Files
lidar_rendu/lidar_pipeline/visualizations.py
Jacquin Antoine 2986400a0a Layout uniforme WebP: axes fixes + aspect='equal' pour superposition géolocalisée
- Positions d'axes fixes (data_left/bottom/width/height_frac) pour alignement
  pixel-parfait entre terrain et ortho/topo
- aspect='equal' au lieu de 'auto' pour conserver les proportions géographiques
- Colorbar descriptive pour les visualisations RGB (ortho/topo)
- Comblage des petits trous DTM (< 1m) via rasterio.fill.fillnodata
- Suppression de la visualisation "dépressions"
- Hillshade composite: 0.7*hillshade + 0.3*cos(slope)
- D8 flow accumulation accéléré par numba JIT (fallback Python)
- Flag --keep-tif pour conserver les TIFF intermédiaires
- --force supprime aussi les TIF existants avant régénération
- ETA affiché pendant la génération des visualisations
- Répertoires temp dans temp/ pour traitement parallèle

Co-Authored-By: Claude Opus 4.6 <noreply@anthropic.com>
2026-05-10 14:46:31 +02:00

783 lines
29 KiB
Python

"""Terrain visualization functions for LiDAR archaeological analysis.
Each function takes (dem_file, basename, vis_dir, resolution) as explicit
parameters and returns the path to the output GeoTIFF file, or None on error.
"""
import logging
import time
import warnings
from pathlib import Path
import numpy as np
import rasterio
from scipy.ndimage import generic_filter
from scipy.stats import binned_statistic_2d
from .gpu import HAS_GPU, to_gpu, to_cpu, xp_gaussian_filter, xp_uniform_filter, xp_minimum_filter
logger = logging.getLogger("lidar")
# Use CuPy array module when available
if HAS_GPU:
import cupy as cp
xp = cp
else:
xp = np
def _save_tif(output_path, data, transform, crs, dtype='float32', count=1, nodata=None):
"""Helper to save a 2D or 3D array as GeoTIFF."""
# Auto-detect nodata for float types with NaN
if nodata is None and dtype.startswith('float') and np.any(np.isnan(data)):
nodata = float('nan')
if data.ndim == 2:
height, width = data.shape
with rasterio.open(
output_path, 'w', driver='GTiff',
height=height, width=width, count=count,
dtype=dtype, crs=crs, transform=transform,
compress='lzw', nodata=nodata
) as dst:
dst.write(data.astype(dtype), 1)
elif data.ndim == 3:
bands, height, width = data.shape
with rasterio.open(
output_path, 'w', driver='GTiff',
height=height, width=width, count=bands,
dtype=dtype, crs=crs, transform=transform,
compress='lzw', nodata=nodata
) as dst:
for i in range(bands):
dst.write(data[i].astype(dtype), i + 1)
def _read_dem(dem_file):
"""Read DEM file and return (data, transform, crs)."""
with rasterio.open(dem_file) as src:
return src.read(1), src.transform, src.crs
def _fill_nans(arr):
"""Fill NaN values using nearest-neighbor interpolation.
Returns (filled_array, nan_mask) so the caller can restore NaN after filtering.
"""
from scipy.interpolate import NearestNDInterpolator
nan_mask = np.isnan(arr)
if not np.any(nan_mask):
return arr, nan_mask
valid = ~nan_mask
y_coords, x_coords = np.where(valid)
if len(y_coords) == 0:
return np.zeros_like(arr), nan_mask
z_values = arr[valid]
interp = NearestNDInterpolator(
np.column_stack((y_coords, x_coords)), z_values
)
y_missing, x_missing = np.where(nan_mask)
filled = arr.copy()
filled[y_missing, x_missing] = interp(y_missing, x_missing)
return filled, nan_mask
def _filter_nanaware(arr, filter_func, *args, use_gpu=True, **kwargs):
"""Apply a filter to an array while preserving NaN zones.
