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The Status of the SNS 3 rd SPL Collaboration Meeting CERN Nov. 11-13, 2009 Sang-ho Kim SCL Area Manager SNS/ORNL

The Status of the SNS 3 rd SPL Collaboration Meeting CERN Nov. 11-13, 2009 Sang-ho Kim SCL Area Manager SNS/ORNL

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Page 1: The Status of the SNS 3 rd SPL Collaboration Meeting CERN Nov. 11-13, 2009 Sang-ho Kim SCL Area Manager SNS/ORNL

The Status of the SNS3rd SPL Collaboration Meeting

CERNNov. 11-13, 2009

Sang-ho KimSCL Area Manager

SNS/ORNL

Page 2: The Status of the SNS 3 rd SPL Collaboration Meeting CERN Nov. 11-13, 2009 Sang-ho Kim SCL Area Manager SNS/ORNL

2 Managed by UT-Battellefor the U.S. Department of Energy

Outlines

• SNS operational status• Technical Issues and status

– RFQ– Foil– HVCM– Beam loss & Activation– SCL

• Power Upgrade; Impact on SCL• Summary

Page 3: The Status of the SNS 3 rd SPL Collaboration Meeting CERN Nov. 11-13, 2009 Sang-ho Kim SCL Area Manager SNS/ORNL

3 Managed by UT-Battellefor the U.S. Department of Energy

SNS Accelerator Complex

945 ns

1 ms macropulse

Cur

rent

mini-pulse

Cur

rent

1ms

Front-End:Produce a 1-msec

long, chopped, H- beam

1 GeV LINAC

Accumulator Ring: Compress 1 msec

long pulse to 700 nsec

Chopper system makes gaps

Ion Source2.5 MeV 1000 MeV87 MeV

CCLCCL SRF, =0.61SRF, =0.61 SRF, =0.81SRF, =0.81

186 MeV 387 MeV

DTLDTLRFQRFQ

Accumulator Ring

RTBT

Target

Injection Extraction

RF

Collimators

Liquid Hg Target

PUP

1300 MeV

Page 4: The Status of the SNS 3 rd SPL Collaboration Meeting CERN Nov. 11-13, 2009 Sang-ho Kim SCL Area Manager SNS/ORNL

4 Managed by UT-Battellefor the U.S. Department of Energy

Parameters DesignIndividually

achieved

Highest production

beam

Beam Energy (GeV) 1.0 1.01 0.93

Peak Beam current (mA) 38 40 36

Average Beam Current (mA) 26 26 24

Beam Pulse Length (s) 1000 1000 825

Repetition Rate (Hz) 60 60 60

Beam Power on Target (kW) 1440 1030 1030

Linac Beam Duty Factor (%) 6.0 5.0 5.0

Beam intensity on Target (protons per pulse) 1.5 x 1014 1.55x 1014 1.1 x 1014

SCL Cavities in Service 81 80 80

Major Parameters achieved vs. designed

Page 5: The Status of the SNS 3 rd SPL Collaboration Meeting CERN Nov. 11-13, 2009 Sang-ho Kim SCL Area Manager SNS/ORNL

5 Managed by UT-Battellefor the U.S. Department of Energy

SNS Beam Power Performance History1 MW beam power on target achieved in routine operation

Ion Source,LEBT

Stripperfoil

TargetCMS leak

HVCM

Page 6: The Status of the SNS 3 rd SPL Collaboration Meeting CERN Nov. 11-13, 2009 Sang-ho Kim SCL Area Manager SNS/ORNL

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Smooth Running…

Page 7: The Status of the SNS 3 rd SPL Collaboration Meeting CERN Nov. 11-13, 2009 Sang-ho Kim SCL Area Manager SNS/ORNL

7 Managed by UT-Battellefor the U.S. Department of Energy

Sometimes not…

Page 8: The Status of the SNS 3 rd SPL Collaboration Meeting CERN Nov. 11-13, 2009 Sang-ho Kim SCL Area Manager SNS/ORNL

8 Managed by UT-Battellefor the U.S. Department of Energy

Power delivery goals for FY09

0100200300400500600700800900

1000110012001300140015001600170018001900200021002200230024002500

1 3 5 7 9 11 13 15 17 19 21 23 25 27 29 31 33 35 37 39 41 43 45 47 49 51 53

Weeks Since October 1, 2008

Inte

gra

ted

Be

am

Po

we

r (M

W-h

rs)

