Index: trunk/MagicSoft/Simulation/Detector/ReflectorII/config.mk.linux =================================================================== --- trunk/MagicSoft/Simulation/Detector/ReflectorII/config.mk.linux (revision 1432) +++ trunk/MagicSoft/Simulation/Detector/ReflectorII/config.mk.linux (revision 1432) @@ -0,0 +1,61 @@ +################################################################## +# +# config.mk +# +# @file config.mk +# @title small configuration file for Makefile +# @author J C Gonz\'alez +# @email gonzalez@mppmu.mpg.de +# @date Fri Mar 12 11:51:11 MET 1999 +# +#_______________________________________________________________ +# +# Created: Fri Mar 12 11:51:11 MET 1999 +# Author: Jose Carlos Gonzalez +# Purpose: Makefile for the compilation of the reflector program +# Notes: +# +#--------------------------------------------------------------- +# $RCSfile: config.mk.linux,v $ +# $Revision: 1.1 $ +# $Author: bigongia $ +# $Date: 2002-07-24 14:43:34 $ +################################################################## +# @maintitle + +# @code + +# program + +PROGRAM = camera + +# compilers & tools + +CC = gcc +CXX = g++ +F77 = g77 + +DOCUM = ../sus/sus +RATE = ../../comstat/comstat -g -p + +# includes + +INCLUDE = ../include-GENERAL +INCLUDE_COR = ../include-CORSIKA +INCLUDE_MC = ../include-MC +INCLUDE_REFL = . + +OPTIM = +DEBUG = -g + +# libraries + +RANLIBDIR = ../lib +CERNDIR = /CERN + +# system + +SYSTEM = linux + +# @endcode +##EOF Index: trunk/MagicSoft/Simulation/Detector/ReflectorII/doc/Tdas0205.tex =================================================================== --- trunk/MagicSoft/Simulation/Detector/ReflectorII/doc/Tdas0205.tex (revision 1432) +++ trunk/MagicSoft/Simulation/Detector/ReflectorII/doc/Tdas0205.tex (revision 1432) @@ -0,0 +1,627 @@ +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +%%% magic-tdas.tex -- template to write MAGIC-TDAS documents +%%%----------------------------------------------------------------- +%%% Kopyleft (K) 2000 J C Gonzalez +%%% Max-Planck-Institut fuer Physik, +%%% Foehringer Ring 6, 80805 Muenchen, Germany +%%% E-mail: gonzalez@mppmu.mpg.de +%%%----------------------------------------------------------------- +%%% This program is free software; you can redistribute, copy, +%%% modify, use it and its documentation for any purpose, +%%% provided that the above copyright notice appear in all +%%% copies and that both that copyright notice and this +%%% permission notice appear in supporting documentation. +%%% +%%% This piece of code is distributed in the hope that it will +%%% be useful, but WITHOUT ANY WARRANTY; without even the +%%% implied warranty of FITNESS FOR A PARTICULAR PURPOSE. +%%% +%%% Although you can actually do whatever you want with this +%%% file (following the copyright notice above), your are +%%% strongly encouraged NOT to edit directly this file. +%%% Instead, make a copy and edit the copy for your purposes. +%%% +%%% Modifying thie original file means that you actually have +%%% the (very basic) knowledge needed to make things by your +%%% own, and therefore... you will not get _any_ additional +%%% support :-) +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +%%% Last update: Time-stamp: +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +% +\documentclass[12pt]{article} + +\usepackage{magic-tdas} + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +%% BEGIN DOCUMENT +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +\begin{document} + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +%% Please, for the formatting just include here the standard +%% elements: title, author, date, plus TDAScode +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +\title{ The Reflector simulation program v.0.5 } +\author{A.Moralejo\\ + \texttt{}} +\date{June 04, 2002\\} +\TDAScode{MAGIC-TDAS 02-05\\ 020604/AMoralejo} +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% + +%% title %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +\maketitle + +%% abstract %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +\begin{abstract} +In this document we provide a brief description of Reflector program +(version 0.5) and a guide to install and run it. +\end{abstract} + +%% contents %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +\thetableofcontents + +\newpage + +%% body %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% + +%------------------------------------------------------------ +\section{Introduction} + +The Reflector program was originally written by Jose Carlos Gonz\'alez +and then improved by Harald Kornmayer. In September 2001 D. Bastieri +and C. Bigongiari released a new version (v.0.4) to adapt it to a +format change in the MMCS output. The Reflector program reads in MMCS +output files (cerxxxxxx files from corsika) and writes an output file +with the information about all the photons which reach the telescope +focal plane (taking into account atmospheric and mirror absorption) +and which are within the camera radius defined in the file +{\bf magic.def}. + +%------------------------------------------------------------ +\section{Description of simulation} + +The main steps of the simulation are: + +\begin{enumerate} + +\item Atmospheric absorption. + +\item Checking if the photon hits the dish. + +\item Aluminum absorption. + +\item Determination of the mirror hitted. + +\item Mirror reflection. + +\item Checking if the photon is inside the camera borders. + +\item Calculation of photon arrival time on camera. + +\end{enumerate} + +The reflection of each mirror element is simulated in a realistic way +by introducing a gaussian spread of the reflected photons positions on +the camera plane. The sigma of this PSF is defined via the +{\bf point\_spread} parameter in the telescope description file {\bf +magic.def}, and has a value of 0.5 cm, which corresponds approximately +to the quality of the MAGIC mirrors produced up to date. Also the +possible misalignment of mirror elements is simulated (see section +\ref{neededfiles}). + +\section{Notes on version 0.5} + +\begin{enumerate} + +\item An error was found by T. Hengstebeck in step 2 (see above) in version +0.4. This was the main reason for the release of this corrected +version 0.5. The error was in {\bf ph2cph.c}, and was a confusion between +{\it CORSIKA}'s coordinate system and the coordinate system of the +telescope. The error had no effect when the telescope was pointing at +zenith, but resulted on a loss of photons (which should have been +reflected), which became larger with increasing $\theta$. The +fractions of lost photons were negligible up to $\theta \simeq +10^\circ$ and then 0.006, 0.012, 0.019, 0.070, 0.286, 0.433 +respectively for $\theta = $ 15, 20, 25, 40, 60 and $70^\circ$. + +\item NEW VARIABLES: some variables which were unused in the event +header of the output have changed meaning to incorporate +some relevant items. The header size is the same as before, so this +output files will be readable by all {\bf camera} versions at least up +to 0.5. The twelve new variables (see header structure in section +\ref{out}) are the following: +% +\begin{itemize} +\item {\bf TelescopePhi, TelescopeTheta:} telescope orientation chosen in +the input card (in degrees). +\item {\bf ViewConeRadius:} if ViewConeRadius $> 0$, indicates the outer radius +of the viewing cone chosen in {\it CORSIKA} via the \texttt{VIEWCONE} +option for the random generation of the of the primaries' incidence +directions. The inner radius is assumed 0, and the direction around +which the cone is defined is given by the header variables {\bf ThetaMin}, +{\bf PhiMin} (which equal in that case {\bf ThetaMax}, {\bf PhiMax}). The +\texttt{VIEWCONE} option should be the standard for MAGIC MC +generation in the case of