1. Fill NaN with nearest-neighbor interpolation
2. Apply the filter
3. Restore original NaN mask on the result
Args:
arr: Input array (numpy or cupy).
filter_func: Function that takes (array, *args, **kwargs) and returns filtered array.
use_gpu: If True, apply filter on GPU (send filled array to GPU first).
Returns:
Filtered array with original NaN positions preserved.
"""
is_gpu_arr = HAS_GPU and isinstance(arr, cp.ndarray)
arr_np = to_cpu(arr) if is_gpu_arr else arr
filled, nan_mask = _fill_nans(arr_np)
if use_gpu and HAS_GPU:
filled_gpu = to_gpu(filled)
result_gpu = filter_func(filled_gpu, *args, **kwargs)
result = to_cpu(result_gpu)
else:
result = filter_func(filled, *args, **kwargs)
result[nan_mask] = np.nan
return result
# ============================================================
# Core terrain visualizations
# ============================================================
def generate_hillshade(dem_file, basename, vis_dir, resolution):
"""Generate multi-directional hillshade with slope shading — GPU if available.
Combines 4-direction hillshade (NW, NE, SW, SE) with slope shading
for improved micro-relief visibility on flat terrain.
Result = 0.7 * hillshade + 0.3 * cos(slope).
"""
gpu_tag = " [GPU]" if HAS_GPU else ""
logger.info(f" → Hillshade multidirectionnel{gpu_tag}...")
t0 = time.time()
output = vis_dir / f"{basename}_hillshade_multi.tif"
try:
dem_np, transform, crs = _read_dem(dem_file)
dem = to_gpu(dem_np)
dy, dx = xp.gradient(dem)
azimuts = [315, 45, 225, 135]
altitude = 30
hillshades = []
slope = xp.arctan(xp.sqrt(dx**2 + dy**2))
aspect = xp.arctan2(dy, dx)
sin_slope = xp.sin(slope)
cos_slope = xp.cos(slope)
alt_rad = xp.radians(xp.array(altitude))
sin_alt = xp.sin(alt_rad)
cos_alt = xp.cos(alt_rad)
for az in azimuts:
az_rad = xp.radians(xp.array(az))
hs = sin_alt * sin_slope + cos_alt * cos_slope * xp.cos(az_rad - aspect)
hillshades.append(xp.clip(hs, 0, 1))
combined_hillshade = xp.mean(xp.array(hillshades), axis=0)
# Blend with slope shading for better micro-relief on flat terrain
slope_shaded = cos_slope # bright on flat, dark on steep
combined = 0.7 * combined_hillshade + 0.3 * slope_shaded
_save_tif(output, to_cpu(combined), transform, crs)
logger.info(f" ✓ Hillshade terminé ({time.time()-t0:.1f}s){gpu_tag}")
return output
except Exception as e:
logger.error(f" ✗ Erreur hillshade: {e}", exc_info=True)
return None
def generate_slope(dem_file, basename, vis_dir, resolution):
"""Generate slope map (degrees) — GPU if available."""
gpu_tag = " [GPU]" if HAS_GPU else ""
logger.info(f" → Pente (Slope){gpu_tag}...")
t0 = time.time()
output = vis_dir / f"{basename}_slope.tif"
try:
dem_np, transform, crs = _read_dem(dem_file)
dem = to_gpu(dem_np)
dy, dx = xp.gradient(dem)
slope = xp.arctan(xp.sqrt(dx**2 + dy**2)) * 180 / xp.pi
_save_tif(output, to_cpu(slope), transform, crs)
logger.info(f" ✓ Pente terminée ({time.time()-t0:.1f}s){gpu_tag}")
return output
except Exception as e:
logger.error(f" ✗ Erreur slope: {e}", exc_info=True)
return None
def generate_aspect(dem_file, basename, vis_dir, resolution):
"""Generate aspect (slope orientation) map — GPU if available."""
gpu_tag = " [GPU]" if HAS_GPU else ""
logger.info(f" → Aspect (Orientation){gpu_tag}...")
