Difference between revisions of "S5 Testing and Performance Summary"

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|SL1||STB1-G1203202 ||1,4,17 || 0|| 0||
 
|SL1||STB1-G1203202 ||1,4,17 || 0|| 0||
 
|-   
 
|-   
|SL1||STB2-G1203206  ||1,4,17 || 0|| 0||
+
|SL1||STB2-G1203206  ||0 || 0|| 0||
 
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|-  
|SL1||STB3-G1203199
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|SL1||STB3-G1203199 ||0 || 11,17 || 0||
 
  |-
 
  |-
|SL1||STB4-1203201  
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|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