hadronic primaries. However, if ViewConeRadius +is 0, it will mean that the \texttt{VIEWCONE} option has not been used and +the generation of directions has been done in a ``square'' sky window +{\bf (PhiMin, PhiMax), (ThetaMin, ThetaMax)}, as in older versions of +{\it CORSIKA}. +\item {\bf num\_mirrors:} total number of mirrors in the dish. For +{\it historical} reasons we are using as default a dish with 920 +mirrors. This should perhaps be updated in the future to the final +design with (may be) 956 mirrors. It is not a very critical detail, +since the only difference will be a global change in the amount of +light reaching the camera, and this amount depends also on other +factors like mirror reflectivity (which in the real telescope will +change with time). +\item {\bf mean\_reflectivity:} mean value of the mirror reflectivity values +in the range 270 - 610 nm, as read from the input file +{\bf reflectivity.dat}. No spectral weighting is done on this mean, since at +the time of the calculation the Cherenkov spectrum is not known by the +program. In principle, we will still use a constant reflectivity value of 0.9, +independent of wavelength, but this may change in the future to render +the simulation more realistic. +\item {\bf longi\_Nmax, logi\_t0, longi\_tmax, longi\_a, longi\_b, longi\_c, +longi\_chi2:} longitudinal charged particle distribution +parameters and $\chi^2$ of the fit. See {\it CORSIKA} manual for +precise meaning of these (which changed slightly from version +5.61 onwards). The most important of them is {\bf longi\_tmax}, the +atmospheric depth (in g/cm$^2$) of the shower maximum. +\end{itemize} +% +\item We added an option to tell the Reflector program where (in +{\it CORSIKA}'s +coordinates) the telescope should be placed (see section +\ref{opt}). This is important because the cerxxxxxx files contain only +the photons which reach the ground +near the telescope (in the standard mode of production for MAGIC, +those hitting a sphere of 20 m diameter centered on the telescope), +and the previous versions of Reflector only worked if the +telescope was placed at its default position (0,0). For certain +studies it is sometimes necessary to shift the telescope to a +different position (for instance, to generate showers with impact +point fixed with respect to the telescope). + +\item In the magic.def file which comes with Reflector\_0.5 the value of the +parameter {\bf camera\_width} (radius around the center of the camera +beyond which the photons are not written to the Reflector output file) +has been changed from 100 to 70 cm, which allows to reduce the size of +the output files, while it is a value safe enough to keep all the +photons needed by the camera program. + +\item Removed some useless bits of code: in previous versions a +binary file, {\bf magic.def.mirr}, containing the mirror data was +created once the ASCII file {\bf magic.def} was read. Later, everytime the +Reflector was run, it read the mirror data from magi.def.mirr. Now +magic.def.mirr has been suppressed and the data are always read from +magic.def. Another obsolete file, {\bf focals.dat} has been removed +from the {\bf Data/} directory. + +\end{enumerate} + +%------------------------------------------------------------ +\section{How to Install Reflector Program \label{installation}} + +You can get the current version of the Reflector Program from the +MAGIC web page: \\ +{\bf http://hegra1.mppmu.mpg.de/MAGICWeb/ }\\ +You can find +the latest public version of this program as tarred gzipped file in +the Monte Carlo Download area (you need the usual password). You have to +download the file reflector\_0.5.tar.gz and then follow the +instructions below: + +\begin{description} +\item[Decompress the file using:] + gunzip reflector*.tar.gz +\item[Unpack the tar file with:] + tar xvf reflector*.tar +\item[Make symbolic links running the