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Re-calibrating UCAL to correct for the light absorbtion.
The algebra here provides technical background for
the material discussed in 4.4.2.
By
and
I denote the amplitude and calibration constant in
case of no light absorbtion, and by
and
- the actual ones,
respectively.
If the light intensity in scintillator gets attenuated with distance
and the scintillator
length is
, then the amplitude observed in a single channel
(averaged over all positions in
and eliminating the pedestal) is not
as it were in the absence of attenuation, but
.
Each UCAL tower is served by two PMT tubes, so we have
and
;
their gains are matched so that
.
Calibrating a channel
, I require that
 |
(98) |
where
is to be determined and
is known.
We will denote
as
to indicate that this is
the energy observable which we know how to calibrate.
The left and right PMT register the light which passes the distance
and
, respectively (if the source is point-like).
We use the product of the two so that our new observable is
 |
(99) |
It is independent of
, but has yet to be calibrated, i.e.
related to
.
Next we notice that
from A.1, and
that in the absence of absorption for the gain-matched tubes
, and therefore
 |
(100) |
where we recognized that the
and
-dependent prefactor can be
expressed in terms of the easily measurable averages.
This means that calibration can be restored for the product with the help
of the expression:
 |
(101) |
By itself, this result is natural and predictable.
Its value lies in the fact that absorbtion length is now related to
observables.
Next: Subtracting background effects in
Up: Hadron Single- and Multiparticle
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Mikhail Kopytine
2001-08-09