- /*
- * This file is part of Aptdec.
- * Copyright (c) 2004-2009 Thierry Leconte (F4DWV), Xerbo (xerbo@protonmail.com) 2019-2020
- *
- * Aptdec is free software: you can redistribute it and/or modify
- * it under the terms of the GNU General Public License as published by
- * the Free Software Foundation, either version 2 of the License, or
- * (at your option) any later version.
- *
- * This program is distributed in the hope that it will be useful,
- * but WITHOUT ANY WARRANTY; without even the implied warranty of
- * MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
- * GNU General Public License for more details.
- *
- * You should have received a copy of the GNU General Public License
- * along with this program. If not, see <https://www.gnu.org/licenses/>.
- *
- */
-
- #include <stdio.h>
- #include <string.h>
- #include <math.h>
- #include <stdlib.h>
-
- #include "apt.h"
- #include "offsets.h"
- #include "libs/reg.h"
- #include "image.h"
-
- #define REGORDER 3
- typedef struct {
- double cf[REGORDER + 1];
- } rgparam_t;
-
- // Compute regression
- static void rgcomp(double x[16], rgparam_t * rgpr) {
- // { 0.106, 0.215, 0.324, 0.433, 0.542, 0.652, 0.78, 0.87, 0.0 }
- const double y[9] = { 31.07, 63.02, 94.96, 126.9, 158.86, 191.1, 228.62, 255.0, 0.0 };
-
- polyreg(REGORDER, 9, x, y, rgpr->cf);
- }
-
- // Convert a value to 0-255 based off the provided regression curve
- static double rgcal(float x, rgparam_t *rgpr) {
- double y, p;
- int i;
-
- for (i = 0, y = 0.0, p = 1.0; i < REGORDER + 1; i++) {
- y += rgpr->cf[i] * p;
- p = p * x;
- }
- return y;
- }
-
- static double tele[16];
- static double Cs;
-
- void apt_histogramEqualise(float **prow, int nrow, int offset, int width){
- // Plot histogram
- int histogram[256] = { 0 };
- for(int y = 0; y < nrow; y++)
- for(int x = 0; x < width; x++)
- histogram[(int)CLIP(prow[y][x+offset], 0, 255)]++;
-
- // Calculate cumulative frequency
- long sum = 0, cf[256] = { 0 };
- for(int i = 0; i < 255; i++){
- sum += histogram[i];
- cf[i] = sum;
- }
-
- // Apply histogram
- int area = nrow * width;
- for(int y = 0; y < nrow; y++){
- for(int x = 0; x < width; x++){
- int k = (int)prow[y][x+offset];
- prow[y][x+offset] = (256.0f/area) * cf[k];
- }
- }
- }
-
- void apt_linearEnhance(float **prow, int nrow, int offset, int width){
- // Plot histogram
- int histogram[256] = { 0 };
- for(int y = 0; y < nrow; y++)
- for(int x = 0; x < width; x++)
- histogram[(int)CLIP(prow[y][x+offset], 0, 255)]++;
-
- // Find min/max points
- int min = -1, max = -1;
- for(int i = 5; i < 250; i++){
- if(histogram[i]/width/(nrow/255.0) > 0.1){
- if(min == -1) min = i;
- max = i;
- }
- }
-
- // Stretch the brightness into the new range
- for(int y = 0; y < nrow; y++){
- for(int x = 0; x < width; x++){
- prow[y][x+offset] = (prow[y][x+offset]-min) / (max-min) * 255.0f;
- prow[y][x+offset] = CLIP(prow[y][x+offset], 0.0f, 255.0f);
- }
- }
- }
-
- // Brightness calibrate, including telemetry
- void calibrateImage(float **prow, int nrow, int offset, int width, rgparam_t regr){
- offset -= SYNC_WIDTH+SPC_WIDTH;
-
- for (int y = 0; y < nrow; y++) {
- for (int x = 0; x < width+SYNC_WIDTH+SPC_WIDTH+TELE_WIDTH; x++) {
- float pv = (float)rgcal(prow[y][x + offset], ®r);
- prow[y][x + offset] = CLIP(pv, 0, 255);
- }
- }
- }
-
- double teleNoise(double wedges[16]){
- double pattern[9] = { 31.07, 63.02, 94.96, 126.9, 158.86, 191.1, 228.62, 255.0, 0.0 };
- double noise = 0;
- for(int i = 0; i < 9; i++)
- noise += fabs(wedges[i] - pattern[i]);
-
- return noise;
- }
-
- // Get telemetry data for thermal calibration
- int apt_calibrate(float **prow, int nrow, int offset, int width) {
- double teleline[APT_MAX_HEIGHT] = { 0.0 };
- double wedge[16];
- rgparam_t regr[APT_MAX_HEIGHT/FRAME_LEN + 1];
- int telestart, mtelestart = 0;
- int channel = -1;
-
- // The minimum rows required to decode a full frame
- if (nrow < 192) {
- fprintf(stderr, "Telemetry decoding error, not enough rows\n");
- return 0;
- }
-
- // Calculate average of a row of telemetry
- for (int y = 0; y < nrow; y++) {
- for (int x = 3; x < 43; x++)
- teleline[y] += prow[y][x + offset + width];
-
- teleline[y] /= 40.0;
- }
-
- /* Wedge 7 is white and 8 is black, this will have the largest
- * difference in brightness, this can be used to find the current
- * position within the telemetry.
