSMnWjnfGDzIfrNE/edit?pli=1

Reviewed By: euclid1767

Differential Revision: D58825272

fbshipit-source-id: 463f8c60014bd9cde898d72875bec49ffc75e453

Summary: In order to work properly with `torch.compile()`, we need to decorate any function that calls a custom C++/CUDA extension with `torch.compiler.disable` so that it knows to insert a graph break.

Reviewed By: podgorskiy

Differential Revision: D59776177

fbshipit-source-id: d80eb43858836f8b8647d2a35b30d0b863989e94

Summary: Created from CodeHub with https://fburl.com/edit-in-codehub

Reviewed By: una-dinosauria

Differential Revision: D58369133

fbshipit-source-id: cf6a0e4710be579f60f6d569d23c50183dfd6018

Summary: Created from CodeHub with https://fburl.com/edit-in-codehub

Reviewed By: tsimk

Differential Revision: D58368652

fbshipit-source-id: 8f3f426f0825255e5e6d6b32b8f1bdb2cde6e161

fbshipit-source-id: afc575e8e7d8e2796a3f77d8b1c6c4fcb999558d