Nevar pievienot vairāk kā 25 tēmas Tēmai ir jāsākas ar burtu vai ciparu, tā var saturēt domu zīmes ('-') un var būt līdz 35 simboliem gara.

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  1. /*
  2. * This file is part of Aptdec.
  3. * Copyright (c) 2004-2009 Thierry Leconte (F4DWV), Xerbo (xerbo@protonmail.com) 2019-2020
  4. *
  5. * Aptdec is free software: you can redistribute it and/or modify
  6. * it under the terms of the GNU General Public License as published by
  7. * the Free Software Foundation, either version 2 of the License, or
  8. * (at your option) any later version.
  9. *
  10. * This program is distributed in the hope that it will be useful,
  11. * but WITHOUT ANY WARRANTY; without even the implied warranty of
  12. * MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
  13. * GNU General Public License for more details.
  14. *
  15. * You should have received a copy of the GNU General Public License
  16. * along with this program. If not, see <https://www.gnu.org/licenses/>.
  17. *
  18. */
  19. #include <stdio.h>
  20. #include <string.h>
  21. #include <sndfile.h>
  22. #include <math.h>
  23. #include <stdlib.h>
  24. #include "offsets.h"
  25. #include "messages.h"
  26. #define REGORDER 3
  27. typedef struct {
  28. double cf[REGORDER + 1];
  29. } rgparam_t;
  30. typedef struct {
  31. float *prow[3000]; // Row buffers
  32. int nrow; // Number of rows
  33. int chA, chB; // ID of each channel
  34. char name[256]; // Stripped filename
  35. } image_t;
  36. typedef struct {
  37. char *type; // Output image type
  38. char *effects;
  39. int satnum; // The satellite number
  40. char *map; // Path to a map file
  41. char *path; // Output directory
  42. } options_t;
  43. extern void polyreg(const int m, const int n, const double x[], const double y[], double c[]);
  44. // Compute regression
  45. static void rgcomp(double x[16], rgparam_t * rgpr) {
  46. // { 0.106, 0.215, 0.324, 0.433, 0.542, 0.652, 0.78, 0.87, 0.0 }
  47. const double y[9] = { 31.07, 63.02, 94.96, 126.9, 158.86, 191.1, 228.62, 255.0, 0.0 };
  48. polyreg(REGORDER, 9, x, y, rgpr -> cf);
  49. }
  50. // Convert a value to 0-255 based off the provided regression curve
  51. static double rgcal(float x, rgparam_t *rgpr) {
  52. double y, p;
  53. int i;
  54. for (i = 0, y = 0.0, p = 1.0; i < REGORDER + 1; i++) {
  55. y += rgpr->cf[i] * p;
  56. p = p * x;
  57. }
  58. return(y);
  59. }
  60. static double tele[16];
  61. static double Cs;
  62. static int nbtele;
  63. void histogramEqualise(float **prow, int nrow, int offset, int width){
  64. // Plot histogram
  65. int histogram[256] = { 0 };
  66. for(int y = 0; y < nrow; y++)
  67. for(int x = 0; x < width; x++)
  68. histogram[(int)floor(prow[y][x+offset])]++;
  69. // Find min/max points
  70. int min = -1, max = -1;
  71. for(int i = 5; i < 250; i++){
  72. if(histogram[i]/width/(nrow/255.0) > 0.2){
  73. if(min == -1)
  74. min = i;
  75. max = i;
  76. }
  77. }
  78. //printf("Column %i-%i: Min: %i, Max %i\n", offset, offset+width, min, max);
  79. // Spread values to avoid overshoot
  80. min -= 5; max += 5;
  81. // Stretch the brightness into the new range
  82. for(int y = 0; y < nrow; y++)
  83. for(int x = 0; x < width; x++)
  84. prow[y][x+offset] = CLIP((prow[y][x+offset]-min) / (max-min) * 255.0, 0, 255);
  85. }
  86. // Brightness calibrate, including telemetry
  87. void calibrateBrightness(float **prow, int nrow, int offset, int width, int telestart, rgparam_t regr[30]){
  88. offset -= SYNC_WIDTH+SPC_WIDTH;
  89. for (int n = 0; n < nrow; n++) {
  90. float *pixelv = prow[n];
  91. for (int i = 0; i < width+SYNC_WIDTH+SPC_WIDTH+TELE_WIDTH; i++) {
  92. float pv = pixelv[i + offset];
  93. // Blend between the calculated regression curves
  94. /* FIXME: this can actually make the image look *worse*
  95. * if the signal has a constant input gain.