script:] + refl-install +\item[Go to the directory where the source files are:] + cd MagicProgs/Simulation/Detector/Reflector\_0.5/ +\item[Check if all dependencies are fulfilled:] + make depend +\item[Compile the program:] + make +\end{description} + +If everything goes right you should have an executable file called +{\bf reflector}. + +%------------------------------------------------------------ +\section{How to Run Reflector Program \label{running}} + +You need a steering card to run the Reflector program. You can find an +example in the {\bf MagicProgs/Simulation/Detector/Reflector\_0.5/input.card} +file. You have to modify this file according to your needs (see below +for instructions about steering card) and then run the program with the +following statement:\\ + +\hspace{1cm}{\bf reflector $<$ input.card} + +%------------------------------------------------------------ +\section{Needed Files \label{neededfiles}} + +The Reflector program needs some other files to run. These files are +the following: +\begin{itemize} +\item {\bf magic.def}: contains the description of MAGIC telescope +geometry, together with some other parameters needed by the Reflector +program. +\item {\bf axisdev.dat}: contains data to simulate the possible +deviation of the spot of each single mirror on the camera plane due +to its non perfect alignment. The values are x, y coordinates +distributed at random (according to a gaussian with $\sigma \simeq +0.5$ cm). +\item {\bf reflectivity.dat}: contains the mirror reflectivity index as +a function of the wavelength. +\end{itemize} + +All these files are usually in the {\bf +MagicProgs/Simulation/Detector/Data/} directory and in principle you +should {\bf not} make any change in them. + +%------------------------------------------------------------ +\section{Steering Card} + +The steering card sets all the parameters and options +to steer the reflection simulation. Each line of the steering card is +a statement with its parameters, if it is the case. Lines beginning +with \# are considered comments. The Reflector program parses all the +lines sequentially. Then if you repeat a statement with different +options only the last one will be considered. + +\subsection{Mandatory Commands} + +\begin{description} + +\item[reflector 0.5] + + This statement must be the first line of the steering card + file. The Reflector program checks it to verify if it is reading + a steering card. + +\item[output\_file /disk99/reflex/Gamma\_0\_7\_1001to1010\_w0.rfl] + + The output\_file command specifies the name and the + path of the output file. The path can be absolute, like in the + example above, or relative. Although any name can be used, + conventionally the Reflector program + output file name has the .rfl extension, and starts with + the primary particle name. The first number indicates the + zenith angle of the incident primaries, the second one + indicates the production site (7 is for Padua) and is related + to the random number generator seed used by CORSIKA. Then the run + number range is shown (10 runs in this case, from 1001 to + 1010). Each run corresponds to 10000 showers. Finally, the + label "w0" means no wobble mode was used (telescope pointing + at the source). Alternatively, the "w+" or "w-" labels (only + in gamma files) refer to the two pointings in the + Wobble-observation mode (see TDAS 01-05 by W. Wittek). + +\item[ct\_file ../Data/magic.def] + + The ct\_file statement defines where the program can find the + telescope characteristics. The path in the example above is + correct to run reflector in + MagicProgs/Simu\-la\-tion/De\-tector/Reflector\_0.5/ directory. + If you want to run it in a different directory you have to modify the + path accordingly. + +\item[atm\_model ATM\_CORSIKA] + The atm\_model statement says to the program what kind of + atmospheric absorption model to use. Possible choices are: + ATM\_CORSIKA, ATM\_ISO\-THERMAL, ATM\_90\-PER\-CENT and + ATM\_NO\-ATMO\-SPHE\-RE. + +\item[fixed\_target 0. 