orbit effect from main dipoles in sps at high energy
DESCRIPTION
Orbit effect from main dipoles in SPS at high energy. K. Cornelis. Orbit after alignment at 6000ms (FT optics). Plan H RMS= 1.608 Plan V RMS= 1.226. The B-field in SPS dipoles. Magnetising field from windings (depends on geometry of windings ). - PowerPoint PPT PresentationTRANSCRIPT
Orbit effect from main dipoles in SPS at high energy
K. Cornelis
Stephane Cettour Cave
Orbit after alignment at 6000ms (FT optics)
• Plan H RMS= 1.608• Plan V RMS= 1.226
The B-field in SPS dipoles
Magnetising field from windings (depends on geometry of windings)
Field due to polarisation in the yoke (depends on geometry of the yoke, composition of the yoke, and field)
Yoke and windings geometry such that best field quality at 300 GeV.
SPS dipoles
-1000 0 1000 2000 3000 4000 5000 6000 70000
0.5
1
1.5
2
2.5
Bfield
current (A)
Fiel
d
450 GeV
300 GeV
Static fields of dipoles• Yoke composition as homogenous as can be
(laminations of special melt).
• Magnets measured and shimmed to give the correct at 1T (~220GeV).
• Different places of the yoke will come to saturation at different magnetising fields, resulting in a change of geometry of the fields. In identical magnets this change should be the same but, e.g. shims have a different effect then the yoke when in saturation.
• From about 2004 until about 2010, uncorrected dipoles have been installed. Recent beam based measurements with uncorrected C- coated magnets showed errors from 10 to 25 mrad
-1000 0 1000 2000 3000 4000 5000 6000 70000
0.5
1
1.5
2
2.5
Bfield
current (A)
Fiel
d
Dynamic effects from induced currents in vacuum chamber
dB/dt
B ~ -dB/dt
B
x
Chromaticity effect from Eddy Currents
0 500 1000 1500 2000 2500 3000 3500 4000 4500 5000-0.2
00.20.40.60.8
11.21.41.6
Horizontal chroma error from eddy currents in a cngs cycle
Cycle time
Chro
mati
cyty
corr
ectio
n
0 1000 2000 3000 4000 5000 60000
0.10.20.30.40.50.60.7
horizontal chroma error from eddy currents in pilot cycle.
Cycle time
chro
mati
city
com
pens
ation
Dipole error from decaying eddy currents
0 200 400 600 800 1000 1200 1400
-2
-1.5
-1
-0.5
0
0.5
1
Radi
al p
ositi
on
Time in cycle
2000 4000 6000 8000 10000 12000 14000
-3
-2
-1
0
1
2
3
4
5
0 2000 4000 6000 8000 10000 12000 140000
1000
2000
3000
4000
5000
6000
7000
LHC fast
Amplitude and decay time depend on shape of vacuum chamber, thickness and specific resistance of material.
Effect : 6 mrad/magnet at 26 GeV0.35 mrad/magnet at 450 GeV
If magnet differences are at the % level, the orbit kick is less than .05mrad/magnet at 450 GeV
Possible sources of “local” errors
Weird vacuum chambers
Possible sources of “local” errors: Earth loops
Earth loops around magnets can enhance the field suppression
Short between spires in the coil gives a strong field supression proportional to dB/dt
Normally the short circuit gets worse rapidly and the orbit becomes so bad that the beam is destroyed and the magnet has to be changed
In position 3.26 a temperature dependent dB/dt kick could be observed 10
/8/2
012
20:2
4
10/8
/201
2 21
:36
10/8
/201
2 22
:48
10/9
/201
2 0:
00
10/9
/201
2 1:
12
10/9
/201
2 2:
24
10/9
/201
2 3:
36
10/9
/201
2 4:
48
10/9
/201
2 6:
00
10/9
/201
2 7:
12
-160
-140
-120
-100
-80
-60
-40
-20
0
Kick
at m
ax d
B/dt
/B
Time after restart
The problem is there since October but it does not get worse.
Summary and Conclusions• In the horizontal plane, the orbit at high energy is not only due to
misalignment, but results also from dipole errors.• During several years the shimming of dipoles was neglected resulting in
horizontal orbit kicks of a few tens or micro radians. • The errors due to eddy currents in the vacuum chamber are negligible
at 450 GeV.• Earth loops around magnets can make a bigger effect but it is difficult to
know how much. We have no total picture of the state of the machine. The bad earth connections will be removed during LS1.
• These errors are normally stable in time.• Short circuit between windings can give huge kicks, but it normally kills
the magnet in a short time. However, it can not be excluded that very weak shorts stay stable and vary slowly in time.