libcamera/utils/raspberrypi/ctt/ctt_alsc.py
Laurent Pinchart 626172a16b libcamera: Drop file name from header comment blocks
Source files in libcamera start by a comment block header, which
includes the file name and a one-line description of the file contents.
While the latter is useful to get a quick overview of the file contents
at a glance, the former is mostly a source of inconvenience. The name in
the comments can easily get out of sync with the file name when files
are renamed, and copy & paste during development have often lead to
incorrect names being used to start with.

Readers of the source code are expected to know which file they're
looking it. Drop the file name from the header comment block.

The change was generated with the following script:

----------------------------------------

dirs="include/libcamera src test utils"

declare -rA patterns=(
	['c']=' \* '
	['cpp']=' \* '
	['h']=' \* '
	['py']='# '
	['sh']='# '
)

for ext in ${!patterns[@]} ; do
	files=$(for dir in $dirs ; do find $dir -name "*.${ext}" ; done)
	pattern=${patterns[${ext}]}

	for file in $files ; do
		name=$(basename ${file})
		sed -i "s/^\(${pattern}\)${name} - /\1/" "$file"
	done
done
----------------------------------------

This misses several files that are out of sync with the comment block
header. Those will be addressed separately and manually.

Signed-off-by: Laurent Pinchart <laurent.pinchart@ideasonboard.com>
Reviewed-by: Daniel Scally <dan.scally@ideasonboard.com>
2024-05-08 22:39:50 +03:00