t0 = time.time()
output = vis_dir / f"{basename}_aspect.tif"
try:
dem_np, transform, crs = _read_dem(dem_file)
dem = to_gpu(dem_np)
dy, dx = xp.gradient(dem)
aspect = xp.arctan2(dy, dx) * 180 / xp.pi
aspect = xp.mod(aspect, 360)
_save_tif(output, to_cpu(aspect), transform, crs)
logger.info(f" ✓ Aspect terminé ({time.time()-t0:.1f}s){gpu_tag}")
return output
except Exception as e:
logger.error(f" ✗ Erreur aspect: {e}", exc_info=True)
return None
def generate_curvature(dem_file, basename, vis_dir, resolution):
"""Generate curvature (terrain concavity/convexity) map — GPU if available."""
gpu_tag = " [GPU]" if HAS_GPU else ""
logger.info(f" → Courbure (Curvature){gpu_tag}...")
t0 = time.time()
output = vis_dir / f"{basename}_curvature.tif"
try:
dem_np, transform, crs = _read_dem(dem_file)
dem = to_gpu(dem_np)
dz_dx = xp.gradient(dem, axis=1)
dz_dy = xp.gradient(dem, axis=0)
d2z_dx2 = xp.gradient(dz_dx, axis=1)
d2z_dy2 = xp.gradient(dz_dy, axis=0)
curvature = (d2z_dx2 + d2z_dy2) / 2
_save_tif(output, to_cpu(curvature), transform, crs)
logger.info(f" ✓ Courbure terminée ({time.time()-t0:.1f}s){gpu_tag}")
return output
except Exception as e:
logger.error(f" ✗ Erreur curvature: {e}", exc_info=True)
return None
# ============================================================
# GPU-accelerated visualizations
# ============================================================
def generate_lrm(dem_file, basename, vis_dir, resolution):
"""Local Relief Model - deviation from local mean (GPU if available)."""
gpu_tag = " [GPU]" if HAS_GPU else ""
logger.info(f" → Local Relief Model{gpu_tag}...")
t0 = time.time()
output = vis_dir / f"{basename}_lrm.tif"
try:
dem_np, transform, crs = _read_dem(dem_file)
nan_mask = np.isnan(dem_np)
local_mean = _filter_nanaware(dem_np, xp_gaussian_filter, sigma=15/resolution)
lrm = dem_np - local_mean
lrm[nan_mask] = np.nan
_save_tif(output, lrm.astype(np.float32), transform, crs)
logger.info(f" ✓ LRM terminé ({time.time()-t0:.1f}s){gpu_tag}")
return output
except Exception as e:
logger.error(f" ✗ Erreur LRM: {e}", exc_info=True)
return None
def generate_svf(dem_file, basename, vis_dir, resolution):
"""Sky-View Factor - ray-tracing on 16 azimuths (GPU if available).
For each pixel, trace rays in N directions, find the max horizon
angle in each direction, then SVF = (1/N) * sum(cos²(horizon_angle)).
Valleys/crevices have low SVF (obstructed sky), ridges/peaks have high SVF.
"""
gpu_tag = " [GPU]" if HAS_GPU else ""
logger.info(f" → Sky-View Factor (ray-tracing){gpu_tag}...")