  96. */
  97. /*int k, kof;
  98. k = (n - telestart) / FRAME_LEN;
  99. if (k >= nbtele)
  100. k = nbtele - 1;
  101. kof = (n - telestart) % FRAME_LEN;
  102. if (kof < 64) {
  103. if (k < 1) {*/
  104. pv = rgcal(pv, &(regr[4]));
  105. /*} else {
  106. pv = rgcal(pv, &(regr[k])) * (64 + kof) / FRAME_LEN +
  107. rgcal(pv, &(regr[k - 1])) * (64 - kof) / FRAME_LEN;
  108. }
  109. } else {
  110. if ((k + 1) >= nbtele) {
  111. pv = rgcal(pv, &(regr[k]));
  112. } else {
  113. pv = rgcal(pv, &(regr[k])) * (192 - kof) / FRAME_LEN +
  114. rgcal(pv, &(regr[k + 1])) * (kof - 64) / FRAME_LEN;
  115. }
  116. }
  117. */
  118. pv = CLIP(pv, 0, 255);
  119. pixelv[i + offset] = pv;
  120. }
  121. }
  122. }
  123. // Get telemetry data for thermal calibration/equalization
  124. int calibrate(float **prow, int nrow, int offset, int width) {
  125. double teleline[3000] = { 0.0 };
  126. double wedge[16];
  127. rgparam_t regr[30];
  128. int n, k;
  129. int mtelestart = 0, telestart;
  130. int channel = -1;
  131. // Calculate average of a row of telemetry
  132. for (n = 0; n < nrow; n++) {
  133. float *pixelv = prow[n];
  134. // Average the center 40px
  135. for (int i = 3; i < 43; i++) teleline[n] += pixelv[i + offset + width];
  136. teleline[n] /= 40.0;
  137. }
  138. // The minimum rows required to decode a full frame
  139. if (nrow < 192) {
  140. fprintf(stderr, ERR_TELE_ROW);
  141. return(0);
  142. }
  143. /* Wedge 7 is white and 8 is black, which will have the largest
  144. * difference in brightness, this will always be in the center of
  145. * the frame and can thus be used to find the start of the frame
  146. */
  147. double max = 0.0;
  148. for (n = nrow / 3 - 64; n < 2 * nrow / 3 - 64; n++) {
  149. float df;
  150. // (sum 4px below) / (sum 4px above)
  151. df = (teleline[n - 4] + teleline[n - 3] + teleline[n - 2] + teleline[n - 1]) /
  152. (teleline[n + 0] + teleline[n + 1] + teleline[n + 2] + teleline[n + 3]);
  153. // Find the maximum difference
  154. if (df > max) {
  155. mtelestart = n;
  156. max = df;
  157. }
  158. }
  159. // Find the start of the first frame
  160. telestart = (mtelestart - FRAME_LEN/2) % FRAME_LEN;
  161. // Make sure that theres at least one full frame in the image
  162. if (nrow < telestart + FRAME_LEN) {
  163. fprintf(stderr, ERR_TELE_ROW);
  164. return(0);
  165. }
  166. // For each frame
  167. for (n = telestart, k = 0; n < nrow - FRAME_LEN; n += FRAME_LEN, k++) {
  168. float *pixelv = prow[n];
  169. int j;
  170. // Turn each wedge into a value
  171. for (j = 0; j < 16; j++) {
  172. // Average the middle 6px
  173. wedge[j] = 0.0;
  174. for (int i = 1; i < 7; i++) wedge[j] += teleline[(j * 8) + n + i];
  175. wedge[j] /= 6;
  176. }
