electron cloud & vacuum pressure observations: 2011 proton run

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Electron cloud & vacuum pressure observations: 2011 proton run G. Bregliozzi on the behalf of the TE-VSC group 1. General layout of the LHC vacuum system 2. Electron cloud at 25 & 50 ns: Vacuum Observation 3. Pressure Spikes & Heating effects 4. Strategy and Mitigation solutions 5. Conclusion

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G. Bregliozzi on the behalf of the TE-VSC group. Electron cloud & vacuum pressure observations: 2011 proton run. General layout of the LHC vacuum system Electron cloud at 25 & 50 ns: Vacuum Observation Pressure Spikes & Heating effects Strategy and Mitigation solutions Conclusion. - PowerPoint PPT Presentation

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Page 1: Electron cloud  & vacuum pressure observations: 2011 proton run

Electron cloud & vacuum pressure observations: 2011 proton run

G. Bregliozzi on the behalf of the TE-VSC group

1. General layout of the LHC vacuum system2. Electron cloud at 25 & 50 ns: Vacuum

Observation3. Pressure Spikes & Heating effects4. Strategy and Mitigation solutions

5. Conclusion

Page 2: Electron cloud  & vacuum pressure observations: 2011 proton run

The LHC cryogenic vacuum system

2G. Bregliozzi – TE-VSC-

LBV

Stand Alone Magnet at 4.5 K in LSSBeam Screen @ 5 – 20K

Unbaked

LHe

RT

compatibility reason with cryo vacuum system

L ~ 0.5 m

Cold-Warm transition

ARC and IT at 1.9 K

It takes advantage of the cryogenic cooling for the superconducting magnets: the pumping is distributed onto surfaces cooled at temperature in the range 1.9 to 20 K.

Cold beam pipes (Stand Alone Magnet) are also present in the 8 long straight sections.

Cold-Warm transition present in each connections between room temperature and cryogenic system: unbaked due to compatibility reason with cryogenic vacuum system and vacuum sectorization.

GaugeGauge

Page 3: Electron cloud  & vacuum pressure observations: 2011 proton run

The LHC RT vacuum system

Bake

d

3G. Bregliozzi – TE-VSC-LBV

“Combined” sector both side of each experiment

Both beams circulates in the same beam pipe“Twin” sector

Beams circulate in different beam pipes

Uncoated parts in the room temperature beam pipes

The pumping system rely mainly on TiZrV thin film coating with some localised ion pumps NEG-NEG AreaGauge

Gauge Gauge

Page 4: Electron cloud  & vacuum pressure observations: 2011 proton run

Electron Cloud at 25 & 50 ns

Vacuum Observation

Page 5: Electron cloud  & vacuum pressure observations: 2011 proton run

Vacuum System Performances

5G. Bregliozzi – TE-VSC-LBV

V. Baglin, R. Cimino, 2003

Secondary Electron Yield: TiZrV

C. Scheuerlein et al. Appl.Surf.Sci 172(2001)

No electron cloud in NEG areas after vacuum activation

Baked and unbaked cryogenic areas requires scrubbing

Page 6: Electron cloud  & vacuum pressure observations: 2011 proton run

10-11

10-6

E-cloud Effects in LHC Vacuum at 50 ns

Bunch spacing 50 ns

SP ElectronsElectrons

6G. Bregliozzi – TE-VSC-LBV

No Scrubbing and Vacuum Cleaning: Almost as received surfaces

Factor 5

• Pressure increase is function of the (Baked and Unbaked), pumping speed and length of the area .• Two distinctive area in the LHC: Unbaked and baked.

1·10-7

2·10-8

444 bunches

Data from 20.11.2010

Page 7: Electron cloud  & vacuum pressure observations: 2011 proton run

Bunch spacing 25 ns

10-11

10-6

E-cloud Effects in LHC Vacuum at 25 ns

7G. Bregliozzi – TE-VSC-LBV

Factor 50

Cold-Warm Transition apparently high pressure increase..........