90.] + + This statement fixes the telescope axis position. The first + number is the zenith angle $\theta$ (deg) while the second is + the azimuthal angle $\phi$ (deg). This corresponds to {\it + CORSIKA}'s definition of primary particle incident direction + (see {\it CORSIKA} manual). $\phi = 90^\circ$ means that the + telescope is pointing towards East (bear in mind that in {\it + CORSIKA} $(\phi, \theta)$ indicates the direction of the {\it + momentum} of the incident particle). + + +\item[cer\_files] + + All the lines following this statement are considered files to + be processed by the Reflector program, one for each line, + eventually with their paths (see the example below). Therefore this + command must be the last one.\\ + \\ + cer\_files\\ + /disk99/cer001001\\ + /disk99/cer001002\\ + /disk99/cer001003\\ + ........ \\ + /disk99/cer001009\\ + /disk99/cer001010\\ + \\ + The cer file name can be followed by two numbers, for example: + \\ + /disk99/cer001001 376 5723\\ + \\ + In this case the program processes only the events between and + including the numbers given. + +\end{description} + +\subsection{Optional Commands \label{opt}} + +\begin{description} + +\item[verbose\_level 1] + + Sets the quantity of information printed out by Reflector + when running. Possible values are 0 to 4 + +\item[max\_events 50000] + + Fixes the maximum number of events to process. + +\item[energy\_cuts 100 1000] + + This statement forces the Reflector to process only showers + with primary energy between the given values (GeV). + +\item[seeds n1 n2] + + Seeds for the random number generators to used by the program + for the simulation of the absorption (both in the atmosphere + and on the mirror). Default values are 3141592 and + 2718182. + +\item[telescope\_position x y] + + Option included in version 0.5 of Reflector. Usually it is + not needed, since for normal MC production for MAGIC the + telescope is placed at the origin of coordinates (0,0). But, + if for some reason, we produce cerxxxxxx files with the + telescope in a different position, we must inform the + Reflector program in the input card using this option + (otherwise Reflector will fail to {\it find} the photons + in the cer file). + +\item[reflectivity\_file /path/reflectivity.dat] + + File containing mirror reflectivity as a function of + wavelength (see section \ref{neededfiles}). If this option is + not supplied, the program will look for + ``../Data/reflectivity.dat'' as previous versions of + Reflector did. + +\item[axisdev\_file /path/axisdev.dat] + + File containing single mirror spot deviation in {\bf x} and + {\bf y} on the camera in cm (see section + \ref{neededfiles}) for each mirror. If this option is not + supplied, the program will look for ``../Data/axisdev.dat'' + as previous versions of Reflector did. + +\end{description} + +%------------------------------------------------------------ +\section{Output file \label{out}} + +The output file begins with some ascii lines:\\ +\\ +\verb"reflector 0.5" \\ +\verb"START---RUN" \\ +\verb"START-EVENT" \\ +After the \verb"START-EVENT" flag there is a blank line and then the +binary event header, which contains the following informations (each +variable is a 4-byte float number): +\\ + +\begin{tabular}{ll} + +Variable & Description \\ +\hline + +EvtNumber & Event Number \\ +PrimaryID & Primary particle identification code \\ +Etotal & Primary particle total energy (GeV) \\ +Thick0 & CORSIKA's starting altitude in g/cm2 \\ +FirstTarget & CORSIKA's number of first target if fixed \\ +zFirstInt & Height of first interaction in cm \\ +p[3] & Primary particle momentum in x,y,-z directions (GeV) \\ +Theta & Primary particle zenith angle (rad) \\ +Phi & Primary particle azimuth angle (rad) \\ + +NumRndSeq & Number