Changeset 6603 for trunk


Ignore:
Timestamp:
02/18/05 16:03:18 (20 years ago)
Author:
gaug
Message:
*** empty log message ***
Location:
trunk/MagicSoft/TDAS-Extractor
Files:
2 edited

Legend:

Unmodified
Added
Removed
  • trunk/MagicSoft/TDAS-Extractor/Criteria.tex

    r6602 r6603  
    110110
    111111
    112 \subsection{Applicability for Different Sampling Speeds / No Pulse Shaping.}
    113112
    114 The current read-out system of the MAGIC telescope~\cite{Magic-DAQ} with 300~MSamples/s is relatively slow compared to the fast pulses of
    115 about 2\,ns FWHM of Cherenkov pulses.
    116 To acquire the pulse shape an artificial pulse shaping to about 6.5\,ns FWHM is used. Thereby also more night sky background light
    117 is integrated which acts as noise.
    118 
    119 For 2 ns FWHM fast pulses a 2 GSamples/s FADC provides at least 4 sampling points. This permits a reasonable reconstruction of the pulse shape. First prototype tests with fast digitization systems for MAGIC have been successfully conducted \cite{GSamlesFADC}. The signals have been reconstructed within the common MAGIC Mars software framework.
    120 
    121 
    122 \subsection{CPU Requirements}
    123 
    124 Depending on the reconstruction algorithm the signal reconstruction can take a significant amount of CPU time.
    125 Especially the more sophisticated signal extractors can be time consuming which search for the position of the Cherenkov signals
    126 in the recorded FADC time slices and perform a fit to these samples. At any case, the extractor should not be significantly slower than
    127 the reading and writing routines of the MARS software.
    128 
    129 Thus, for an online-analysis a different extraction algorithm might be chosen than for the final most accurate
    130 reconstruction of the signals offline.
    131 
    132 \subsection{Treatment of Calibration Pulses}
     113\subsection{Intrinsic Differences between Calibration and Cosmics Pulses}
    133114
    134115The calibration pulse reconstruction sets two important constraints to the signal extractor:
     
    144125\end{enumerate}
    145126
     127\subsection{Reconstruction Speed}
     128
     129Depending on the reconstruction algorithm the signal reconstruction can take a significant amount of CPU time.
     130Especially the more sophisticated signal extractors can be time consuming which search for the position of the Cherenkov signals
     131in the recorded FADC time slices and perform a fit to these samples. At any case, the extractor should not be significantly slower than
     132the reading and writing routines of the MARS software.
     133
     134Thus, for an online-analysis a different extraction algorithm might be chosen than for the final most accurate
     135reconstruction of the signals offline.
     136
     137\subsection{Applicability for Different Sampling Speeds / No Pulse Shaping.}
     138
     139The current read-out system of the MAGIC telescope~\cite{Magic-DAQ} with 300~MSamples/s is relatively slow compared to the fast pulses of
     140about 2\,ns FWHM of Cherenkov pulses.
     141To acquire the pulse shape an artificial pulse shaping to about 6.5\,ns FWHM is used. Thereby also more night sky background light
     142is integrated which acts as noise.
     143
     144For 2 ns FWHM fast pulses a 2 GSamples/s FADC provides at least 4 sampling points. This permits a reasonable reconstruction of the pulse shape. First prototype tests with fast digitization systems for MAGIC have been successfully conducted \cite{GSamlesFADC}. The signals have been reconstructed within the common MAGIC Mars software framework.
     145
    146146%%% Local Variables:
    147147%%% mode: latex
  • trunk/MagicSoft/TDAS-Extractor/Results.tex

