Changeset 316
- Timestamp:
- 11/10/99 07:42:41 (25 years ago)
- File:
-
- 1 edited
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trunk/MagicSoft/Simulation/Detector/Camera/camera.h
r308 r316 19 19 //= 20 20 //= $RCSfile: camera.h,v $ 21 //= $Revision: 1. 1.1.1$21 //= $Revision: 1.2 $ 22 22 //= $Author: harald $ 23 //= $Date: 1999-11- 05 11:59:31 $23 //= $Date: 1999-11-10 07:42:41 $ 24 24 //= 25 25 //=////////////////////////////////////////////////////////////////////// … … 236 236 //!@{ 237 237 238 #define QE_FILE " qe.dat"238 #define QE_FILE "../Data/qe.dat" 239 239 240 240 //!@} … … 278 278 /* 279 279 *$Log: not supported by cvs2svn $ 280 *Revision 1.1.1.1 1999/11/05 11:59:31 harald 281 *This the starting point for CVS controlled further developments of the 282 *camera program. The program was originally written by Jose Carlos. 283 *But here you can find a "rootified" version to the program. This means 284 *that there is no hbook stuff in it now. Also the output of the 285 *program changed to the MagicRawDataFormat. 286 * 287 *The "rootification" was done by Dirk Petry and Harald Kornmayer. 288 * 289 *In the following you can see the README file of that version: 290 * 291 *================================================== 292 * 293 *Fri Oct 22 1999 D.P. 294 * 295 *The MAGIC Monte Carlo System 296 * 297 *Camera Simulation Programme 298 *--------------------------- 299 * 300 *1) Description 301 * 302 *This version is the result of the fusion of H.K.'s 303 *root_camera which is described below (section 2) 304 *and another version by D.P. which had a few additional 305 *useful features. 306 * 307 *The version compiles under Linux with ROOT 2.22 installed 308 *(variable ROOTSYS has to be set). 309 * 310 *Compile as before simply using "make" in the root_camera 311 *directory. 312 * 313 *All features of H.K.'s root_camera were retained. 314 * 315 *Additional features of this version are: 316 * 317 * a) HBOOK is no longer used and all references are removed. 318 * 319 * b) Instead of HBOOK, the user is given now the possibility of 320 * having Diagnostic data in ROOT format as a complement 321 * to the ROOT Raw data. 322 * 323 * This data is written to the file which is determined by 324 * the new input parameter "diag_file" in the camera parameter 325 * file. 326 * 327 * All source code file belonging to this part have filenames 328 * starting with "MDiag". 329 * 330 * The user can read the output file using the following commands 331 * in an interactive ROOT session: 332 * 333 * root [0] .L MDiag.so 334 * root [1] new TFile("diag.root"); 335 * root [2] new TTreeViewer("T"); 336 * 337 * This brings up a viewer from which all variables of the 338 * TTree can be accessed and histogrammed. This example 339 * assumes that you have named the file "diag.root", that 340 * you are using ROOT version 2.22 or later and that you have 341 * the shared object library "MDiag.so" which is produced 342 * by the Makefile along with the executable "camera". 343 * 344 * ! The contents of the so-called diag file is not yet fixed. 345 * ! At the moment it is what J.C.G. used to put into the HBOOK 346 * ! ntuple. In future versions the moments calculation can be 347 * ! removed and the parameter list be modified correspondingly. 348 * 349 * c) Now concatenated reflector files can be read. This is useful 350 * if you have run the reflector with different parameters but 351 * you want to continue the analysis with all reflector data 352 * going into ONE ROOT outputfile. 353 * 354 * The previous camera version contained a bug which made reading 355 * of two or more concatenated reflector files impossible. 356 * 357 * d) The reflector output format was changed. It is now version 358 * 0.4 . 359 * The change solely consists in a shortening of the flag 360 * definition in the file 361 * 362 * include-MC/MCCphoton.hxx 363 * 364 * ! IF YOU WANT TO READ REFLECTOR FORMAT 0.3, you can easily 365 * ! do so by recompiling camera with the previous version of 366 * ! include-MC/MCCphoton.hxx. 367 * 368 * The change was necessary for saving space and better 369 * debugging. From now on, this format can be frozen. 370 * 371 * ! For producing reflector output in the new format, you 372 * ! of course have to recompile your reflector with the 373 * ! new include-MC/MCCphoton.hxx . 374 * 375 * e) A first version of the pixelization with the larger 376 * outer pixels is implemented. THIS IS NOT YET FULLY 377 * TESTED, but first rough tests show that it works 378 * at least to a good approximation. 