of different CORSIKA random sequences (max. 10) \\ +RndData[10][3] & RndData[i][0]: integer seed of sequence i \\ + & RndData[i][1]: number of offset random calls (mod +$10^6$) of sequence i. \\ + & RndData[i][2]: number of offset random calls ($/ +10^6$) of sequence i. \\ + +RunNumber & Run number \\ +DateRun & Date of run yymmdd \\ +Corsika\_version & Version of {\it CORSIKA} \\ + +NumObsLev & Number of observation levels (should be always 1 for +us) \\ +HeightLev & Height of observation level in cm \\ +num\_mirrors & Number of mirrors \\ +mean\_reflectivity & Mean reflectivity between 270 and 610 nm \\ +& \\ +& 6 next variables: CORSIKA longitudinal particle fit parameters \\ +& \hspace{0.5cm} (see CORSIKA manual for precise meaning and units)\\ +longi\_Nmax & Numer of charged particles at maximum \\ +longi\_t0 & Atmospheric depth of shower starting point (N=0) \\ +longi\_tmax & Atmospheric depth of shower maximum (g/cm$^2$) \\ +longi\_a & \\ +longi\_b & For {\bf longi\_a}, {\bf longi\_b}, {\bf longi\_c}, see CORSIKA manual \\ +longi\_c & \\ +longi\_chi2 & $\chi^2/dof$ of the fit\\ +& \\ +SlopeSpec & Energy spectrum slope \\ +ELowLim & Energy lower limit (GeV) \\ +EUppLim & Energy upper limit (GeV) \\ + +ThetaMin & Minimum Theta of primaries (deg) \\ +ThetaMax & Maximum Theta of primaries (deg) \\ +PhiMin & Minimum Phi of primaries (deg) \\ +PhiMax & Maximum Phi of primaries (deg) \\ + +CWaveLower & Wavelength lower limit (nm) \\ +CWaveUpper & Wavelength upper limit (nm) \\ +CorePos[2][20] & Core positions of randomized shower \\ +TimeFirst & Arrival time on camera of first photon (ns) \\ +TimeLast & Arrival time on camera of last photon (ns) \\ + + & Next three variables changed meaning in version 0.5: \\ + +telescopePhi & Telescope azimuth (rad). Measured from South, counter-clockwise \\ +telescopeTheta & Telescope zenith angle (rad) \\ + +ViewConeRadius & Outer radius (deg) in {\it CORSIKA}'s VIEWCONE +option, if used. Inner r is assumed 0.\\ + + +\hline +\end{tabular} +% +\newpage +% +\begin{tabular}{ll} + +Variable & Description \\ +\hline + + +CORSIKAPhs & Original photons written by {\it CORSIKA} \\ +AtmAbsPhs & Photons absorbed by the atmosphere \\ +MirrAbsPhs & Photons absorbed by the mirror \\ +OutOfMirrPhs & Photons outside the mirror \\ +BlackSpotPhs & Photons lost in the "black spot" \\ +OutOfChamPhs & Photons outside the camera \\ +CPhotons & Photons reaching the camera \\ + +\hline +\end{tabular} + +\vspace*{1cm} +The event header is followed by 8-word blocks, one for each photon +that reaches the camera. A photon block contains the following +variables: + +\begin{tabular}{ll} +Variable & Description \\ +\hline +w & Wavelength (nm) \\ +x, y & Impact point in camera coordinates (cm) \\ +u, v & Director cosines \\ +t & Arrival time on camera (ns) \\ +h & Production height (cm) \\ +phi & Incidence angle with respect to camera plane (rad) \\ +\hline +\end{tabular} + +After the last event photon block there is a blank line, an \verb$END---EVENT$ +flag, another blank line and then the following event. After the last +event in a run it appears the flag \verb$END-----RUN$, while after every +processed runs, you can find a \verb$END----FILE$ flag. + + +%------------------------------------------------------------ + +\section{Future improvements} +Possible improvements of the reflector simulation could be: +\begin{enumerate} +\item Introduce dependence of mirror reflectivity as a function of +wavelength using recent measurements performed on real mirrors. +\item Adittion of a Run header: some parameters which are the same for +each run are still kept (again for historical reasons) in the event +header. It would be better to move them to a Run header. This has not +yet been implemented in this version in order to make it compatible with +the corresponding version of the {\it camera} program. I would also +allow to