    r6589 r6603  
    88
    99\begin{table}[htp]
     10\small{%
     11\rotatebox{90}{%
    1012\centering
    11 \small{
    12 \begin{tabular}{|c|c|c|c|c|c|c|c|c|c|c|}
     13\begin{tabular}{|c|c|c|c|c|c|c|c|c|c|c|c|}
    1314\hline
    1415\hline
    15 \multicolumn{11}{|c|}{\large Tested Characteristics} \rule{0mm}{6mm} \rule[-2mm]{0mm}{6mm} \hspace{-3mm}\\
     16\multicolumn{12}{|c|}{\large Tested Characteristics} \rule{0mm}{6mm} \rule[-2mm]{0mm}{6mm} \hspace{-3mm}\\
    1617\hline
    1718\hline
    18 Nr. & Name         &  Res.  & Bias &    Stab. & Stab.  &  Stab. & Res. & Stab.  & Lin. & Speed \\
    19     &              &   $\widehat{S}$    & $\widehat{S}$  &  $\widehat{S}$  &  pulse & low- & $\widehat{T}$ & $\widehat{T}$ &  $\widehat{S}$  & \\
    20     &              &      &     &   &  shape & gain & & &  &  \\
     19Nr. & Name         &  Res.  & Res. & Bias &    Stab. & Stab.  &  Stab. & Res. & Stab.  & Lin. & Speed \\
     20    &              &  $\widehat{S}$ & $\widehat{S}$ & $\widehat{S}$  &  $\widehat{S}$  &  pulse & low- & $\widehat{T}$ & $\widehat{T}$ &  $\widehat{S}$  & \\
     21    &              &  size & const.  &    &   &  shape & gain & & &  &  \\
    2122\hline                                                     
    2223\hline                                                     
    23 1   & Fix Win. (4,4)   & \no & -- & \ok & \no & \no & n/a & n/a & \no & \best \\   
    24 2   & Fix Win. (4,6)   & \ok & -- & \ok & \no & \no & n/a & n/a & \no   & \best \\   
    25 3   & Fix Win. (6.6)   & \ok & -- & \ok & \ok & \no & n/a & n/a & \ok   & \ok \\   
    26 4   & Fix Win. (8,8)   & \no & -- & \ok & \ok & \ok & n/a & n/a & \best & \ok \\   
    27 5   & Fix W. (14,10)   & \no & -- & \no & \ok & \ok & n/a & n/a & \best & \ok \\   
     241   & Fix Win. (4,4)   & \no & \no & -- & \ok & \no & \no & n/a & n/a & \no & \best \\   
     252   & Fix Win. (4,6)   & \no & \no & -- & \ok & \no & \no & n/a & n/a & \no   & \best \\   
     263   & Fix Win. (6.6)   & \ok & \ok & -- & \ok & \ok & \no & n/a & n/a & \ok   & \ok \\   
     274   & Fix Win. (8,8)   & \no & \ok & -- & \ok & \ok & \ok & n/a & n/a & \best & \ok \\   
     285   & Fix W. (14,10)   & \no & \ok & -- & \no & \ok & \ok & n/a & n/a & \best & \ok \\   
    2829\hline                                 
    29 6   & FW. Spl. (4,4) & \no & -- & \ok & \no & \no & n/a  &  n/a & \no & \ok \\   
    30 7   & FW. Spl. (4,6) & \ok  & -- & \ok & \no & \no & n/a  &  n/a & \no & \ok \\   
    31 8   & FW. Spl. (6.6) & \ok  & -- & \ok & \ok & \no & n/a  &  n/a & \no & \ok \\   
    32 9   & FW. Spl. (8,8) & \no  & -- & \ok & \ok & \ok & n/a  &  n/a & \ok & \ok \\   
    33 10  & FW. Spl (14,10) & \no  & -- & \no & \ok & \ok & n/a  &  n/a & \ok & \ok \\   
     306   & FW. Spl. (4,4) & \ok  & \no & -- & \ok & \no & \no & n/a  &  n/a & \no & \ok \\   
     317   & FW. Spl. (4,6) & \ok  & \no & -- & \ok & \no & \no & n/a  &  n/a & \no & \ok \\   
     328   & FW. Spl. (6.6) & \ok  & \ok & -- & \ok & \ok & \no & n/a  &  n/a & \no & \ok \\   
     339   & FW. Spl. (8,8) & \no  & \ok & -- & \ok & \ok & \ok & n/a  &  n/a & \ok & \ok \\   
     3410  & FW. Spl (14,10) & \no  & \ok &  -- & \no & \ok & \ok & n/a  &  n/a & \ok & \ok \\   
    3435\hline                               
    35 11  & FW. Pk S. (2,2)& \no  & -- & \no & \no & \no & n/a  &  n/a & \no & \ok \\   
    36 12  & FW. Pk S. (4,4)& \no  & -- & \ok & \no & \no & n/a  &  n/a & \no & \ok \\   
    37 13  & FW. Pk S. (4.6)& \ok & -- & \ok & \no & \no & n/a  &  n/a & \no & \ok \\   
    38 14  & FW. Pk S. (6,6)& \ok  & -- & \ok & \ok & \no & n/a  &  n/a & \no & \ok \\   
    39 15  & FW. Pk S. (8,8)& \no  & -- & \ok & \ok & \ok & n/a  &  n/a & \ok & \ok \\   
    40 16  & FW Pk S (14,10)& \no  & -- & \no & \ok & \ok & n/a  &  n/a & \ok & \ok \\   
     3611  & FW. Pk S. (2,2)& \no  & \no & -- & \no & \no & \no & n/a  &  n/a & \no & \ok \\   
     3712  & FW. Pk S. (4,4)& \no  & \no & -- & \ok & \no & \no & n/a  &  n/a & \no & \ok \\   
     3813  & FW. Pk S. (4.6)& \no  & \no & -- & \ok & \no & \no & n/a  &  n/a & \no & \ok \\   
     3914  & FW. Pk S. (6,6)& \ok  & \ok & -- & \ok & \ok & \no & n/a  &  n/a & \no & \ok \\   