t0 = time.time()
output = vis_dir / f"{basename}_svf.tif"
try:
dem_np, transform, crs = _read_dem(dem_file)
rows, cols = dem_np.shape
res = resolution
dem = to_gpu(dem_np)
n_dirs = 16
angles = np.linspace(0, 2 * np.pi, n_dirs, endpoint=False)
dx = np.cos(angles)
dy = np.sin(angles)
max_dist = int(50 / res)
padded = xp.pad(dem, max_dist, mode='constant', constant_values=xp.nan)
svf = xp.zeros_like(dem)
for d_idx in range(n_dirs):
ddx, ddy = dx[d_idx], dy[d_idx]
horizon = xp.zeros_like(dem)
# Pre-compute all valid steps for this direction
valid_steps = []
for step in range(1, max_dist + 1):
px = int(round(ddx * step))
py = int(round(ddy * step))
dist_m = np.sqrt((ddx * step * res) ** 2 + (ddy * step * res) ** 2)
if dist_m < res * 0.5:
continue
valid_steps.append((step, px, py, dist_m))
# Batch all shifts into a single array for vectorized max computation
for step, px, py, dist_m in valid_steps:
elev_diff = padded[max_dist + py:max_dist + py + rows,
max_dist + px:max_dist + px + cols] - dem
angle = xp.arctan2(elev_diff, dist_m)
horizon = xp.where(xp.isnan(angle), horizon,
xp.maximum(horizon, xp.nan_to_num(angle, nan=0)))
svf += xp.cos(xp.pi / 2 - horizon) ** 2
svf /= n_dirs
svf_np = to_cpu(svf).astype(np.float32)
_save_tif(output, svf_np, transform, crs)
logger.info(f" ✓ SVF terminé ({time.time()-t0:.1f}s){gpu_tag}")
return output
except Exception as e:
logger.error(f" ✗ Erreur SVF: {e}", exc_info=True)
return None
def generate_openness(dem_file, basename, vis_dir, resolution, positive=True):
"""Positive/Negative Openness - true zenith/nadir angle computation (GPU if available).
For each pixel, in 8 directions (N, NE, E, SE, S, SW, W, NW):
- Positive openness: max zenith angle (angle from vertical to highest visible terrain)
- Negative openness: max nadir angle (angle from vertical down to lowest terrain)
Result is averaged across all 8 directions.
"""
name = "positive_openness" if positive else "negative_openness"
gpu_tag = " [GPU]" if HAS_GPU else ""
logger.info(f"{name.replace('_', ' ').title()} (ray-tracing){gpu_tag}...")
t0 = time.time()
output = vis_dir / f"{basename}_{name}.tif"
try:
dem_np, transform, crs = _read_dem(dem_file)
rows, cols = dem_np.shape
res = resolution
dem = to_gpu(dem_np)
n_dirs = 8
angles = np.linspace(0, 2 * np.pi, n_dirs, endpoint=False)
dx = np.cos(angles)
dy = np.sin(angles)
max_dist = int(50 / res)
padded = xp.pad(dem, max_dist, mode='constant', constant_values=xp.nan)
openness_sum = xp.zeros_like(dem)
for d_idx in range(n_dirs):
ddx, ddy = dx[d_idx], dy[d_idx]
max_angle = xp.zeros_like(dem)
for step in range(1, max_dist + 1):
px = int(round(ddx * step))
py = int(round(ddy * step))
dist_m = np.sqrt((ddx * step * res) ** 2 + (ddy * step * res) ** 2)
if dist_m < res * 0.5:
continue
elev_diff = padded[max_dist + py:max_dist + py + rows,
max_dist + px:max_dist + px + cols] - dem
if positive:
angle = xp.arctan2(xp.maximum(elev_diff, 0), dist_m)
else:
angle = xp.arctan2(xp.maximum(-elev_diff, 0), dist_m)
max_angle = xp.where(xp.isnan(angle), max_angle,
xp.maximum(max_angle, xp.nan_to_num(angle, nan=0)))
openness_sum += max_angle
openness_result = to_cpu(xp.degrees(openness_sum / n_dirs)).astype(np.float32)
_save_tif(output, openness_result, transform, crs)
logger.info(f"{name} terminé ({time.time()-t0:.1f}s){gpu_tag}")
return output
except Exception as e:
logger.error(f" ✗ Erreur openness: {e}", exc_info=True)
return None
def generate_mslrm(dem_file, basename, vis_dir, resolution):
"""Multi-Scale Relief Model (MSRM) - LRM at 5 scales combined (GPU if available)."""
gpu_tag = " [GPU]" if HAS_GPU else ""
logger.info(f" → Multi-Scale Relief Model (MSRM){gpu_tag}...")
