titles_qslp

                              Titles: QSLP
                              ============
 
    Contact:  S. Biller, Oxford.
 
    Revision History:-
    ================
 
    3.02  S. Biller       First version

  The bank number specifies to 1/2 crate to which the calibrations refer.
     These numbers run from 1-18, so bank numbers 1 and 2 refer to the first
     and second half of crate 0.

  The offset to the main link for a particular calibration value is given by

   OFFSET = 6*[(ice-1)*(nchannels*ncards/2) + (ich-1)*(ncards/2) + (jca-1)] 
            + 2*(N-1)
 
  where ice is the cell index (1 to nells), ich is the channel index
  (1 to nchannels), jca is the card index for this 1/2 crate (1 to ncards/2),
  and N refers to either QHS,QHL or QLX charges (thus running from 1 to 3).


Titles Files
------------

   These are of the form   qeca_yyyymmdd_vv.dat 
 
 
Verification
------------
 
 

Description
-----------
 
    Holds ECA QSlopes and intercepts  (linear fit)
 

Data Words
----------
 
    Data types: B(bit), I, F, D(double), H(hollerith 4 char)
 
   +1   I   linear fit QHS slope times 100 for 1st cccc (defined by OFFSET)
   +2   I   linear fit QHS intercept times 10 for 1st cccc (defined by OFFSET)
   +3   I   linear fit QHL slope times 100 for 1st cccc (defined by OFFSET)
   +4   I   linear fit QHL intercept times 10 for 1st cccc (defined by OFFSET)
   +5   I   linear fit QLX slope times 100 for 1st cccc (defined by OFFSET)
   +6   I   linear fit QLX intercept times 10 for 1st cccc (defined by OFFSET)

   +7   I   linear fit QHS slope times 100 for 2nd cccc (defined by OFFSET)
   +8   I   linear fit QHS intercept times 10 for 2nd cccc (defined by OFFSET)
   +9   I   linear fit QHL slope times 100 for 2nd cccc (defined by OFFSET)
   +10  I   linear fit QHL intercept times 10 for 2nd cccc (defined by OFFSET)
   +11  I   linear fit QLX slope times 100 for 2nd cccc (defined by OFFSET)
   +12  I   linear fit QLX intercept times 10 for 2nd cccc (defined by OFFSET)
     .
     .
     .
     .
     .
     .
     .
     .