Baked System: clear indication of pre-scrubbing and pre-

cleaning at 50 nsBunch spacing 25 ns

8·10-8

1.5·10-9

2100 bunches

Still two distinctive area in the LHC: Unbaked and baked.

Data from 14.10.2011

Page 8: Electron cloud  & vacuum pressure observations: 2011 proton run

Heat load due to electron cloud effects:Bending magnets and drift spaces

8G. Bregliozzi – TE-VSC-LBV

Simulated heat load due to electron cloud as a function of the maximum secondary electron yield for bending magnets and drift spaces in the LHC

arcs

F. Zimmermann: LHC Project Note 201

Drift: Baked and Unbaked transition

Bend: ARC with saw tooth

25 ns Baked and Unbaked

transitions: almost fully scrubbed.

Pressure increase: dominated by desorption of beam screen (~24 Km of LHC)

LHC performance limited by electron density in ARCs

with high power dissipated in the beam

screen.

50 ns Larger conditioning rate in

field free regions compared to ARC and stand alone magnets.

Pressure increase in baked and unbaked transitions

was limiting the LHC performance.

Page 9: Electron cloud  & vacuum pressure observations: 2011 proton run

E-cloud Effects in LHC Vacuum at 25 nsEffectiveness of the scrubbing

Case of Cold-Warm Transition

8·10+10 p/b

25 ns operation just at the limit of the multipacting threshold

Absence of “optimized” beam cleaning

9G. Bregliozzi – TE-VSC-LBV

New beam time is required for further scrubbing and analysis at 25 ns

Page 10: Electron cloud  & vacuum pressure observations: 2011 proton run

Synchrotron radiation Effectiveness of 25 ns scrubbing run

• Pressure reduction observed during the year while accumulating photon dose• Accumulated dose so far 1023 ph/m

Beam conditioning of the arc vacuum system

Further cleaning after 25 ns MDs

10G. Bregliozzi – TE-VSC-LBV

Page 11: Electron cloud  & vacuum pressure observations: 2011 proton run

Pressure Spikes &

Heating Effects

Page 12: Electron cloud  & vacuum pressure observations: 2011 proton run

Pressure Spikes in LSS2 and LSS8

• Frequently, pressure spikes are observed mainly at LSS2 and LSS8• Location of pressure spikes is in LSS2 and LSS8: TCTVB-TCLIA/TCDD areasFill 2266 Fill 2267- Spikes during stable

beams above 10-8 mbar- D1L2, D1L8, D1R8

- Spikes during injection and stable beams above 10-7 mbar

- D1L8, D1R8

Page 13: Electron cloud  & vacuum pressure observations: 2011 proton run

Point 2 Left side: Side view

Typical default in the RF Finger

TCDD

D1L2

VPIA.A151.4L2.X

VGPB.120.4L2.X

Christmas break: The non-conform modules will be repaired and consolidated.

Further studies ongoing.

Heating of RF fingers and spring

holding the RF fingers in contact

with the slots

Spring and RF fingers were

deformed between May and November

2011

During beam operation possible electric arcs could induce degassing: pressure spikes 13G. Bregliozzi – TE-VSC-

LBV

Page 14: Electron cloud  & vacuum pressure observations: 2011 proton run

14G. Bregliozzi – TE-VSC-LBV

Pressure increase in TDI LSS2 and LSS8

Target Dump Injection for LHC (78 m from IP2)LSS 2

LSS 8

TDI Jaws Distance:• 22 mm: pressure increased• 55mm : pressure stays at 10-8 mbar

Christmas break: the pumping at TDI2L will be doubled

22mm 55mm

Page 15: Electron cloud  & vacuum pressure observations: 2011 proton run

CMS Forward Area: Pressure Increase

Pressure excursion at 18 m does not seems to be triggered

by multipacting

• CMS background suffers from pressure rise localized around 18 m from the IP

Fill 2241 at 50 ns bunch spacing

Christmas break: X-Ray and upgrade of pumping system 15G. Bregliozzi – TE-VSC-

LBV

Fill 2251 at 25 ns bunch spacing, small pressure rise were detected

• The CMS magnetic field ensure the multipacting suppression

Page 16: Electron cloud  & vacuum pressure observations: 2011 proton run

16G. Bregliozzi – TE-VSC-LBV

ALICE Background• ALICE background is dominated by the pressure rise at 110 m

from IP that must be below 10-8 mbar

• One layer (1 Km) of solenoid was installed at each extremity to check potential electron cloud activity: a small reduction of the pressure was observed with solenoid ON.