ActualInternal Goal

Commitment

Internal Goal 2471.3Commitment 1977.0Actual 2161.4

Difference 184.4(actual-commitment)

Page 9: The Status of the SNS 3 rd SPL Collaboration Meeting CERN Nov. 11-13, 2009 Sang-ho Kim SCL Area Manager SNS/ORNL

9 Managed by UT-Battellefor the U.S. Department of Energy

FY09 Neutron Production hours goalsFY09 NP Hours Goals

0

200

400

600

800

1000

1200

1400

1600

1800

2000

2200

2400

2600

2800

3000

3200

3400

3600

3800

4000

4200

1 3 5 7 9 11 13 15 17 19 21 23 25 27 29 31 33 35 37 39 41 43 45 47 49 51 53Weeks

Hrs

. NP Scheduled Hours

NP Commitment Hours

NP Delivered Hours

Internal Goal 4125.6Commitment 3506.8Delivered 3541.2

Difference 34.4(delivered-commitment)

Page 10: The Status of the SNS 3 rd SPL Collaboration Meeting CERN Nov. 11-13, 2009 Sang-ho Kim SCL Area Manager SNS/ORNL

10 Managed by UT-Battellefor the U.S. Department of Energy

High Intensity Beam Studies – 7/11/20091 Hz beam

• The linac delivered the full pulse length• For the first time we verified the Ring can stably store

and extract the design intensity of 1.5 x1014 ppp

Cur

rent

(m

A)

Time relative to Ring Extraction (turns)

Linac Beam waveform: • ~ 1 msec long• produces the design intensity

Beam Pulse Extracted from the Ring:• Full baseline design intensity stored and extracted• No gross instability observed

Page 11: The Status of the SNS 3 rd SPL Collaboration Meeting CERN Nov. 11-13, 2009 Sang-ho Kim SCL Area Manager SNS/ORNL

11 Managed by UT-Battellefor the U.S. Department of Energy

Technical Issues and Status

Page 12: The Status of the SNS 3 rd SPL Collaboration Meeting CERN Nov. 11-13, 2009 Sang-ho Kim SCL Area Manager SNS/ORNL

12 Managed by UT-Battellefor the U.S. Department of Energy

Resonance error

Loosing closed-loop

RFQ instability• It was difficult to get stable operation at 60 Hz, >700us

– >30 min. down time in a day– Resonance error goes down loosing closed loop

Resonance error

Vane water temperature

10 min.

20 kHz

• One of limitations for 1 MW; − Since March 09; an extensive investigation− Why? What causes this instability? Limiting condition?− How can we improve the stability of operation?

Page 13: The Status of the SNS 3 rd SPL Collaboration Meeting CERN Nov. 11-13, 2009 Sang-ho Kim SCL Area Manager SNS/ORNL

13 Managed by UT-Battellefor the U.S. Department of Energy

All stable except net RF power resonance error fluctuation

• Resonance error; pure passive parameter• Net RF power=forward power – reflected power

+/-2 kHz

+/-10 kWNet RF power

Resonance error

Water temperature

Page 14: The Status of the SNS 3 rd SPL Collaboration Meeting CERN Nov. 11-13, 2009 Sang-ho Kim SCL Area Manager SNS/ORNL

14 Managed by UT-Battellefor the U.S. Department of Energy

RFQ Instability; findings• Direct correlation between Net RF power and res. Error

– When Net power > +40 kW RFQ becomes unstable• Changes in resonance error

– Vanes are getting hotter/colder at a constant field, water temperature• Load changes are clearly observed when

– Hydrogen flow rate is changed; slow response

– (Source off) vs. (source on/beam off); fast response

– (Source on/beam off) vs. (source on/beam on); fast response• Theory

– RFQ (especially vane) absorbs hydrogen from ion source

– Hydrogen are desorbed by ion beam bombardments

– Local vacuum goes up (gauge reading at the wall may not see any changes)

– Local discharge (very mild) starts; discharge conditions changes

– Vane temperature changes resonance error changes

– When discharge reaches a runaway condition instability

Page 15: The Status of the SNS 3 rd SPL Collaboration Meeting CERN Nov. 11-13, 2009 Sang-ho Kim SCL Area Manager SNS/ORNL

