A. Verweij, TE-MPE. 2 Feb 2009, LHC Performance Workshop – Chamonix 2009
Training the dipolesTraining the dipoles
- Training during HWC- Training during HWC
- Estimate to reach 6, 6.5, and 7 TeV- Estimate to reach 6, 6.5, and 7 TeV
- Quench propagation- Quench propagation
Arjan Verweij, TE-MPEArjan Verweij, TE-MPE
Acknowledgment to everybody involved in the HWC
A. Verweij, TE-MPE. 2 Feb 2009, LHC Performance Workshop – Chamonix 2009
QuenchQuenchDipole Quench: Transition from the superconducting to the normal state
(usually due to local temperature rise), resulting in a detectable resistive
voltage, exceeding the threshold voltage for a duration larger than the
discrimination time.
Quench classification:
Heater induced/provoked quench
Natural (training) quench
Secondary quench (due to
increase of the bath temperature,
ramp rate, etc)
(Beam induced quench)
Calculations based on experiments, G. Willering, PhD thesis 2009
A local energy deposition of about
100 J is enough to trigger a quench
(i.e. a falling raindrop of 2 mm
diameter).
Circuit quench: Heater
induced/Natural quench +
secondary quenches.
A. Verweij, TE-MPE. 2 Feb 2009, LHC Performance Workshop – Chamonix 2009
Sector 1st training quench [A]
I_max
[A]# training quenches
Starting in:
# ALS # ANS # NOE
1-2 - 9310 0 0 0 0
2-3 - 9310 0 0 0 0
3-4 - 8715 (bus) 0 0 0 0
4-5 9789 10274 3 0 0 3
5-6 10004 11173 27 0 1 26
6-7 - 9310 0 0 0 0
7-8 8965 9310 1 0 1 0
8-1 - 9310 0 0 0 0
RB circuit quenches during HWCRB circuit quenches during HWC
A. Verweij, TE-MPE. 2 Feb 2009, LHC Performance Workshop – Chamonix 2009
Magnet distribution per sectorMagnet distribution per sector
4956 56
46
28
57 5464
96
60 65
46
42
36 40 24
9
38 33
62
84
61 60 66
0
20
40
60
80
100
120
140
160
S12 S23 S34 S45 S56 S67 S78 S81
3 (NOE)
2 (ANS)
1 (ALS)
A. Verweij, TE-MPE. 2 Feb 2009, LHC Performance Workshop – Chamonix 2009
Nr. of quenches in SM-18 to reach given currentNr. of quenches in SM-18 to reach given current
7000
8000
9000
10000
11000
12000
13000
10 100 1000 10000
Number of quenches
Cu
rren
t [A
]
All dipoles
Dipoles used in S56
x 11
x 6.8
A. Verweij, TE-MPE. 2 Feb 2009, LHC Performance Workshop – Chamonix 2009
Training during HWCTraining during HWC
8500
9000
9500
10000
10500
11000
11500
12000
12500
13000
1 10 100 1000
Quench number
Qu
ench
cu
rren
t [A
]
5.5 TeV
7 TeV
6.5 TeV
6 TeV
S45
S56 in SM-18
S56
S78
190
A. Verweij, TE-MPE. 2 Feb 2009, LHC Performance Workshop – Chamonix 2009
RB circuit S45: comparison with SM-18RB circuit S45: comparison with SM-18
7000
8000
9000
10000
11000
12000
13000
0 20 40 60 80 100 120 140
Magnet number (order by 1st quench in SM18)
Cu
rren
t [A
]
ALS: 1st training quench SM18
ANS: 1st training quench SM18
NOE: 1st training quench SM18
NOE: Quenches sector 45
7 TeV
6 TeV
A. Verweij, TE-MPE. 2 Feb 2009, LHC Performance Workshop – Chamonix 2009
RB circuit S56: comparison with SM-18RB circuit S56: comparison with SM-18
7000
8000
9000
10000
11000
12000
13000
0 20 40 60 80 100 120 140
Magnet number (ordered by 1st quench in SM18)
Cu
rren
t [A
]
ALS: 1st training quench SM18
