Difference between revisions of "S5 Testing and Performance Summary"
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| Line 25: | Line 25: | ||
|SL1||STB1-G1203202 ||1,4,17 || 0|| 0|| | |SL1||STB1-G1203202 ||1,4,17 || 0|| 0|| | ||
|- | |- | ||
| − | |SL1||STB2-G1203206 || | + | |SL1||STB2-G1203206 ||0 || 0|| 0|| |
|- | |- | ||
| − | |SL1||STB3-G1203199 | + | |SL1||STB3-G1203199 ||0 || 11,17 || 0|| |
|- | |- | ||
| − | |SL1||STB4-1203201 | + | |SL1||STB4-1203201 ||0 || 11,17 || 0|| |
|- | |- | ||
|SL1||STB5-G1203198 | |SL1||STB5-G1203198 | ||
Revision as of 15:59, 28 September 2013
Testing results
Signal Testing for the Wires
Signal testing performed to all S6's wires for cosmic rays, the testing was simultaneously with the wire burning process. In general the signal is detected when the voltage on the sense wire at least was 1200V, guard's 535V, and field's -750V.
The results are shown in the following table:
Testing results
Signal Testing for the Wires
Signal testing performed to all S6's wires for cosmic rays, the testing was simultaneously with the wire burning process. In general the signal is detected when the voltage on the sense wire at least was 1200V, guard's 535V, and field's -750V.
The results are shown in the following table:
| Super Layer | STP Board | Wires without any Signal | Hot wires | High Noise Wires | Notes |
| Super Layer | STP Board | Wires without any Signal | Hot wires | High Noise Wires | Notes |
| SL1 | STB1-G1203202 | 1,4,17 | 0 | 0 | |
| SL1 | STB2-G1203206 | 0 | 0 | 0 | |
| SL1 | STB3-G1203199 | 0 | 11,17 | 0 | |
| SL1 | STB4-1203201 | 0 | 11,17 | 0 | |
| SL1 | STB5-G1203198 | ||||
| SL1 | STB6-G1203200 | ||||
| SL1 | STB7-G1203204 | ||||
| SL2 | STB1-K1200874 | ||||
| SL2 | STB2-K1200875 | ||||
| SL2 | STB3-K1200873 | ||||
| SL2 | STB4-K1200869 | ||||
| SL2 | STB5-K1200871 | ||||
| SL2 | STB6-K1200870 | ||||
| SL2 | STB7-K1200872
|