15 Managed by UT-Battellefor the U.S. Department of Energy

RFQ operation improvements

• Minimize H2 flow rate in Ion Source (minimize H2 absorption)• Better source alignment (minimum, uniform desorption)• Operate chiller in a good regulation region• Run the gradient at a lower end

– No affection in transmission, beam loss, beam quality

• Run at positive resonance error (around 12 kHz ± 5kHz)– Colder vane

• New auto tuning mechanism (LLRF)– Fine tuning; pulse width adjustment (+/- 30 us)– Coarse tuning; chiller temperature at 0.1 C step

No trip due to instability at 60 Hz, 900 us (limited by HVCM pulse width) during this operation period started on 8/29/09

Page 16: The Status of the SNS 3 rd SPL Collaboration Meeting CERN Nov. 11-13, 2009 Sang-ho Kim SCL Area Manager SNS/ORNL

16 Managed by UT-Battellefor the U.S. Department of Energy

Foil issues• May 09 ~ June 09; foil failures at >700 kW run• June 09~July 09; ~ 400 kW• Causes?

– Best foil failure theory to date is that one of the primary causes is vacuum breakdown (arcing) caused by charge build up on the stripper foils, caused by SEM and maybe thermionic electron emission

– Another primary cause is reflected convoy electrons and possibly also electrons from trailing edge multipacting

– Some of our foil failures also involved convoy electrons hitting the foil bracket

Cathode spot?

Page 17: The Status of the SNS 3 rd SPL Collaboration Meeting CERN Nov. 11-13, 2009 Sang-ho Kim SCL Area Manager SNS/ORNL

17 Managed by UT-Battellefor the U.S. Department of Energy

Foil failures

(Failed May 3)

(Failed May 3)

(Failed June 12)

tear

(Failed June 15)

(Used for high intensity run July 11-13)

Page 18: The Status of the SNS 3 rd SPL Collaboration Meeting CERN Nov. 11-13, 2009 Sang-ho Kim SCL Area Manager SNS/ORNL

18 Managed by UT-Battellefor the U.S. Department of Energy

Foil Fluttering & Glowing Edge/Spot

Page 19: The Status of the SNS 3 rd SPL Collaboration Meeting CERN Nov. 11-13, 2009 Sang-ho Kim SCL Area Manager SNS/ORNL

19 Managed by UT-Battellefor the U.S. Department of Energy

Foil Status

• Our best guess to date is that we have multiple foil failure mechanisms, and the biggest ones are vacuum breakdown, reflected convoy electrons, and trailing edge multipacting

• The Sep – Dec run has new Ti brackets, new foil mounting method, and diamond foils with a longer free length

• Also an HBC foil, and a diamond foil mounted at an angle• The new instrumentation (foil camera, temperature

measurement, clearing electrode, faster vacuum update rates) should help us to understand what is going on

• No foil failure since September and till now in November– But still need more understandings

Page 20: The Status of the SNS 3 rd SPL Collaboration Meeting CERN Nov. 11-13, 2009 Sang-ho Kim SCL Area Manager SNS/ORNL

20 Managed by UT-Battellefor the U.S. Department of Energy

HVCM Improvement

• New capacitors• New IGBTs, physical configuration changes, etc• Running at about 82 % of design duty• This run (since September 1, 09~)

– Much less down time due to smoke alarm related– Still major down time in SNS

Page 21: The Status of the SNS 3 rd SPL Collaboration Meeting CERN Nov. 11-13, 2009 Sang-ho Kim SCL Area Manager SNS/ORNL

21 Managed by UT-Battellefor the U.S. Department of Energy

Activation Buildup Trends3 Month Run Cycle Interval

• Finishing the run at lower power helps reduce the residual activation• SCL is also lower because of reduced loss/C• SNS is not limited by beam loss

Page 22: The Status of the SNS 3 rd SPL Collaboration Meeting CERN Nov. 11-13, 2009 Sang-ho Kim SCL Area Manager SNS/ORNL

22 Managed by UT-Battellefor the U.S. Department of Energy

SNS SCL, Operations and Performance• The first high-energy SC linac for protons, and the first pulsed operational

machine at a relatively high duty • We have learned a lot in the last 5 years about operation of pulsed SC linacs:

– Operating temperature, Heating by electron loadings (cavity, FPC, beam pipes), Multipacting & Turn-on difficulties, HOM coupler issues, RF Control, Tuner issues, Beam loss, interlocks, alarms, monitoring, …

• Current operating parameters are providing very stable and reliable SCL operation – Less than one trip of the SCL per day mainly by errant beam or control noise

• Proactive maintenance strategy (fix annoyances/problems before they limit performance)

• Beam energy (930 MeV) is lower than design (1000 MeV) due to high-beta cavity gradient limitations (mainly limited by field emission)

• No cavity performance degradation has occurred to Oct. 09– Field emission very stable – Recently Nov. 09; One cavity has been showing performance degradation

• Several cryomodules were successfully repaired without disassembly– Multiple beam-line repairs were successfully performed

Page 23: The Status of the SNS 3 rd SPL Collaboration Meeting CERN Nov. 11-13, 2009 Sang-ho Kim SCL Area Manager SNS/ORNL

23 Managed by UT-Battellefor the U.S. Department of Energy

Electron loading usually results in end group heating/beam pipe heating + quenching/gas burst

Electron Loading and Heating (Due to Field Emission and Multipacting)

• Field Emission due to high surface electric field

Multipacting; secondary emission– At resonant condition (geometry, RF field)– At sweeping region; many combinations

are possible for MP Temporally; filling, decay time Spatially; tapered region Non-resonant electrons accelerated

radiation/heating

– Mild contamination easily Processible– But bad surface processing is very

difficult in a cryomodule (operational)Initial VTA or CM HP tests could have a significant conditioning effects for both. But most dangerous moment !

Page 24: The Status of the SNS 3 rd SPL Collaboration Meeting CERN Nov. 11-13, 2009 Sang-ho Kim SCL Area Manager SNS/ORNL

24 Managed by UT-Battellefor the U.S. Department of Energy

SNS Cavity Operating RegimeAfter initial commissioning and conditioningsurface conditions are quite stable

re-distribution of gases (slow & fast)processible

Gradient settings in SNS SCL; Not uniform gradients as designedBut as high as individually achievableR

adia

tion

(in lo

g, a

rb. U

nit)

Eacc

FE onsetRadiation onset

MP Surface condition

Page 25: The Status of the SNS 3 rd SPL Collaboration Meeting CERN Nov. 11-13, 2009 Sang-ho Kim SCL Area Manager SNS/ORNL

25 Managed by UT-Battellefor the U.S. Department of Energy

Linac 08, Victoria Canada

Gradient Limitations from “Collective Effects”

a b c d

Beam pipe Temperature

individual limits; 19.5, 15, 17, 14.5 MV/m collective limits; 14.5, 15, 15, 10.5 MV/m

Flange T

Coupler or Outer T

• Electrons from Field Emission and Multipacting– Steady state electron activity and sudden bursts

affects other cavities

• Leads to gas activity and heating with subsequent end-group quench and/or reaches intermediate temperature region (5-20k); H2 evaporation and redistribution of gas which changes cavity and coupler conditions

• Example for CM13:

• Electron impact location depends on relative phase and amplitude of adjacent cavities

Page 26: The Status of the SNS 3 rd SPL Collaboration Meeting CERN Nov. 11-13, 2009 Sang-ho Kim SCL Area Manager SNS/ORNL

26 Managed by UT-Battellefor the U.S. Department of Energy

Performance degradation• First time in 4-years operation + commissioning• Limiting gradient of 5a; 14.5 MV/m due to FE Partial quench at 9 MV/m• Beam between MPS trigger and beam truncation off-energy beam much

bigger beam loss at further down-stream gas burst redistribution of gas/particulate changes in performance/condition

• Random, statistical events; made HOM coupler around FPC worse• As beam power goes higher, things could be worse re-verification of MPS is

ongoing

Partial quench

Cavity fieldForward power

Page 27: The Status of the SNS 3 rd SPL Collaboration Meeting CERN Nov. 11-13, 2009 Sang-ho Kim SCL Area Manager SNS/ORNL

27 Managed by UT-Battellefor the U.S. Department of Energy

• Repaired ~10 cryomodules to regain operation of 80 out of 81 cavities– CM19 removed: had one inoperable cavity (excessive power

through HOM); removed both HOM feedthroughs – CM12 removed: removed 4 HOM feedthroughs on 2 cavities– Tuner repairs performed on ~7 CMs– We have warmed up, individually, ~10 CMs in the past 4 years– Individual cryomodules may be warmed up and accessed due to

cryogenic feed via transfer line.