     4015  & FW. Pk S. (8,8)& \no  & \ok & -- & \ok & \ok & \ok & n/a  &  n/a & \ok & \ok \\   
     4116  & FW Pk S (14,10)& \no  & \ok & -- & \no & \ok & \ok & n/a  &  n/a & \ok & \ok \\   
    4142\hline                               
    42 17  & Slid. W. (2,2)       & \ok & \ok & \ok & \no & \no & \no & \no & \no & \ok \\   
    43 18  & Slid. W. (4,4)       & \ok & \ok & \ok & \ok & \ok & \no & \no & \no & \ok \\   
    44 19  & Slid. W. (4.6)       & \ok & \ok & \ok & \ok & \ok & \ok & \no & \ok & \ok \\   
    45 20  & Slid. W. (6,6)       & \no & \ok & \ok & \ok & \ok & \no & \ok & \ok & \ok \\   
    46 21  & Slid. W. (8,8)       & \no & \ok & \ok & \ok & \ok & \ok & \ok & \ok & \ok \\   
    47 22  & Slid. W. (14,10)       & \no & \ok & \ok & \ok & \ok & \no & \ok & \ok & \ok \\   
     4317  & Slid. W. (2,2)       & \ok & \no & \ok & \ok & \no & \no & \no & \no & \no & \ok \\   
     4418  & Slid. W. (4,4)       & \ok & \ok & \ok & \ok & \ok & \ok & \no & \no & \no & \ok \\   
     4519  & Slid. W. (4.6)       & \ok & \ok & \ok & \ok & \ok & \ok & \ok & \no & \ok & \ok \\   
     4620  & Slid. W. (6,6)       & \no & \ok & \ok & \ok & \ok & \ok & \no & \ok & \ok & \ok \\   
     4721  & Slid. W. (8,8)       & \no & \ok & \ok & \ok & \ok & \ok & \ok & \ok & \ok & \ok \\   
     4822  & Slid. W. (14,10)       & \no & \no & \ok & \ok & \ok & \ok & \no & \ok & \ok & \ok \\   
    4849\hline                               
    49 23  & Spline Ampl.           & \ok & \no & \no & \nt   & \ok & \ok   & \no & \no & \ok \\
    50     &                        &     &     &     & \test &     &       &     &     &     \\
    51 24  & Splne Int. (1,1.5)     & \ok & \ok & \ok & \nt   & \ok & \best & \ok & \no & \ok \\
    52     &                        &     &     &     & \test &     &       &     &     &     \\
    53 25  & Spline Int. (2,3)      & \ok &\ok  & \best&\nt   & \ok & \best & \ok & \ok & \no \\
    54     &                        &     &     &     & \test &     &       &     &     &     \\
    55 26  & Spline Int. (4,6)      & \ok &\ok  & \ok & \ok & \ok & \best & \ok & \ok & \no \\
    56 27  & Spline Int. (6,9)      & \no &\best& \ok & \ok & \ok & \best & \ok & \ok & \no \\
     5023  & Spline Ampl.           & \ok & \no & \no & \no & \nt   & \ok & \ok   & \no & \no & \ok \\
     51    &                        &     &     &     &     & \test &     &       &     &     &     \\
     5224  & Splne Int. (1,1.5)     & \ok & \no & \ok & \ok & \nt   & \ok & \best & \ok & \no & \ok \\
     53    &                        &     &     &     &     & \test &     &       &     &     &     \\
     5425  & Spline Int. (2,3)      & \ok & \ok & \ok  & \best&\nt   & \ok & \best & \ok & \ok & \no \\
     55    &                        &     &     &     &     & \test &     &       &     &     &     \\
     5626  & Spline Int. (4,6)      & \ok & \ok & \ok  & \ok & \ok & \ok & \best & \ok & \ok & \no \\
     5727  & Spline Int. (6,9)      & \no & \ok & \best& \ok & \ok & \ok & \best & \ok & \ok & \no \\
    5758\hline                                                                         
    58 28  & Dig. Filt. (6,6)       & \ok   &\ok & \ok & \ok  & \ok & \ok  & \ok & \ok & \ok \\
    59 29  & Dig. Filt. (4,4)       & \best &\ok & \ok & \ok  & \ok & \best& \ok & \ok & \ok \\
     5928  & Dig. Filt. (6,6)       & \ok & \ok & \ok & \ok & \ok  & \ok & \ok  & \ok & \ok & \ok \\
     6029  & Dig. Filt. (4,4)       & \best & \no & \ok & \ok & \ok  & \ok & \best& \ok & \ok & \ok \\
    6061\hline
    6162\hline
     
    6566charge signal $\widehat{S}$ and time $\widehat{T}$, and speed. \ok\ means that the extractor has passed the
    6667test, without being among the best. \no\ means that the extractor has severely failed the test and should
    67 not be taken because of that reason. \best\ means that the extractor(s) have come out as best of the particular test.
     68not be taken because of that reason. \best\ means that the extractor(s) have come out as best of the particular test.}
    6869}
    6970\label{tab:result}
Note: See TracChangeset for help on using the changeset viewer.