299 lines
9.9 KiB
Python

# SPDX-License-Identifier: BSD-2-Clause
#
# Copyright (C) 2019, Raspberry Pi Ltd
#
# camera tuning tool for ALSC (auto lens shading correction)
from ctt_image_load import *
import matplotlib.pyplot as plt
from matplotlib import cm
from mpl_toolkits.mplot3d import Axes3D
"""
preform alsc calibration on a set of images
"""
def alsc_all(Cam, do_alsc_colour, plot):
imgs_alsc = Cam.imgs_alsc
"""
create list of colour temperatures and associated calibration tables
"""
list_col = []
list_cr = []
list_cb = []
list_cg = []
for Img in imgs_alsc:
col, cr, cb, cg, size = alsc(Cam, Img, do_alsc_colour, plot)
list_col.append(col)
list_cr.append(cr)
list_cb.append(cb)
list_cg.append(cg)
Cam.log += '\n'
Cam.log += '\nFinished processing images'
w, h, dx, dy = size
Cam.log += '\nChannel dimensions: w = {} h = {}'.format(int(w), int(h))
Cam.log += '\n16x12 grid rectangle size: w = {} h = {}'.format(dx, dy)
"""
convert to numpy array for data manipulation
"""
list_col = np.array(list_col)
list_cr = np.array(list_cr)
list_cb = np.array(list_cb)
list_cg = np.array(list_cg)
cal_cr_list = []
cal_cb_list = []
"""
only do colour calculations if required
"""
if do_alsc_colour:
Cam.log += '\nALSC colour tables'
for ct in sorted(set(list_col)):
Cam.log += '\nColour temperature: {} K'.format(ct)
"""
average tables for the same colour temperature
"""
indices = np.where(list_col == ct)
ct = int(ct)
t_r = np.mean(list_cr[indices], axis=0)
t_b = np.mean(list_cb[indices], axis=0)
"""
force numbers to be stored to 3dp.... :(
"""
t_r = np.where((100*t_r) % 1 <= 0.05, t_r+0.001, t_r)
t_b = np.where((100*t_b) % 1 <= 0.05, t_b+0.001, t_b)
t_r = np.where((100*t_r) % 1 >= 0.95, t_r-0.001, t_r)
t_b = np.where((100*t_b) % 1 >= 0.95, t_b-0.001, t_b)
t_r = np.round(t_r, 3)
t_b = np.round(t_b, 3)
r_corners = (t_r[0], t_r[15], t_r[-1], t_r[-16])
b_corners = (t_b[0], t_b[15], t_b[-1], t_b[-16])
r_cen = t_r[5*16+7]+t_r[5*16+8]+t_r[6*16+7]+t_r[6*16+8]
r_cen = round(r_cen/4, 3)
b_cen = t_b[5*16+7]+t_b[5*16+8]+t_b[6*16+7]+t_b[6*16+8]
b_cen = round(b_cen/4, 3)
Cam.log += '\nRed table corners: {}'.format(r_corners)
Cam.log += '\nRed table centre: {}'.format(r_cen)
Cam.log += '\nBlue table corners: {}'.format(b_corners)
Cam.log += '\nBlue table centre: {}'.format(b_cen)
cr_dict = {
'ct': ct,
'table': list(t_r)
}
cb_dict = {
'ct': ct,
'table': list(t_b)
}
cal_cr_list.append(cr_dict)
cal_cb_list.append(cb_dict)
Cam.log += '\n'
else:
cal_cr_list, cal_cb_list = None, None
"""
average all values for luminance shading and return one table for all temperatures
"""
lum_lut = np.mean(list_cg, axis=0)
lum_lut = np.where((100*lum_lut) % 1 <= 0.05, lum_lut+0.001, lum_lut)
lum_lut = np.where((100*lum_lut) % 1 >= 0.95, lum_lut-0.001, lum_lut)
lum_lut = list(np.round(lum_lut, 3))
"""
calculate average corner for lsc gain calculation further on
"""
corners = (lum_lut[0], lum_lut[15], lum_lut[-1], lum_lut[-16])
Cam.log += '\nLuminance table corners: {}'.format(corners)
l_cen = lum_lut[5*16+7]+lum_lut[5*16+8]+lum_lut[6*16+7]+lum_lut[6*16+8]
l_cen = round(l_cen/4, 3)
Cam.log += '\nLuminance table centre: {}'.format(l_cen)
av_corn = np.sum(corners)/4
return cal_cr_list, cal_cb_list, lum_lut, av_corn
"""
calculate g/r and g/b for 32x32 points arranged in a grid for a single image
"""
def alsc(Cam, Img, do_alsc_colour, plot=False):
Cam.log += '\nProcessing image: ' + Img.name
"""
get channel in correct order
"""
channels = [Img.channels[i] for i in Img.order]
"""
calculate size of single rectangle.
-(-(w-1)//32) is a ceiling division. w-1 is to deal robustly with the case
where w is a multiple of 32.
"""
w, h = Img.w/2, Img.h/2
dx, dy = int(-(-(w-1)//16)), int(-(-(h-1)//12))
"""
average the green channels into one
"""
av_ch_g = np.mean((channels[1:3]), axis=0)
if do_alsc_colour:
"""
obtain 16x12 grid of intensities for each channel and subtract black level
"""
g = get_16x12_grid(av_ch_g, dx, dy) - Img.blacklevel_16
r = get_16x12_grid(channels[0], dx, dy) - Img.blacklevel_16
b = get_16x12_grid(channels[3], dx, dy) - Img.blacklevel_16
"""
calculate ratios as 32 bit in order to be supported by medianBlur function
"""
cr = np.reshape(g/r, (12, 16)).astype('float32')