• Installed an additional modulator and re-worked klystron topology in order to provide higher klystron voltage (for beam loading and faster cavity filling)

• Further increases in beam energy require increasing the installed cavity gradients to design values

Increasing the Beam Energy

Page 28: The Status of the SNS 3 rd SPL Collaboration Meeting CERN Nov. 11-13, 2009 Sang-ho Kim SCL Area Manager SNS/ORNL

28 Managed by UT-Battellefor the U.S. Department of Energy

SCL energy

• Limiting factors; mainly field emission

• 80 out of 81 cavities; 930 MeV +10 MeV

0

2

4

6

8

10

12

14

16

18

1a 1c

2b

3a 3c

4b

5a 5c

6b

7a 7c

8b

9a 9c

10

b

11

a

11

c

12

b

12

d

13

b

13

d

14

b

14

d

15

b

15

d

16

b

16

d

17

b

17

d

18

b

18

d

19

b

19

d

20

b

20

d

21

b

21

d

22

b

22

d

23

b

23

d

Cavity number

Ea

cc

(M

V/m

)

Aug_09 Nov_08

28

HOMB

Additional HVCM; enough RF power for design currentH01 repaired and put in the slot of CM19

0 10 20 30 40 50 60

Electron loading (EG heating, gas

burst, quench)

Coupler Heating

HOM

Quench (cell)

Lorentz forcedetuning

No limits up to 22MV/m

No. of cavities

One does not reach steady state mechanicalvibration

1 cavity is disabledCM19 removed and repaired

CM12 removed and found vacuum leaks at 3 HOM feedthroughs (fixed)

Page 29: The Status of the SNS 3 rd SPL Collaboration Meeting CERN Nov. 11-13, 2009 Sang-ho Kim SCL Area Manager SNS/ORNL

29 Managed by UT-Battellefor the U.S. Department of Energy

• A program is underway to develop and apply plasma cleaning methods to installed accelerator RF components

Plasma Processing Development

29

0.01

0.10

1.00

10.00

100.00

0 2 4 6 8 10 12

Eacc (MV/m)

Do

se

Ra

te (

BL

M7

)

baseline before processing

after processing

– If successful this should significantly reduce field emission, mulitpacting and increase operating stability of RF structures

• First test on SNS cavity allows 2 MV/m increase for same radiation levels

• Experimental Program Includes

– Witness samples from standard processes

– TM020 test cavity – And full RF structures (3-cell

test cavity) for procedure development

Page 30: The Status of the SNS 3 rd SPL Collaboration Meeting CERN Nov. 11-13, 2009 Sang-ho Kim SCL Area Manager SNS/ORNL

30 Managed by UT-Battellefor the U.S. Department of Energy

AP_Talk Feb. 19, 2009

Ionization ChamberInternal Ionization ChamberPhosphor Screen, Camera, Faraday Cup

IC0

IC1

IC2IC3 IC4 IC5 IC6

IC7

IC-int

Phosphor Screen& Faraday Cup

Phosphor Screen& Faraday Cup

Cavity ACavity BCavity CCavity D

Cavity D 12 MV/mCamera exposure; 30 ms

Cavity A 9.3MV/mCamera exposure; 30 ms

Radiation/electron activity diagnostics in the Test Cave

Page 31: The Status of the SNS 3 rd SPL Collaboration Meeting CERN Nov. 11-13, 2009 Sang-ho Kim SCL Area Manager SNS/ORNL

31 Managed by UT-Battellefor the U.S. Department of Energy

Test Cavity

Witness Sample for Chemistry

Demountable witness plate

SRF cavityFPC Flange

Surface analysis

Microwave Plasma processor

150.00

3.3 GHz, TM020 modeEp/Bp=1.12 (MV/m)/mTEx. Ep=50 MV/m, Bp=56 mTPdiss=36 W at 4.2 K

150 mm

-Cold testw/ dual mode (CW or pulse) -Plasma processing

FPC Flange

3–cell cavity For R&D

Page 32: The Status of the SNS 3 rd SPL Collaboration Meeting CERN Nov. 11-13, 2009 Sang-ho Kim SCL Area Manager SNS/ORNL