- */
- float max = 0.0f;
- for (int n = nrow / 3 - 64; n < 2 * nrow / 3 - 64; n++) {
- float df;
-
- // (sum 4px below) - (sum 4px above)
- df = (float)((teleline[n - 4] + teleline[n - 3] + teleline[n - 2] + teleline[n - 1]) -
- (teleline[n + 0] + teleline[n + 1] + teleline[n + 2] + teleline[n + 3]));
-
- // Find the maximum difference
- if (df > max) {
- mtelestart = n;
- max = df;
- }
- }
-
- telestart = (mtelestart + 64) % FRAME_LEN;
-
- // Make sure that theres at least one full frame in the image
- if (nrow < telestart + FRAME_LEN) {
- fprintf(stderr, "Telemetry decoding error, not enough rows\n");
- return 0;
- }
-
- // Find the least noisy frame
- double minNoise = -1;
- int bestFrame = -1;
- for (int n = telestart, k = 0; n < nrow - FRAME_LEN; n += FRAME_LEN, k++) {
- int j;
-
- for (j = 0; j < 16; j++) {
- int i;
-
- wedge[j] = 0.0;
- for (i = 1; i < 7; i++)
- wedge[j] += teleline[n + j * 8 + i];
- wedge[j] /= 6;
- }
-
- double noise = teleNoise(wedge);
- if(noise < minNoise || minNoise == -1){
- minNoise = noise;
- bestFrame = k;
-
- // Compute & apply regression on the wedges
- rgcomp(wedge, ®r[k]);
- for (int j = 0; j < 16; j++)
- tele[j] = (float)rgcal((float)wedge[j], ®r[k]);
-
- /* Compare the channel ID wedge to the reference
- * wedges, the wedge with the closest match will
- * be the channel ID
- */
- float min = -1;
- for (int j = 0; j < 6; j++) {
- float df = (float)(tele[15] - tele[j]);
- df *= df;
-
- if (df < min || min == -1) {
- channel = j;
- min = df;
- }
- }
-
- // Find the brightness of the minute marker, I don't really know what for
- Cs = 0.0;
- int i, j = n;
- for (i = 0, j = n; j < n + FRAME_LEN; j++) {
- float csline = 0.0;
- for (int l = 3; l < 43; l++)
- csline += prow[n][l + offset - SPC_WIDTH];
- csline /= 40.0;
-
- if (csline > 50.0) {
- Cs += csline;
- i++;
- }
- }
- Cs = rgcal((float)(Cs / i), ®r[k]);
- }
- }
-
- if(bestFrame == -1){
- fprintf(stderr, "Something has gone very wrong, please file a bug report.\n");
- return 0;
- }
-
- calibrateImage(prow, nrow, offset, width, regr[bestFrame]);
-
- return channel + 1;
-
- }
-
- extern float quick_select(float arr[], int n);
-
- // Biased median denoise, pretyt ugly
- #define TRIG_LEVEL 40
- void apt_denoise(float **prow, int nrow, int offset, int width){
- for(int y = 2; y < nrow-2; y++){
- for(int x = offset+1; x < offset+width-1; x++){
- if(prow[y][x+1] - prow[y][x] > TRIG_LEVEL ||
- prow[y][x-1] - prow[y][x] > TRIG_LEVEL ||
- prow[y+1][x] - prow[y][x] > TRIG_LEVEL ||
- prow[y-1][x] - prow[y][x] > TRIG_LEVEL){
- prow[y][x] = quick_select((float[]){
- prow[y+2][x-1], prow[y+2][x], prow[y+2][x+1],
- prow[y+1][x-1], prow[y+1][x], prow[y+1][x+1],
- prow[y-1][x-1], prow[y-1][x], prow[y-1][x+1],
- prow[y-2][x-1], prow[y-2][x], prow[y-2][x+1]
- }, 12);
- }
- }
- }
- }
- #undef TRIG_LEVEL
-
- // Flips a channel, for northbound passes
- void apt_flipImage(apt_image_t *img, int width, int offset){
- for(int y = 1; y < img->nrow; y++){
- for(int x = 1; x < ceil(width / 2.0); x++){
- // Flip top-left & bottom-right
- float buffer = img->prow[img->nrow - y][offset + x];
- img->prow[img->nrow - y][offset + x] = img->prow[y][offset + (width - x)];
- img->prow[y][offset + (width - x)] = buffer;
- }
- }
- }
-
- // Calculate crop to reomve noise from the start and end of an image