  177. // Compute regression on the wedges
  178. rgcomp(wedge, &(regr[k]));
  179. // Read the telemetry values from the middle of the image
  180. if (k == nrow / (2*FRAME_LEN)) {
  181. int l;
  182. // Equalise
  183. for (j = 0; j < 16; j++) tele[j] = rgcal(wedge[j], &(regr[k]));
  184. /* Compare the channel ID wedge to the reference
  185. * wedges, the wedge with the closest match will
  186. * be the channel ID
  187. */
  188. float min = -1;
  189. for (j = 0; j < 6; j++) {
  190. float df;
  191. df = tele[15] - tele[j];
  192. df *= df;
  193. if (df < min || min == -1) {
  194. channel = j;
  195. min = df;
  196. }
  197. }
  198. // Cs computation, still have no idea what this does
  199. int i;
  200. for (Cs = 0.0, i = 0, j = n; j < n + FRAME_LEN; j++) {
  201. double csline;
  202. for (csline = 0.0, l = 3; l < 43; l++)
  203. csline += pixelv[l + offset - SPC_WIDTH];
  204. csline /= 40.0;
  205. if (csline > 50.0) {
  206. Cs += csline;
  207. i++;
  208. }
  209. }
  210. Cs /= i;
  211. Cs = rgcal(Cs, &(regr[k]));
  212. }
  213. }
  214. nbtele = k;
  215. calibrateBrightness(prow, nrow, offset, width, telestart, regr);
  216. return(channel + 1);
  217. }
  218. // --- Temperature Calibration --- //
  219. #include "satcal.h"
  220. typedef struct {
  221. double Nbb;
  222. double Cs;
  223. double Cb;
  224. int ch;
  225. } tempparam_t;
  226. // IR channel temperature compensation
  227. static void tempcomp(double t[16], int ch, int satnum, tempparam_t *tpr) {
  228. double Tbb, T[4];
  229. double C;
  230. tpr -> ch = ch - 4;
  231. // Compute equivalent T blackbody temperature
  232. for (int n = 0; n < 4; n++) {
  233. float d0, d1, d2;
  234. C = t[9 + n] * 4.0;
  235. d0 = satcal[satnum].d[n][0];
  236. d1 = satcal[satnum].d[n][1];
  237. d2 = satcal[satnum].d[n][2];
  238. T[n] = d0;
  239. T[n] += d1 * C;
  240. C = C * C;
  241. T[n] += d2 * C;
  242. }
  243. Tbb = (T[0] + T[1] + T[2] + T[3]) / 4.0;
  244. Tbb = satcal[satnum].rad[tpr->ch].A + satcal[satnum].rad[tpr->ch].B * Tbb;
  245. // Compute radiance blackbody
  246. C = satcal[satnum].rad[tpr->ch].vc;
  247. tpr->Nbb = c1 * C * C * C / (expm1(c2 * C / Tbb));
  248. // Store count blackbody and space
  249. tpr->Cs = Cs * 4.0;
  250. tpr->Cb = t[14] * 4.0;
  251. }
  252. // IR channel temperature calibration
  253. static double tempcal(float Ce, int satnum, tempparam_t * rgpr) {
  254. double Nl, Nc, Ns, Ne;
  255. double T, vc;
  256. Ns = satcal[satnum].cor[rgpr->ch].Ns;
  257. Nl = Ns + (rgpr->Nbb - Ns) * (rgpr->Cs - Ce * 4.0) / (rgpr->Cs - rgpr->Cb);
  258. Nc = satcal[satnum].cor[rgpr->ch].b[0] +
  259. satcal[satnum].cor[rgpr->ch].b[1] * Nl +
  260. satcal[satnum].cor[rgpr->ch].b[2] * Nl * Nl;
  261. Ne = Nl + Nc;
