Source code for polsartools.polsar.cp.mf3cc

import os
import numpy as np
from polsartools.utils.proc_utils import process_chunks_parallel
from polsartools.utils.utils import conv2d,time_it
from .cp_infiles import cpc2files
[docs] @time_it def mf3cc(in_dir, chi=45, psi=0, win=1, fmt="tif", cog=False, ovr = [2, 4, 8, 16], comp=False, max_workers=None,block_size=(512, 512), progress_callback=None # for QGIS plugin ): """Perform Model-Free 3-Component Decomposition for compact-pol SAR data. This function implements the model-free three-component decomposition for compact-polarimetric SAR data, decomposing the total backscattered power into surface (Ps), double-bounce (Pd), and volume (Pv) scattering components, along with the scattering-type parameter (Theta_CP). Examples -------- >>> # Basic usage with default parameters >>> mf3cc("/path/to/cp_data") >>> # Advanced usage with custom parameters >>> mf3cc( ... in_dir="/path/to/cp_data", ... chi=-45, ... win=5, ... fmt="tif", ... cog=True, ... block_size=(1024, 1024) ... ) Parameters ---------- in_dir : str Path to the input folder containing compact-pol C2 matrix files. chi : float, default=45 Ellipticity angle chi of the transmitted wave in degrees. For circular polarization, chi = 45° (right circular) or -45° (left circular). psi : float, default=0 Orientation angle psi of the transmitted wave in degrees. For circular polarization, typically 0°. win : int, default=1 Size of the spatial averaging window. Larger windows reduce speckle noise but decrease spatial resolution. fmt : {'tif', 'bin'}, default='tif' Output file format: - 'tif': GeoTIFF format with georeferencing information - 'bin': Raw binary format cog : bool, default=False If True, creates Cloud Optimized GeoTIFF (COG) outputs with internal tiling and overviews for efficient web access. ovr : list[int], default=[2, 4, 8, 16] Overview levels for COG creation. Each number represents the decimation factor for that overview level. comp : bool, default=False If True, applies LZW compression to the output GeoTIFF files. max_workers : int | None, default=None Maximum number of parallel processing workers. If None, uses CPU count - 1 workers. block_size : tuple[int, int], default=(512, 512) Size of processing blocks (rows, cols) for parallel computation. Larger blocks use more memory but may be more efficient. Returns ------- None Writes four output files to disk: 1. Ps_mf3cc: Surface scattering power component 2. Pd_mf3cc: Double-bounce scattering power component 3. Pv_mf3cc: Volume scattering power component 4. Theta_CP_mf3cc: Scattering-type parameter """ write_flag=True input_filepaths = cpc2files(in_dir) output_filepaths = [] if fmt == "bin": output_filepaths.append(os.path.join(in_dir, "Ps_mf3cc.bin")) output_filepaths.append(os.path.join(in_dir, "Pd_mf3cc.bin")) output_filepaths.append(os.path.join(in_dir, "Pv_mf3cc.bin")) output_filepaths.append(os.path.join(in_dir, "Theta_CP_mf3cc.bin")) else: output_filepaths.append(os.path.join(in_dir, "Ps_mf3cc.tif")) output_filepaths.append(os.path.join(in_dir, "Pd_mf3cc.tif")) output_filepaths.append(os.path.join(in_dir, "Pv_mf3cc.tif")) output_filepaths.append(os.path.join(in_dir, "Theta_CP_mf3cc.tif")) process_chunks_parallel(input_filepaths, list(output_filepaths), win, write_flag, process_chunk_mf3cc, *[chi, psi], block_size=block_size, max_workers=max_workers, num_outputs=len(output_filepaths), cog=cog, ovr=ovr, comp=comp, progress_callback=progress_callback )
def process_chunk_mf3cc(chunks, window_size, *args, **kwargs): chi=args[-2] psi=args[-1] # print(chi,psi): kernel = np.ones((window_size,window_size),np.float32)/(window_size*window_size) c11_T1 = np.array(chunks[0]) c12_T1 = np.array(chunks[1])+1j*np.array(chunks[2]) c21_T1 = np.conj(c12_T1) c22_T1 = np.array(chunks[3]) ncols,nrows = np.shape(c11_T1) if window_size>1: c11_T1 = conv2d(np.real(c11_T1),kernel)+1j*conv2d(np.imag(c11_T1),kernel) c12_T1 = conv2d(np.real(c12_T1),kernel)+1j*conv2d(np.imag(c12_T1),kernel) c21_T1 = conv2d(np.real(c21_T1),kernel)+1j*conv2d(np.imag(c21_T1),kernel) c22_T1 = conv2d(np.real(c22_T1),kernel)+1j*conv2d(np.imag(c22_T1),kernel) c2_det = (c11_T1*c22_T1-c12_T1*c21_T1) c2_trace = c11_T1+c22_T1 # t2_span = t11s*t22s m1 = np.real(np.sqrt(1.0-(4.0*c2_det/np.power(c2_trace,2)))) # Compute Stokes parameters s0 = c11_T1 + c22_T1 s1 = c11_T1 - c22_T1 s2 = np.real(c12_T1 + c21_T1) s3 = np.where(chi >= 0, 1j * (c12_T1 - c21_T1), -1j * (c12_T1 - c21_T1)) s3 = np.real(s3) SC = ((s0)-(s3))/2; OC = ((s0)+(s3))/2; h = (OC-SC) # span = c11s + c22s val = ((m1*s0*h))/((SC*OC + (m1**2)*(s0**2))) thet = np.real(np.arctan(val)) theta_CP = np.rad2deg(thet) Ps_CP= (((m1*(c2_trace)*(1.0+np.sin(2*thet))/2))) Pd_CP= (((m1*(c2_trace)*(1.0-np.sin(2*thet))/2))) Pv_CP= (c2_trace*(1.0-m1)) return Ps_CP.astype(np.float32), Pd_CP.astype(np.float32), Pv_CP.astype(np.float32), theta_CP.astype(np.float32)