- int apt_cropNoise(apt_image_t *img){
- #define NOISE_THRESH 180.0
-
- // Average value of minute marker
- float spc_rows[APT_MAX_HEIGHT] = { 0.0 };
- int startCrop = 0; int endCrop = img->nrow;
- for(int y = 0; y < img->nrow; y++) {
- for(int x = 0; x < SPC_WIDTH; x++) {
- spc_rows[y] += img->prow[y][x + (CHB_OFFSET - SPC_WIDTH)];
- }
- spc_rows[y] /= SPC_WIDTH;
-
- // Skip minute markings
- if(spc_rows[y] < 10) {
- spc_rows[y] = spc_rows[y-1];
- }
- }
-
- // 3 row average
- for(int y = 0; y < img->nrow; y++){
- spc_rows[y] = (spc_rows[y+1] + spc_rows[y+2] + spc_rows[y+3])/3;
- //img.prow[y][0] = spc_rows[y];
- }
-
- // Find ends
- for(int y = 0; y < img->nrow-1; y++) {
- if(spc_rows[y] > NOISE_THRESH){
- endCrop = y;
- }
- }
- for(int y = img->nrow; y > 0; y--) {
- if(spc_rows[y] > NOISE_THRESH) {
- startCrop = y;
- }
- }
-
- //printf("Crop rows: %i -> %i\n", startCrop, endCrop);
-
- // Remove the noisy rows at start
- for(int y = 0; y < img->nrow-startCrop; y++) {
- memmove(img->prow[y], img->prow[y+startCrop], sizeof(float)*2150);
- }
-
- // Ignore the noisy rows at the end
- img->nrow = (endCrop - startCrop);
-
- return startCrop;
- }
-
- // --- Temperature Calibration --- //
- #include "satcal.h"
-
- typedef struct {
- double Nbb;
- double Cs;
- double Cb;
- int ch;
- } tempparam_t;
-
- // IR channel temperature compensation
- static void tempcomp(double t[16], int ch, int satnum, tempparam_t *tpr) {
- double Tbb, T[4];
- double C;
-
- tpr->ch = ch - 4;
-
- // Compute equivalent T blackbody temperature
- for (int n = 0; n < 4; n++) {
- float d0, d1, d2;
-
- C = t[9 + n] * 4.0;
- d0 = satcal[satnum].d[n][0];
- d1 = satcal[satnum].d[n][1];
- d2 = satcal[satnum].d[n][2];
- T[n] = d0;
- T[n] += d1 * C;
- C *= C;
- T[n] += d2 * C;
- }
- Tbb = (T[0] + T[1] + T[2] + T[3]) / 4.0;
- Tbb = satcal[satnum].rad[tpr->ch].A + satcal[satnum].rad[tpr->ch].B * Tbb;
-
- // Compute blackbody radiance temperature
- C = satcal[satnum].rad[tpr->ch].vc;
- tpr->Nbb = c1 * C * C * C / (expm1(c2 * C / Tbb));
-
- // Store blackbody count and space
- tpr->Cs = Cs * 4.0;
- tpr->Cb = t[14] * 4.0;
- }
-
- // IR channel temperature calibration
- static double tempcal(float Ce, int satnum, tempparam_t * rgpr) {
- double Nl, Nc, Ns, Ne;
- double T, vc;
-
- Ns = satcal[satnum].cor[rgpr->ch].Ns;
- Nl = Ns + (rgpr->Nbb - Ns) * (rgpr->Cs - Ce * 4.0) / (rgpr->Cs - rgpr->Cb);
- Nc = satcal[satnum].cor[rgpr->ch].b[0] +
- satcal[satnum].cor[rgpr->ch].b[1] * Nl +
- satcal[satnum].cor[rgpr->ch].b[2] * Nl * Nl;
-
- Ne = Nl + Nc;
-
- vc = satcal[satnum].rad[rgpr->ch].vc;
- T = c2 * vc / log(c1 * vc * vc * vc / Ne + 1.0);
- T = (T - satcal[satnum].rad[rgpr->ch].A) / satcal[satnum].rad[rgpr->ch].B;
-
- // Convert to celsius
- T -= 273.15;
- // Rescale to 0-255 for -120°C to +40°C
- T = (T + 100.0) / 160.0 * 255.0;
-
- return T;
- }
-
- // Temperature calibration wrapper
- void temperature(options_t *opts, apt_image_t *img, int offset, int width){
- tempparam_t temp;
-
- printf("Temperature... ");
- fflush(stdout);
-
- tempcomp(tele, img->chB, opts->satnum - 15, &temp);
-
- for (int y = 0; y < img->nrow; y++) {
- for (int x = 0; x < width; x++) {
- img->prow[y][x + offset] = (float)tempcal(img->prow[y][x + offset], opts->satnum - 15, &temp);
- }
- }
- printf("Done\n");
- }
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