  262. vc = satcal[satnum].rad[rgpr->ch].vc;
  263. T = c2 * vc / log1p(c1 * vc * vc * vc / Ne);
  264. T = (T - satcal[satnum].rad[rgpr->ch].A) / satcal[satnum].rad[rgpr->ch].B;
  265. // Rescale to 0-255 for -60'C to +40'C
  266. T = (T - 273.15 + 60.0) / 100.0 * 256.0;
  267. return(T);
  268. }
  269. // Temperature calibration wrapper
  270. void temperature(options_t *opts, image_t *img, int offset, int width){
  271. tempparam_t temp;
  272. printf("Temperature... ");
  273. fflush(stdout);
  274. tempcomp(tele, img->chB, opts->satnum - 15, &temp);
  275. for (int y = 0; y < img->nrow; y++) {
  276. float *pixelv = img->prow[y];
  277. for (int x = 0; x < width; x++) {
  278. float pv = tempcal(pixelv[x + offset], opts->satnum - 15, &temp);
  279. pixelv[x + offset] = CLIP(pv, 0, 255);
  280. }
  281. }
  282. printf("Done\n");
  283. }
  284. void distrib(options_t *opts, image_t *img, char *chid) {
  285. int max = 0;
  286. // Options
  287. options_t options;
  288. options.path = opts->path;
  289. // Image options
  290. image_t distrib;
  291. strcpy(distrib.name, img->name);
  292. distrib.nrow = 256;
  293. // Assign memory
  294. for(int i = 0; i < 256; i++)
  295. distrib.prow[i] = (float *) malloc(sizeof(float) * 256);
  296. for(int n = 0; n < img->nrow; n++) {
  297. float *pixelv = img->prow[n];
  298. for(int i = 0; i < CH_WIDTH; i++) {
  299. int y = CLIP((int)pixelv[i + CHA_OFFSET], 0, 255);
  300. int x = CLIP((int)pixelv[i + CHB_OFFSET], 0, 255);
  301. distrib.prow[y][x]++;
  302. if(distrib.prow[y][x] > max)
  303. max = distrib.prow[y][x];
  304. }
  305. }
  306. // Scale to 0-255
  307. for(int x = 0; x < 256; x++)
  308. for(int y = 0; y < 256; y++)
  309. distrib.prow[y][x] = distrib.prow[y][x] / max * 255.0;
  310. extern int ImageOut(options_t *opts, image_t *img, int offset, int width, char *desc, char *chid, char *palette);
  311. ImageOut(&options, &distrib, 0, 256, "Distribution", chid, NULL);
  312. }
  313. extern float quick_select(float arr[], int n);
  314. // Recursive biased median denoise
  315. #define TRIG_LEVEL 40
  316. void denoise(float **prow, int nrow, int offset, int width){
  317. for(int y = 2; y < nrow-2; y++){
  318. for(int x = offset+1; x < offset+width-1; x++){
  319. if(prow[y][x+1] - prow[y][x] > TRIG_LEVEL ||
  320. prow[y][x-1] - prow[y][x] > TRIG_LEVEL ||
  321. prow[y+1][x] - prow[y][x] > TRIG_LEVEL ||
  322. prow[y-1][x] - prow[y][x] > TRIG_LEVEL){
  323. prow[y][x] = quick_select((float[]){
  324. prow[y+2][x-1], prow[y+2][x], prow[y+2][x+1],
  325. prow[y+1][x-1], prow[y+1][x], prow[y+1][x+1],
  326. prow[y-1][x-1], prow[y-1][x], prow[y-1][x+1],
  327. prow[y-2][x-1], prow[y-2][x], prow[y-2][x+1]
  328. }, 12);
  329. }
  330. }
  331. }
  332. }
  333. #undef TRIG_LEVEL