ANS: 1st training quench SM18
NOE: 1st training quench SM18
ANS: Quenches sector 56
NOE: Quenches sector 56
7 TeV
6 TeV
A. Verweij, TE-MPE. 2 Feb 2009, LHC Performance Workshop – Chamonix 2009
Retesting of NOE magnet 3383 in SM-18Retesting of NOE magnet 3383 in SM-18
11691
1069110544
11304
12346
7000
8000
9000
10000
11000
12000
13000
Cu
rren
t [A
]
Quench 1st test (Aug 2005)
Quenches 2nd test (Oct 2008)
Stable operation at 12850 A
1st cold test (Aug 2005) 2nd cold test (Oct 2008)
Data from N. Catalan Lasheras
Note: 3383 suffered a transport accident, during which diode, IFS box and N-line were damaged
A. Verweij, TE-MPE. 2 Feb 2009, LHC Performance Workshop – Chamonix 2009
Sector
Number of magnets Number of quenches
ALS ANS NOE@ 6 TeV
(±2)
@ 6.5 TeV
(±30%)
1-2 49 96 9 00 44
2-3 56 60 38 11 88
3-4 56 65 33 11 88
4-5 46 46 62 22 1212
5-6 28 42 84 11 1515
6-7 57 36 61 22 1212
7-8 54 40 60 22 1212
8-1 64 24 66 22 1313
Total 154 154 154 1111 8484
Estimated dipole training to reach 6 and 6.5 TeVEstimated dipole training to reach 6 and 6.5 TeV
Est. 1: Based on 115 MB’s that have been submitted to a thermal cycle in SM-18 (2008 before HWC, P. Xydi and A. Siemko)
Est. 2: Extrapolation from sector 5-6 data + est. 1 for ALS & ANS
Est. 3: 2 quenches per NOE magnet + est. 1 for ALS & ANS
Est. 4: 3 quenches per NOE magnet + est. 1 for ALS & ANS
A. Verweij, TE-MPE. 2 Feb 2009, LHC Performance Workshop – Chamonix 2009
Sector
Number of magnets Number of quenches
ALS ANS NOE Est. 1 Est. 2 Est. 3 Est. 4
1-2 49 96 9 2222 4141 4040 4949
2-3 56 60 38 2323 9797 9292 130130
3-4 56 65 33 2121 8787 8383 116116
4-5 46 46 62 2222 145145 136136 198198
5-6 28 42 84 2121 190190 178178 262262
6-7 57 36 61 2020 142142 133133 194194
7-8 54 40 60 1414 140140 132132 192192
8-1 64 24 66 1919 151151 142142 208208
Total 154 154 154 162162 993993 936936 13491349
Estimated dipole training to reach 7 TeVEstimated dipole training to reach 7 TeV
Est. 1: Based on 115 MB’s that have been submitted to a thermal cycle in SM-18 (2008 before HWC, P. Xydi and A. Siemko)
Est. 2: Extrapolation from sector 5-6 data + est. 1 for ALS & ANS
Est. 3: 2 quenches per NOE magnet + est. 1 for ALS & ANS
Est. 4: 3 quenches per NOE magnet + est. 1 for ALS & ANS
The number of “circuit quenches” might be a bit smaller as compared to the number of “dipole quenches” due to “parallel training” of 2 or more dipoles during the same circuit quench.
A. Verweij, TE-MPE. 2 Feb 2009, LHC Performance Workshop – Chamonix 2009
RB quench propagationRB quench propagationCryogenic recovery time: see talk Serge ClaudetCryogenic recovery time: see talk Serge Claudet
Almost instantaneous (within 1 sec)
Observed 11 times on 8 different magnets. Caused by:
- an almost equal quench current
- an unbalance > 100 mV (triggering the QPS) due to very different inter-strand
coupling currents between the 2 apertures,
- traveling voltage waves due to the opening of the dump switches,
- other noise.
See also the talk of Karl Hubert Mess.
Through thermal propagation (typical delay 30-300 s)
Observed for all quenches > 6 kA.