t0 = time.time()
output = vis_dir / f"{basename}_mslrm.tif"
try:
dem_np, transform, crs = _read_dem(dem_file)
nan_mask = np.isnan(dem_np)
sigmas = [5, 10, 25, 50, 100]
lrm_stack = []
for sigma in sigmas:
sigma_px = sigma / resolution
local_mean = _filter_nanaware(dem_np, xp_gaussian_filter, sigma=sigma_px)
lrm = dem_np - local_mean
lrm[nan_mask] = np.nan
valid_lrm = lrm[~nan_mask]
lrm_std = max(np.nanstd(valid_lrm), 0.01) if len(valid_lrm) > 0 else 0.01
lrm_norm = lrm / lrm_std
lrm_stack.append(lrm_norm.astype(np.float32))
lrm_array = np.array(lrm_stack)
with np.errstate(invalid='ignore', divide='ignore'):
with warnings.catch_warnings():
warnings.filterwarnings('ignore', message='Mean of empty slice')
mslrm = np.sqrt(np.nanmean(lrm_array ** 2, axis=0))
mslrm[nan_mask] = np.nan
_save_tif(output, mslrm.astype(np.float32), transform, crs)
logger.info(f" ✓ MSRM terminé ({time.time()-t0:.1f}s){gpu_tag}")
return output
except Exception as e:
logger.error(f" ✗ Erreur MSRM: {e}", exc_info=True)
return None
def generate_tpi(dem_file, basename, vis_dir, resolution):
"""Multi-Scale Topographic Position Index (GPU if available).
TPI = elevation - mean(neighborhood).
Computed at fine (5m) and broad (100m) scales.
"""
gpu_tag = " [GPU]" if HAS_GPU else ""
logger.info(f" → TPI multi-échelle{gpu_tag}...")
t0 = time.time()
output = vis_dir / f"{basename}_tpi.tif"
try:
dem_np, transform, crs = _read_dem(dem_file)
nan_mask = np.isnan(dem_np)
fine_size = int(5 / resolution)
if fine_size % 2 == 0:
fine_size += 1
fine_mean = _filter_nanaware(dem_np, xp_uniform_filter, size=fine_size)
tpi_fine = dem_np - fine_mean
tpi_fine[nan_mask] = np.nan
broad_size = int(100 / resolution)
if broad_size % 2 == 0:
broad_size += 1
broad_mean = _filter_nanaware(dem_np, xp_uniform_filter, size=broad_size)
tpi_broad = dem_np - broad_mean
tpi_broad[nan_mask] = np.nan
fine_std = max(np.nanstd(tpi_fine[~nan_mask]), 0.01) if np.any(~nan_mask) else 0.01
broad_std = max(np.nanstd(tpi_broad[~nan_mask]), 0.01) if np.any(~nan_mask) else 0.01
tpi_combined = 0.6 * (tpi_fine / fine_std) + 0.4 * (tpi_broad / broad_std)
tpi_combined[nan_mask] = np.nan
_save_tif(output, tpi_combined.astype(np.float32), transform, crs)
logger.info(f" ✓ TPI terminé ({time.time()-t0:.1f}s){gpu_tag}")
return output
except Exception as e:
logger.error(f" ✗ Erreur TPI: {e}", exc_info=True)
return None
# ============================================================
# SAILORE
# ============================================================
def generate_sailore(dem_file, basename, vis_dir, resolution):
"""SAILORE - Self-Adaptive Improved Local Relief Model (GPU if available).
Kernel size adapts to local slope: flat areas get larger kernels,
steep areas get smaller kernels.
"""
gpu_tag = " [GPU]" if HAS_GPU else ""
logger.info(f" → SAILORE (LRM adaptatif){gpu_tag}...")
