Total energy information is one of the most effective triggers to
identify hadronic events in high energy annihilations. The
advantage of the total energy trigger is that the trigger logic itself
can be simply built as a fast trigger in regard to the trigger timing
latency in data acquisition and the deposit energy of beam backgrounds
in the calorimeter is usually very soft.
Analog-sum signals of STM, called GATESUM, are further processed in an
analog adder (AAA) when the deposit energy in TC is above the
threshold value. This arrangement minimizes incoherent electronics
noise contribution from each TC. AAA first adds up to five GATESUM
signals depending on the cylindrical -direction and the other
analog adder (AAB) finally produces an entire
-ring analog sum
signal. As shown in Fig.
, the
-rings
depending on the
-direction consists of 12 units in the barrel
and 5 units in the end-cap regions, i.e. 3 in the forward and 2 in the
backward end-cap. The scheme of two stage analog summation simplifies
the complexity of cabling between the detector and the electronics hut
located about 30 m away. The current analog driving method was adopted
to reduce the signal attenuation and ground loop effects.
Bhabha events are triggered using back-to-back conditions in the
center of mass frame. Table shows 11 types
of Bhabha triggers based on each
-ring summation. The
neighboring combinations are slightly overlapped with the next
-ring in order to save Bhabha events passing through the
boundary region. These logics provide the trigger efficiency greater
than 99 in real data taking runs.
Type | Logic | Threshold (GeV) |
1 | F1+F2+B1+B2 | 9.0 |
2 | F2+F3+B1+B2+C11 | 9.0 |
3 | F2 | 6.5 |
4 | F3+C10+C11 | 9.0 |
5 | C1+C9+C10 | 9.0 |
6 | C1+C2+C9 | 9.0 |
7 | C2+C8+C9 | 9.0 |
8 | C3+C7+C8 | 9.0 |
9 | C4+C6+C7 | 9.0 |
10 | C5+C6 | 9.0 |
11 | C10 | 3.5 |
Figure (a) shows the singles rate of the total
energy trigger for cosmic rays as a function of threshold
energy. Electronics noise and cosmic ray contributions are clearly
separated around 200 MeV, and the rms noise level is about 50 MeV. For
the physics trigger of total deposit energy, the threshold of about 1
GeV has been used stably.