379 * 380 * The present version implements the camera outline 381 * with 18 "gap-pixels" and 595 pixels in total as 382 * shown in 383 * 384 * http://sarastro.ifae.es/internal/home/hardware/camera/numbering.ps 385 * 386 * This change involved 387 * 388 * (i) The file pixels.dat is no longer needed. Instead 389 * the coordinates are generated by the program itself 390 * (takes maybe 1 second). In the file 391 * 392 * pixel-coords.txt 393 * 394 * in the same directory as this README, you find a list 395 * of the coordinates generated by this new routine. It 396 * has the format 397 * 398 * number i j x y size-factor 399 * 400 * where i and j are J.C.G.'s so called biaxis hexagonal 401 * coordinates (for internal use) and x and y are the 402 * coordinates of the pixel centers in the standard camera 403 * coordinate system in units of centimeters. The value 404 * of "size-factor" determines the linear size of the pixel 405 * relative to the central pixels. 406 * 407 * (ii) The magic.def file has two additional parameters 408 * which give the number of central pixels and the 409 * number of gap pixels 410 * 411 * (iii) In camera.h and camera.cxx several changes were 412 * necessary, among them the introduction of several 413 * new functions 414 * 415 * The newly suggested outline with asymmetric Winston cones 416 * will be implemented in a later version. 417 * 418 * f) phe files can no longer be read since this contradicts 419 * our philosophy that the analysis should be done with other 420 * programs like e.g. EVITA and not with "camera" itself. 421 * This possibility was removed. 422 * 423 * g) ROOT is no longer invoked with an interactive interface. 424 * In this way, camera can better be run as a batch program and 425 * it uses less memory. 426 * 427 * h) small changes concerning the variable "t_chan" were necessary in 428 * order to avoid segmentation faults: The variable is used as an 429 * index and it went sometimes outside the limits when camera 430 * was reading proton data. This is because the reflector files 431 * don't contain the photons in a chronological order and also 432 * the timespread can be considerably longer that the foreseen 433 * digitisation timespan. Please see the source code of camera.cxx 434 * round about line 1090. 435 * 436 * j) several unused variables were removed, a few warning messages 437 * occur when you compile camera.cxx but these can be ignored at 438 * the moment. 439 * 440 *In general the program is of course not finished. It still needs 441 *debugging, proper trigger simulation, simulation of the asymmetric 442 *version of the outer pixels, proper NSB simulation, adaption of 443 *the diag "ntuple" contents to our need and others small improvements. 444 * 445 *In the directory rfl-files there is now a file in reflector format 0.4 446 *containing a single event produced by the starfiled adder. It has 447 *a duration of 30 ns and represents the region around the Crab Nebula. 448 *Using the enclosed input parameter file, camera should process this 449 *file without problems. 450 * 451 *2) The README for the previous version of root_camera 452 * 453 *README for a preliminary version of the 454 *root_camera program. 455 * 456 *root_camera is based on the program "camera"of Jose Carlos 457 *Gonzalez. It was changed in the way that only the pixelisation 458 *and the distibution of the phe to the FADCs works in a 459 *first version. 460 * 461 *Using the #undef command most possibilities of the orignal 462 *program are switched of. 463 * 464 *The new parts are signed by 465 * 466 *- ROOT or __ROOT__ 467 * nearly all important codelines for ROOT output are enclosed 468 * in structures like 469 * #ifdef __ROOT__ 470 * 471 * code 472 * 473 * #endif __ROOT__ 474 * 475 * In same case the new lines are signed by a comment with the word 476 * ROOT in it. 477 * 478 * For timing of the pulse some variable names are changed. 479 * (t0, t1, t --> t_ini, t_fin, t_1st, t_chan,...) 480 * Look also for this changes. 481 * 482 * For the new root-file is also a change in readparm-files 483 * 484 * 485 *- __DETAIL_TRIGGER__ 486 * 487 * This is for the implementation of the current work on trigger 488 * studies. Because the class MTrigger is not well documented it 489 * isn´t a part of this tar file. Only a dummy File exists. 490 * 491 * 492 * 493 *With all files in the archive, the root_camera program should run. 494 * 495 *A reflector file is in the directory rfl-files 496 * 497 *================================================== 498 * 499 *From now on, use CVS for development!!!! 500 * 501 * 502 * 280 503 *Revision 1.3 1999/10/22 15:32:56 petry 281 504 *tidied-up version, really sent to H.K. and N.M., 22-10-99
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