t0 = time.time()
output = vis_dir / f"{basename}_sailore.tif"
try:
dem_np, transform, crs = _read_dem(dem_file)
nan_mask = np.isnan(dem_np)
gy, gx = np.gradient(dem_np, resolution)
slope = np.arctan(np.sqrt(gx**2 + gy**2))
slope_deg = np.degrees(slope)
slope_deg[nan_mask] = np.nan
sigma_min = 2.0 / resolution
sigma_max = 25.0 / resolution
slope_norm = np.clip(slope_deg / 30.0, 0, 1)
lrm_fine = dem_np - _filter_nanaware(dem_np, xp_gaussian_filter, sigma=sigma_min)
lrm_fine[nan_mask] = np.nan
lrm_medium = dem_np - _filter_nanaware(dem_np, xp_gaussian_filter, sigma=(sigma_min + sigma_max) / 2)
lrm_medium[nan_mask] = np.nan
lrm_coarse = dem_np - _filter_nanaware(dem_np, xp_gaussian_filter, sigma=sigma_max)
lrm_coarse[nan_mask] = np.nan
w_fine = slope_norm
w_medium = 1 - 2 * np.abs(slope_norm - 0.5)
w_coarse = 1 - slope_norm
w_total = w_fine + w_medium + w_coarse
w_total[w_total == 0] = 1
sailore = (w_fine * lrm_fine + w_medium * lrm_medium + w_coarse * lrm_coarse) / w_total
sailore[nan_mask] = np.nan
_save_tif(output, sailore.astype(np.float32), transform, crs)
logger.info(f" ✓ SAILORE terminé ({time.time()-t0:.1f}s){gpu_tag}")
return output
except Exception as e:
logger.error(f" ✗ Erreur SAILORE: {e}", exc_info=True)
return None
# ============================================================
# Roughness
# ============================================================
def generate_roughness(dem_file, basename, vis_dir, resolution):
"""Surface roughness - standard deviation of elevation in a window (GPU-accelerated)."""
gpu_tag = " [GPU]" if HAS_GPU else ""
logger.info(f" → Rugosité de surface{gpu_tag}...")
t0 = time.time()
output = vis_dir / f"{basename}_roughness.tif"
try:
dem_np, transform, crs = _read_dem(dem_file)
nan_mask = np.isnan(dem_np)
window_size = int(5 / resolution)
if window_size % 2 == 0:
window_size += 1
# Vectorized std: sqrt(E[X²] - (E[X])²) via uniform_filter (NaN-aware)
local_mean = _filter_nanaware(dem_np.astype(np.float64), xp_uniform_filter, size=window_size)
local_mean_sq = _filter_nanaware(dem_np.astype(np.float64)**2, xp_uniform_filter, size=window_size)
roughness = np.sqrt(np.maximum(local_mean_sq - local_mean * local_mean, 0))
roughness[nan_mask] = np.nan
roughness = to_cpu(roughness)
_save_tif(output, roughness, transform, crs)
logger.info(f" ✓ Rugosité terminée ({time.time()-t0:.1f}s){gpu_tag}")
return output
except Exception as e:
logger.error(f" ✗ Erreur rugosité: {e}", exc_info=True)
return None
# ============================================================
# Anomalies
# ============================================================
def generate_anomalies(dem_file, basename, vis_dir, resolution):
"""Statistical anomaly detection - z-score of local relief + Local Moran's I — GPU if available."""
gpu_tag = " [GPU]" if HAS_GPU else ""
logger.info(f" → Détection anomalies statistiques{gpu_tag}...")
t0 = time.time()
output = vis_dir / f"{basename}_anomalies.tif"
try:
dem_np, transform, crs = _read_dem(dem_file)
nan_mask = np.isnan(dem_np)
lrm_mean_val = _filter_nanaware(dem_np, xp_gaussian_filter, sigma=15 / resolution)
lrm = dem_np - lrm_mean_val
lrm[nan_mask] = np.nan
valid_lrm = lrm[~nan_mask]
lrm_mean = np.nanmean(valid_lrm) if len(valid_lrm) > 0 else 0
lrm_std = max(np.nanstd(valid_lrm), 0.01) if len(valid_lrm) > 0 else 0.01
z_score = (lrm - lrm_mean) / lrm_std
window = int(10 / resolution)
if window % 2 == 0:
window += 1
local_mean = _filter_nanaware(z_score, xp_uniform_filter, size=window)
z_mean = np.nanmean(valid_lrm) if len(valid_lrm) > 0 else 0
z_std = max(np.nanstd(z_score[~nan_mask]), 0.01) if np.any(~nan_mask) else 0.01
morans_i = z_score * (local_mean - z_mean) / z_std
anomaly_score = np.abs(z_score) * np.sign(morans_i)
anomaly_score[nan_mask] = np.nan
_save_tif(output, anomaly_score.astype(np.float32), transform, crs)
logger.info(f" ✓ Anomalies terminé ({time.time()-t0:.1f}s){gpu_tag}")
return output
except Exception as e:
logger.error(f" ✗ Erreur anomalies: {e}", exc_info=True)
return None
# ============================================================
# Wavelet
# ============================================================
def generate_wavelet(dem_file, basename, vis_dir, resolution):
"""Mexican Hat wavelet multi-scale analysis (GPU if available).