32 Managed by UT-Battellefor the U.S. Department of Energy

AFF & Beam ramp-up• When beam current is bigger than ~18 mA average

– field regulations go beyond the threshold RF truncation AFF can not learn

– BLM trips AFF can not learn• Klystron power is usually those at saturation

– Non-linear• We use PW (chopping pattern; ratio between midi-pulse and gap)

– Starting around <18 mA Ib,avg after AFF learned increase Ib,avg

At beginning

Cavity Field

forward

reflected

Forward/reflected are in voltage unit

At start

21b

0

100

200

300

400

500

600

0.0E+00 2.0E+08 4.0E+08 6.0E+08 8.0E+08 1.0E+09 1.2E+09

FCM output^2

Kly

stro

n f

orw

ard

po

wer

HP

M r

ead

ing

(kW

)

KlyF 71kV

KlyF 73kV

KlyF 75kV

Overall gain measurement(from FCM digital output to Klystron forward power)

Page 33: The Status of the SNS 3 rd SPL Collaboration Meeting CERN Nov. 11-13, 2009 Sang-ho Kim SCL Area Manager SNS/ORNL

33 Managed by UT-Battellefor the U.S. Department of Energy

• As an urgent matter, we are constructing two spare high-beta cryomodules– These will be 10CRF851-compliant; vacuum vessel envelope was redesigned

for pressure vessel compatibility

– Cavities are currently being qualified at Jefferson Lab (1st string qualified)

– Plan is to construct/integrate these spare CMs in-house

• The SNS Power Upgrade Project (PUP) has CD-1 approval, and includes the following scope:– 9 additional high-beta CMs to increase energy to 1.3 GeV

– Associated RF systems

– Ring modifications to support higher energy

• We expect to involve industry in PUP CM construction (expect CD-2 approval in the next FY)

• We are continuing to build SRF support facilities to provide basic repair and testing capabilities in support of long-term maintenance and the Upgrade

Ongoing and Future Activities

Page 34: The Status of the SNS 3 rd SPL Collaboration Meeting CERN Nov. 11-13, 2009 Sang-ho Kim SCL Area Manager SNS/ORNL

34 Managed by UT-Battellefor the U.S. Department of Energy

34

Bayonets remain in original positions

“Code” Bolted FlangesJ-T’s repositioned

Power Upgrade Cryomodule Design

Page 35: The Status of the SNS 3 rd SPL Collaboration Meeting CERN Nov. 11-13, 2009 Sang-ho Kim SCL Area Manager SNS/ORNL

35 Managed by UT-Battellefor the U.S. Department of Energy

• In place– Cryomodule test-

cave tied-in to CHL

– High-power RF test-stand

– Cleanroom facility

– Ultrapure Water• High pressure rinse

system in fabrication• Vertical Test Area

design complete; construction starting

• Dedicated Cryogenic Support refrigerator in design

SRF Maintenance and Test Facility

Class 100Class 10,000

CryomoduleAssembly

RF/Couplerprocessing

Test Cave

ChemistryVTA

Class 10

CryomoduleAssembly

Mezzanine(lab space)

HPR

Page 36: The Status of the SNS 3 rd SPL Collaboration Meeting CERN Nov. 11-13, 2009 Sang-ho Kim SCL Area Manager SNS/ORNL

36 Managed by UT-Battellefor the U.S. Department of Energy

Power Upgrade Project (PUP)+ Accelerator Improvement Project (AIP)

Parameter SNS Baseline Power upgrade

Kinetic energy [MeV] 1000 1300

Beam power [MW] 1.4 3.0

Chopper beam-on duty factor [%] 68 70

Linac beam macropulse duty factor [%] 6.0 6.0

Average macropulse H- current, [mA] 26 42

Peak macropulse H- current, [mA] 38 59

Linac average beam current [mA] 1.6 2.5

SRF cryo-module number (medium-beta) 11 11

SRF cryo-module number (high-beta) 12 12+8 (+1 reserve)

SRF cavity number 33+48 33+80 (+4 reserve)

Peak surface gradient (b=0.61 cavity) [MV/m] 27.5 (+/- 2.5) 27.5 (+/- 2.5)