include more detailed information on the used telescope +geometry (number and position of mirrors) and reflectivity (as a +function of wavelength). +\end{enumerate} +\par +Please contact \texttt{moralejo@pd.infn.it}. for suggestions on other +features to be implemented in future versions. + +\section{Appendix} + +The list of all Reflector files follows. +\begin{verbatim} + +refl-install + +MagicProgs/Simulation/Detector/Reflector_0.5/Makefile +MagicProgs/Simulation/Detector/Reflector_0.5/atm.c +MagicProgs/Simulation/Detector/Reflector_0.5/atm.h +MagicProgs/Simulation/Detector/Reflector_0.5/attenu.f +MagicProgs/Simulation/Detector/Reflector_0.5/config.mk.linux +MagicProgs/Simulation/Detector/Reflector_0.5/config.mk.linux-gnu +MagicProgs/Simulation/Detector/Reflector_0.5/config.mk.osf1 +MagicProgs/Simulation/Detector/Reflector_0.5/diag.c +MagicProgs/Simulation/Detector/Reflector_0.5/diag.h +MagicProgs/Simulation/Detector/Reflector_0.5/geometry.c +MagicProgs/Simulation/Detector/Reflector_0.5/geometry.h +MagicProgs/Simulation/Detector/Reflector_0.5/header.c +MagicProgs/Simulation/Detector/Reflector_0.5/header.h +MagicProgs/Simulation/Detector/Reflector_0.5/init.c +MagicProgs/Simulation/Detector/Reflector_0.5/init.h +MagicProgs/Simulation/Detector/Reflector_0.5/input.card +MagicProgs/Simulation/Detector/Reflector_0.5/lagrange.h +MagicProgs/Simulation/Detector/Reflector_0.5/parms.c +MagicProgs/Simulation/Detector/Reflector_0.5/parms.h +MagicProgs/Simulation/Detector/Reflector_0.5/ph2cph.c +MagicProgs/Simulation/Detector/Reflector_0.5/reflector.c +MagicProgs/Simulation/Detector/Reflector_0.5/version.h + +MagicProgs/Simulation/Detector/Reflector_0.5/doc/magic-tdas.sty +MagicProgs/Simulation/Detector/Reflector_0.5/doc/magiclogo.eps +MagicProgs/Simulation/Detector/Reflector_0.5/doc/refl.ps +MagicProgs/Simulation/Detector/Reflector_0.5/doc/refl.tex + +MagicProgs/Simulation/Detector/Data/axisdev.dat +MagicProgs/Simulation/Detector/Data/magic.def +MagicProgs/Simulation/Detector/Data/reflectivity.dat + + +\end{verbatim} + +%%% BIBLIOGRAPHY %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% + +%%>>>> Use the following if you are using BibTeX for bibliography +%\theBibliography + +%%>>>> Or the following if you include here by hand your +%%>>>> bibliographic entries + +\end{document} +% +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +%%% Upper-case A B C D E F G H I J K L M N O P Q R S T U V W X Y Z +%%% Lower-case a b c d e f g h i j k l m n o p q r s t u v w x y z +%%% Digits 0 1 2 3 4 5 6 7 8 9 +%%% Exclamation ! Double quote " Hash (number) # +%%% Dollar $ Percent % Ampersand & +%%% Acute accent ' Left paren ( Right paren ) +%%% Asterisk * Plus + Comma , +%%% Minus - Point . Solidus / +%%% Colon : Semicolon ; Less than < +%%% Equals = Greater than > Question mark ? +%%% At @ Left bracket [ Backslash \ +%%% Right bracket ] Circumflex ^ Underscore _ +%%% Grave accent ` Left brace { Vertical bar | +%%% Right brace } Tilde ~ +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +%% Local Variables: +%% mode:latex +%% mode:font-lock +%% mode:auto-fill +%% time-stamp-line-limit:100 +%% End: +%% EOF Index: trunk/MagicSoft/Simulation/Detector/ReflectorII/input.card =================================================================== --- trunk/MagicSoft/Simulation/Detector/ReflectorII/input.card (revision 1432) +++ trunk/MagicSoft/Simulation/Detector/ReflectorII/input.card (revision 1432) @@ -0,0 +1,27 @@ +reflector 0.5 +# +# Sample parameters file +# +verbose_level 1 +# +fixed_target 0. 90. +# +#Telescope x y (in cm): +telescope_position 0. 0. +# +max_events 1000000000 +#energy_cuts 800. 1000. +# +ct_file ../Data/magic.def +# +#reflectivity_file /mypath/Data/reflectivity.dat +# +#axisdev_file /mypath/Data/axisdev.dat +# +output_file /myout/my.rfl +# +atm_model ATM_CORSIKA +#atm_model ATM_NOATMOSPHERE +# +cer_files +/mydatadisk/cer014006