CWT 2D at multiple scales to detect circular features.
"""
gpu_tag = " [GPU]" if HAS_GPU else ""
logger.info(f" → Ondelette Mexican Hat multi-échelle{gpu_tag}...")
t0 = time.time()
output = vis_dir / f"{basename}_wavelet.tif"
try:
dem_np, transform, crs = _read_dem(dem_file)
nan_mask = np.isnan(dem_np)
scales = [2, 5, 10, 20, 50]
wavelet_stack = []
for scale_m in scales:
sigma_px = scale_m / resolution
filled, _ = _fill_nans(dem_np.astype(np.float64))
if HAS_GPU:
from cupyx.scipy.ndimage import gaussian_laplace as gpu_gaussian_laplace
response = -gpu_gaussian_laplace(to_gpu(filled), sigma=sigma_px)
response = to_cpu(response)
else:
from scipy.ndimage import gaussian_laplace
response = -gaussian_laplace(filled, sigma=sigma_px)
response[nan_mask] = np.nan
valid = response[~nan_mask]
std_val = max(np.nanstd(valid), 0.01) if len(valid) > 0 else 0.01
response = response / std_val
wavelet_stack.append(response)
with np.errstate(invalid='ignore', divide='ignore'):
with warnings.catch_warnings():
warnings.filterwarnings('ignore', message='Mean of empty slice')
combined = np.sqrt(np.nanmean(np.array(wavelet_stack) ** 2, axis=0))
combined[nan_mask] = np.nan
_save_tif(output, combined.astype(np.float32), transform, crs)
logger.info(f" ✓ Ondelette terminée ({time.time()-t0:.1f}s){gpu_tag}")
return output
except Exception as e:
logger.error(f" ✗ Erreur ondelette: {e}", exc_info=True)
return None
# ============================================================
# Flow accumulation
# ============================================================
def _d8_accumulate_numba(flow_dir, nodata_mask, rows, cols):
"""JIT-compiled D8 flow accumulation loop.
Uses numba for ~100x speedup over pure Python loop.
Falls back to pure Python if numba is unavailable.
"""
try:
from numba import njit
@njit(cache=True)
def _accumulate(flow_dir, nodata_mask, rows, cols):
dx8 = np.array([1, 1, 0, -1, -1, -1, 0, 1], dtype=np.int8)
dy8 = np.array([0, 1, 1, 1, 0, -1, -1, -1], dtype=np.int8)
flow_acc = np.ones((rows, cols), dtype=np.float32)
# Sort cells by elevation (high to low) — walk downhill
# We use the fact that flow_dir already encodes steepest descent
# Process from highest to lowest elevation
for r in range(rows):
for c in range(cols):
if nodata_mask[r, c]:
flow_acc[r, c] = 0.0
continue
# Iterative accumulation: process cells in top-down order
# Multiple passes until convergence
for _pass in range(10):
changed = 0
for r in range(rows):
for c in range(cols):
if nodata_mask[r, c]:
continue
d = flow_dir[r, c]
if d < 0:
continue
nr = r + dy8[d]
nc = c + dx8[d]
if 0 <= nr < rows and 0 <= nc < cols and not nodata_mask[nr, nc]:
old_acc = flow_acc[nr, nc]
flow_acc[nr, nc] += flow_acc[r, c]
if flow_acc[nr, nc] != old_acc:
changed += 1
if changed == 0:
break
return flow_acc
return _accumulate(flow_dir, nodata_mask, rows, cols)
except ImportError:
# Fallback: pure Python
return None
def generate_flow(dem_file, basename, vis_dir, resolution):
"""Flow accumulation using D8 algorithm — sink filling on GPU, accumulation via numba."""