Statistics for quenches > 9 kA: propagation to 1 dipole: 3
propagation to 2 dipoles: 9
propagation to 3 dipoles: 15
propagation to 4 dipoles: 6
propagation to 5 dipoles: 1
A. Verweij, TE-MPE. 2 Feb 2009, LHC Performance Workshop – Chamonix 2009
Example thermal quench propagation (I_q=10274 A)Example thermal quench propagation (I_q=10274 A)LBBLA.27R4: 0 s, 10274 A
LBBLC.27R4: 123.5 s, 2844 A (355.7 s, 238 A)
LBALA.27R4: 46.6 s, 6464 ALBALB.26R4: 109.1 s, 3330 A
LBBLA.26R4: 167.4 s, 1748 A
A. Verweij, TE-MPE. 2 Feb 2009, LHC Performance Workshop – Chamonix 2009
Thermal quench propagationThermal quench propagation
0
50
100
150
200
250
300
350
0 2000 4000 6000 8000 10000 12000
Circuit quench current [A]
Del
ay s
eco
nd
ary
qu
ench
[s]
Same half-cell, 15.7 m apart
Same half-cell, 31.3 m apart
Next half-cell, 22.1 m apart
Next half-cell, 37.8 m apart
Next half-cell, 53.4 m apart
A. Verweij, TE-MPE. 2 Feb 2009, LHC Performance Workshop – Chamonix 2009
Thermal quench propagationThermal quench propagation
0
1000
2000
3000
4000
5000
6000
7000
8000
0 2000 4000 6000 8000 10000 12000
Circuit quench current [A]
Sec
on
dar
y q
uen
ch c
urr
ent
[A]
Same half-cell, 15.7 m apart
Same half-cell, 31.3 m apart
Next half-cell, 22.1 m apart
Next half-cell, 37.8 m apart
Next half-cell, 53.4 m apart
A. Verweij, TE-MPE. 2 Feb 2009, LHC Performance Workshop – Chamonix 2009
Quench at 6.9 kA
Quench at 7.0 kA
Quench at 9.0 kA
B30R7 0 0 0
C30R7 61.3 s 58.8 s 40.2 s
A30R7 111.1 s 108.4 s 47.0 s
Reproducibility of thermal quench propagationReproducibility of thermal quench propagation
Quench at 10.7 kA
Quench at 10.9 kA
C15R5 0 0
B15R5 45.1 s 38.3 s
A15R5 81.5 s 72.1 s
C14R5 281 s 270 s
Quench starting in B30R7at 3 different currents
Quench starting in C15R5at 2 different currents
Due to secondary quenching, each quench causes the firing of the heaters of about 4 magnets.
High-field-High-field-heater firingheater firing
SM-18 at warm 1150
SM-18 at cold, 1500 A 1150
SM-18 at cold, training 4100
HWC at cold, 0 A 1700
HWC at cold, I > 0 A 240
A. Verweij, TE-MPE. 2 Feb 2009, LHC Performance Workshop – Chamonix 2009
Conclusion: Dipole trainingConclusion: Dipole training
6 sectors reached 9310 A (5.5 TeV) without a quench. 1 sector showed 1
quench<9310 A, and in 1 sector a busbar joint opened/melted before reaching
9310 A.
Training of S56 showed a completely unexpected behaviour of the NOE
magnets, triggering quenches well below the respective 1st training quenches
in SM-18.
All training quenches in S56 happened (for the moment) on different
magnets, except in one case when a NOE magnet showed a detraining step
(10910 A 10720 A).
Retest in SM-18 of one NOE magnet (that was not installed in the tunnel and
previously tested in Aug 2005) showed a similar time-relaxation effect.
The expected number of RB circuit quenches needed to reach 6, 6.5, and 7
TeV is about 10, 80, and 900 respectively. Note that 900 is a rough estimate
since it is based on a large extrapolation of the S56 training curve and the re-
test of only one NOE magnet. Assuming training in all 8 sectors in parallel,
with 3 quenches per day would then require about 60 days to reach 7 TeV, and
about the same number of heater firings as the entire SM-18 test campaign.
A. Verweij, TE-MPE. 2 Feb 2009, LHC Performance Workshop – Chamonix 2009
Conclusion: Quench propagationConclusion: Quench propagation
Thermal quench propagation time is strongly affected by current level, cell
geometry, cooling conditions, etc.
Large variations in quench propagation time are observed for different
positions in the sector. Reproducibility seems however good.
High field (>7 T) dipole quenches usually cause 2-4 adjacent magnets to
quench while ramping down the circuit. Due to long propagation times (typically
30-100 s to the nearest neighbour) the total dissipated energy in a half cell is
about twice the stored energy of a single MB.
Several cases have been observed where the MB-MB propagation time was less
than 1 s, due to unbalanced coupling currents, traveling waves, noise and similar
quench current level.