cb = np.reshape(g/b, (12, 16)).astype('float32')
cg = np.reshape(1/g, (12, 16)).astype('float32')
"""
median blur to remove peaks and save as float 64
"""
cr = cv2.medianBlur(cr, 3).astype('float64')
cb = cv2.medianBlur(cb, 3).astype('float64')
cg = cv2.medianBlur(cg, 3).astype('float64')
cg = cg/np.min(cg)
"""
debugging code showing 2D surface plot of vignetting. Quite useful for
for sanity check
"""
if plot:
hf = plt.figure(figsize=(8, 8))
ha = hf.add_subplot(311, projection='3d')
"""
note Y is plotted as -Y so plot has same axes as image
"""
X, Y = np.meshgrid(range(16), range(12))
ha.plot_surface(X, -Y, cr, cmap=cm.coolwarm, linewidth=0)
ha.set_title('ALSC Plot\nImg: {}\n\ncr'.format(Img.str))
hb = hf.add_subplot(312, projection='3d')
hb.plot_surface(X, -Y, cb, cmap=cm.coolwarm, linewidth=0)
hb.set_title('cb')
hc = hf.add_subplot(313, projection='3d')
hc.plot_surface(X, -Y, cg, cmap=cm.coolwarm, linewidth=0)
hc.set_title('g')
# print(Img.str)
plt.show()
return Img.col, cr.flatten(), cb.flatten(), cg.flatten(), (w, h, dx, dy)
else:
"""
only perform calculations for luminance shading
"""
g = get_16x12_grid(av_ch_g, dx, dy) - Img.blacklevel_16
cg = np.reshape(1/g, (12, 16)).astype('float32')
cg = cv2.medianBlur(cg, 3).astype('float64')
cg = cg/np.min(cg)
if plot:
hf = plt.figure(figssize=(8, 8))
ha = hf.add_subplot(1, 1, 1, projection='3d')
X, Y = np.meashgrid(range(16), range(12))
ha.plot_surface(X, -Y, cg, cmap=cm.coolwarm, linewidth=0)
ha.set_title('ALSC Plot (Luminance only!)\nImg: {}\n\ncg').format(Img.str)
plt.show()
return Img.col, None, None, cg.flatten(), (w, h, dx, dy)
"""
Compresses channel down to a 16x12 grid
"""
def get_16x12_grid(chan, dx, dy):
grid = []
"""
since left and bottom border will not necessarily have rectangles of
dimension dx x dy, the 32nd iteration has to be handled separately.
"""
for i in range(11):
for j in range(15):
grid.append(np.mean(chan[dy*i:dy*(1+i), dx*j:dx*(1+j)]))
grid.append(np.mean(chan[dy*i:dy*(1+i), 15*dx:]))
for j in range(15):
grid.append(np.mean(chan[11*dy:, dx*j:dx*(1+j)]))
grid.append(np.mean(chan[11*dy:, 15*dx:]))
"""
return as np.array, ready for further manipulation
"""
return np.array(grid)
"""
obtains sigmas for red and blue, effectively a measure of the 'error'
"""
def get_sigma(Cam, cal_cr_list, cal_cb_list):
Cam.log += '\nCalculating sigmas'
"""
provided colour alsc tables were generated for two different colour
temperatures sigma is calculated by comparing two calibration temperatures
adjacent in colour space
"""
"""
create list of colour temperatures
"""
cts = [cal['ct'] for cal in cal_cr_list]
# print(cts)
"""
calculate sigmas for each adjacent cts and return worst one
"""
sigma_rs = []
sigma_bs = []
for i in range(len(cts)-1):
sigma_rs.append(calc_sigma(cal_cr_list[i]['table'], cal_cr_list[i+1]['table']))
sigma_bs.append(calc_sigma(cal_cb_list[i]['table'], cal_cb_list[i+1]['table']))
Cam.log += '\nColour temperature interval {} - {} K'.format(cts[i], cts[i+1])
Cam.log += '\nSigma red: {}'.format(sigma_rs[-1])
Cam.log += '\nSigma blue: {}'.format(sigma_bs[-1])
"""
return maximum sigmas, not necessarily from the same colour temperature
interval
"""
sigma_r = max(sigma_rs) if sigma_rs else 0.005
sigma_b = max(sigma_bs) if sigma_bs else 0.005
Cam.log += '\nMaximum sigmas: Red = {} Blue = {}'.format(sigma_r, sigma_b)
# print(sigma_rs, sigma_bs)
# print(sigma_r, sigma_b)
return sigma_r, sigma_b
"""
calculate sigma from two adjacent gain tables
"""
def calc_sigma(g1, g2):
"""
reshape into 16x12 matrix
"""
g1 = np.reshape(g1, (12, 16))
g2 = np.reshape(g2, (12, 16))
"""
apply gains to gain table
"""
gg = g1/g2
if np.mean(gg) < 1:
gg = 1/gg
"""
for each internal patch, compute average difference between it and its 4
neighbours, then append to list
"""
diffs = []
for i in range(10):
for j in range(14):
"""
note indexing is incremented by 1 since all patches on borders are
not counted
"""
diff = np.abs(gg[i+1][j+1]-gg[i][j+1])
diff += np.abs(gg[i+1][j+1]-gg[i+2][j+1])
diff += np.abs(gg[i+1][j+1]-gg[i+1][j])
diff += np.abs(gg[i+1][j+1]-gg[i+1][j+2])
diffs.append(diff/4)
"""
return mean difference
"""
mean_diff = np.mean(diffs)
return(np.round(mean_diff, 5))