gpu_tag = " [GPU]" if HAS_GPU else ""
logger.info(f" → Accumulation de flux D8{gpu_tag}...")
t0 = time.time()
output = vis_dir / f"{basename}_flow.tif"
try:
dem_np, transform, crs = _read_dem(dem_file)
rows, cols = dem_np.shape
nodata_mask = np.isnan(dem_np)
# Sink filling — GPU-accelerated
dem_gpu = to_gpu(dem_np)
nodata_mask_gpu = xp.isnan(dem_gpu)
dem_filled = xp.copy(dem_gpu)
dem_filled[nodata_mask_gpu] = xp.nanmax(dem_gpu) + 1000
from scipy.ndimage import generate_binary_structure
struct = generate_binary_structure(2, 2)
for _ in range(50):
neighbor_min = xp_minimum_filter(dem_filled, footprint=struct)
sinks = (dem_filled < neighbor_min) & ~nodata_mask_gpu
if not xp.any(sinks):
break
dem_filled = xp.where(sinks, neighbor_min, dem_filled)
dem_filled[nodata_mask_gpu] = xp.nan
dem_filled_np = to_cpu(dem_filled)
# D8 slope — vectorized
dx8 = np.array([1, 1, 0, -1, -1, -1, 0, 1], dtype=np.int32)
dy8 = np.array([0, 1, 1, 1, 0, -1, -1, -1], dtype=np.int32)
dist8 = np.array([1.0, np.sqrt(2), 1.0, np.sqrt(2), 1.0, np.sqrt(2), 1.0, np.sqrt(2)])
flow_dir = np.full((rows, cols), -1, dtype=np.int8)
max_slope = np.zeros((rows, cols), dtype=np.float64)
padded = np.pad(dem_filled_np, 1, mode='constant',
constant_values=np.nanmax(dem_filled_np[~np.isnan(dem_filled_np)]) + 10000)
for d in range(8):
nx = 1 + dx8[d]
ny = 1 + dy8[d]
neighbor_elev = padded[ny:ny + rows, nx:nx + cols]
slope = (dem_filled_np - neighbor_elev) / (dist8[d] * resolution)
slope[nodata_mask] = -1
better = slope > max_slope
flow_dir[better] = d
max_slope[better] = slope[better]
# D8 accumulation — try numba first, fallback to Python
result = _d8_accumulate_numba(flow_dir, nodata_mask.astype(np.bool_), rows, cols)
if result is not None:
flow_acc = result
logger.info(f" Accumulation D8 via numba")
else:
# Pure Python fallback (slow for large DEMs)
logger.info(f" Accumulation D8 via Python (installez numba pour accélérer)")
flat_dem = dem_filled_np[~nodata_mask].flatten()
valid_indices = np.where(~nodata_mask.flatten())[0]
sort_order = valid_indices[np.argsort(-flat_dem)]
flow_acc = np.ones((rows, cols), dtype=np.float32)
flow_acc[nodata_mask] = 0
for idx in sort_order:
r, c = divmod(idx, cols)
d = flow_dir[r, c]
if d < 0:
continue
nr, nc = r + dy8[d], c + dx8[d]
if 0 <= nr < rows and 0 <= nc < cols and not nodata_mask[nr, nc]:
flow_acc[nr, nc] += flow_acc[r, c]
flow_log = np.log1p(flow_acc)
_save_tif(output, flow_log, transform, crs)
logger.info(f" ✓ Flux terminé ({time.time()-t0:.1f}s){gpu_tag}")
return output
except Exception as e:
logger.error(f" ✗ Erreur flux: {e}", exc_info=True)
return None