Christmas break: layout will change, NEG reactivation and possible solenoid re-installation (2 layer).

Page 17: Electron cloud  & vacuum pressure observations: 2011 proton run

Strategy &

Mitigation Solutions

Page 18: Electron cloud  & vacuum pressure observations: 2011 proton run

LHC Strategy for Electron cloud

18G. Bregliozzi – TE-VSC-LBV

The LHC Strategy is scrubbing“Operating the LHC with nominal parameters relies on the surface conditioning (scrubbing) effect, akin to the

process of an RF cavity, by which the secondary emission yield decreases from an initial value of about 2 to about 1.4 or below, after depositing a sufficient dose of electrons on the chamber wall. During commissioning, when the

yield is still high, an increased bunch spacing and/or a reduced bunch intensity will greatly reduce the heat load….” From LHC Design report (p. 116).

• Scrubbing and vacuum cleaning at 25 ns For operation at 50 ns Some LSS sectors are vented during Christmas break: need a

new scrubbing and cleaning of these area.

Scrubbing Run Scenario: Optimize time and efficiency.

Higher and stable beam intensity >1.1 – 1.2·1011 p/b

Fill the machine with lower number of bunches while keeping stable intensity: 72 trains injection, then 144 trains and finally 288 trains.

Determination of scrubbing efficiency: when the beam is dumped, injection of just 1 train with a fixed p/b intensity to check pressure increase. Could be applied after each TS for 24-48 h of time or for a dedicated MD (7-10

days) : the earlier the better.

Page 19: Electron cloud  & vacuum pressure observations: 2011 proton run

Mitigation solutions

19G. Bregliozzi – TE-VSC-LBV

Mitigation Solutions for Heating Effects• TDI: It was shown that running the machine with a gap of 50 mm limit the

increase of pressure and temperature in the TDI jaw.

• VAMTF Modules (Location of pressure spikes):• Installation of different springs to withstand high temperature.• Add NEG cartridges to increase pumping speed.

• ALICE ZDC in LSS2:• Layout will be changed during Christmas break.• NEG reactivation and possible solenoid re-installation(2 layers).

Mitigation Solutions for Electron Cloud• Installation of solenoids in non-coated areas:

In MKI regions to decrease pressure increase during scrubbing run and ID800 to decrease ALICE background.

• Increase local pumping speed by the use of NEG cartridges: Vacuum pilot sector for 2012 run: TDI, VAMTF module in LSS2

and in the cold-warm transition of ITL2 & ITR2.

Page 20: Electron cloud  & vacuum pressure observations: 2011 proton run

ConclusionsELECTRON CLOUD

Scrubbing period with 50 ns was very efficient to reduce the stimulated gas desorption and increase the multipacting

threshold• During this period, pressures increased in the range 10-7 mbar. • During the year, average pressures were in the range 10-9

mbar.

25 ns beams stimulated further gas desorption from the beam screen of ARCs and stand alone magnets: pressure increased

again in the range 10-7 mbar •Another period with 25 ns with <ppb> above threshold is needed for further scrubbing and analysis.

20G. Bregliozzi – TE-VSC-LBV

PRESSURE SPIKES AND HEATING EFFECTS• Pressure increase in TDI and ALICE should be significantly reduced thanks to new layout and the increased parking distance between the TDI jaws.•Consolidation of vacuum module: New spring material and additional pumping.• CMS: Upgrade pumping system and X-rays as complementary diagnostic