Peak surface gradient (b=0.81 cavity) [MV/m] 35 (+2.5/-7.5) 31

Ring injection time [ms] / turns 1.0 / 1060 1.0 / 1100

Ring rf frequency [MHz] 1.058 1.098

Ring bunch intensity [1014] 1.6 2.5

Ring space-charge tune spread, DQsc0.15 0.15

Pulse length on target [ns] 695 691

Page 37: The Status of the SNS 3 rd SPL Collaboration Meeting CERN Nov. 11-13, 2009 Sang-ho Kim SCL Area Manager SNS/ORNL

37 Managed by UT-Battellefor the U.S. Department of Energy

Concerns• Balancing (rf power, gradient, coupler average power)

– 42 mA average current (59 mA peak)

– Existing RF system; 550 kW (at saturation) per cavity

– Existing HVCM; 75 kV, 10 pack configuration

– Existing FPC; ~50 kW average power• No active cooling for inner conductor at vacuum side• Thermal radiation load to end group ~3W

• Optimization works are in progress– Based on what we learned from operational experiences

– Minimize reworks of existing cryomodules

– Multiple approaches for margin (remove the weakest links)

• Changes– Vacuum vessel, FPC (Qex, Higher average power), HOMless, Coupler

cooling configuration, etc.

Page 38: The Status of the SNS 3 rd SPL Collaboration Meeting CERN Nov. 11-13, 2009 Sang-ho Kim SCL Area Manager SNS/ORNL

38 Managed by UT-Battellefor the U.S. Department of Energy

PUP impact on SCL

• Baseline number; 10.1 MV/m (MB), 14.1 MV/m (HB)• Need reworks for the most of existing HB cryomodules;

power coupler (average power) + HP RF + Modulator

0

2

4

6

8

10

12

14

16

0

100

200

300

400

500

600

700

800

0 20 40 60 80 100 120

Eacc

(MV/

m)

RF P

ower

in st

eady

stat

e (k

W)

Cavity Number

Eacc

RF power at the coupler in steady state

Klystron powerAt saturation

Control marginError budget

PUP cavities

Page 39: The Status of the SNS 3 rd SPL Collaboration Meeting CERN Nov. 11-13, 2009 Sang-ho Kim SCL Area Manager SNS/ORNL

39 Managed by UT-Battellefor the U.S. Department of Energy

Option I (based on existing cavity performances)• No reworks for the existing cryomodules + HPRF system +HVCM• New PUP cryomodules

– Cavity radiation threshold >15 MV/m, Coupler>70kW average power (end group heating issues due to thermal radiation)

– 750 kW klystrons + 82 kV HVCM

0

2

4

6

8

10

12

14

16

18

0

100

200

300

400

500

600

700

800

0 20 40 60 80 100 120

Eacc

(MV/

m)

RF P

ower

in st

eady

stat

e (k

W)

Cavity Number

Eacc

RF power at the coupler in steady state

Klystron powerAt saturation

Control marginError budget

PUP cavities

Page 40: The Status of the SNS 3 rd SPL Collaboration Meeting CERN Nov. 11-13, 2009 Sang-ho Kim SCL Area Manager SNS/ORNL

40 Managed by UT-Battellefor the U.S. Department of Energy

Option II • Some reworks for existing system (no rework for the couplers)

– A few kV higher for HVCM For last several CMs

– Some performance improvement; plasma processing

• About same loading on PUP cavities (14.3 MV/m, 700kW RF at saturation)

0

2

4

6

8

10

12

14

16

18

0

100

200

300

400

500

600

700

800

0 20 40 60 80 100 120

Ea

cc

(MV

/m)

RF

Po

we

r in

ste

ad

y s

tate

(k

W)

Cavity Number

Eacc

RF power at the coupler in steady state

Klystron powerAt saturation

Control marginError budget

PUP cavities

Page 41: The Status of the SNS 3 rd SPL Collaboration Meeting CERN Nov. 11-13, 2009 Sang-ho Kim SCL Area Manager SNS/ORNL

41 Managed by UT-Battellefor the U.S. Department of Energy

Summary• 3-yrs operation

– Reached 1 MW operation– Availability is improving– Beam loss seems not a show stopper in SNS

• Technical issues and status– RFQ; Better understanding, very stable operation– HVCM; better in this op. period.

Operational stability needs to be improved– Foil; New batch of foils/brackets, so far no failure

Need more understanding of failure mechanism

– SCL; Tight control, very stable operationPlasma processing R&D to get 1 GeV

• PUP; technical design in this FY.