Difference between revisions of "S5 Testing and Performance Summary"

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The results are shown in the following table:
 
The results are shown in the following table:
  
{| border="1"  |cellpadding="20" cellspacing="0
+
{| border="1"  | cellpadding="20" cellspacing="1
 
|-
 
|-
 
|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||STB1-G1203202 ||1,4 || 0|| 0||
 
|-   
 
|-   
 
|SL1||STB2-G1203206  ||0 || 0|| 0||
 
|SL1||STB2-G1203206  ||0 || 0|| 0||
Line 29: Line 29:
 
|SL1||STB3-G1203199  ||0 || 11,17 || 0||
 
|SL1||STB3-G1203199  ||0 || 11,17 || 0||
 
  |-
 
  |-
|SL1||STB4-1203201  ||0 || 11,17 || 0||
+
|SL1||STB4-1203201  ||0 || || 0||
 
  |-
 
  |-
|SL1||STB5-G1203198
+
|SL1||STB5-G1203198 ||0 || 0|| 0||
 
|-
 
|-
|SL1||STB6-G1203200
+
|SL1||STB6-G1203200   ||0 || 87|| 0||
 
  |-
 
  |-
|SL1||STB7-G1203204
+
|SL1||STB7-G1203204 ||0 || 0|| 0||
 
|-
 
|-
|SL2||STB1-K1200874
+
|SL2||STB1-K1200874 || 1,4,19 || 0|| 0||
 
|-
 
|-
|SL2||STB2-K1200875
+
|SL2||STB2-K1200875||0 || 0|| 0||
 
|-
 
|-
|SL2||STB3-K1200873
+
|SL2||STB3-K1200873||0 || 0|| 67,71,74|| 47,65 has a small signal
 
|-
 
|-
|SL2||STB4-K1200869
+
|SL2||STB4-K1200869||0 || 0|| 0||
 
|-
 
|-
|SL2||STB5-K1200871
+
|SL2||STB5-K1200871||0 || 0|| 0||
 
|-
 
|-
|SL2||STB6-K1200870
+
|SL2||STB6-K1200870||1 || 9,87|| 0|
 
|-
 
|-
|SL2||STB7-K1200872
+
|SL2||STB7-K1200872||7 || 27,50,69,85,93|| 0||
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
|}
 
|}

Latest revision as of 18:21, 7 December 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 0 0
SL1 STB2-G1203206 0 0 0
SL1 STB3-G1203199 0 11,17 0
SL1 STB4-1203201 0 0
SL1 STB5-G1203198 0 0 0
SL1 STB6-G1203200 0 87 0
SL1 STB7-G1203204 0 0 0
SL2 STB1-K1200874 1,4,19 0 0
SL2 STB2-K1200875 0 0 0
SL2 STB3-K1200873 0 0 67,71,74 47,65 has a small signal
SL2 STB4-K1200869 0 0 0
SL2 STB5-K1200871 0 0 0
SL2 STB6-K1200870 1 9,87
SL2 STB7-K1200872 7 27,50,69,85,93 0