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HOM Experiences at the SNS SCL. SPL HOM Workshop CERN June 26, 2009 Sang-ho Kim SNS SCL Area Manager SNS/ORNL. Outline. SNS Intro HOM concerns in SNS SRF cavity Reminder of past histories HOM coupler issue Re-evaluation HOM frequency statistics SNS beam Beam induced signal - PowerPoint PPT Presentation
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HOM Experiences at the SNS SCL
SPL HOM WorkshopCERN
June 26, 2009
Sang-ho Kim
SNS SCL Area Manager
SNS/ORNL
2 Managed by UT-Battellefor the U.S. Department of Energy SPL HOM Workshop at CERN, June 25-26, 2009
Outline
SNS Intro
HOM concerns in SNS SRF cavity Reminder of past histories
HOM coupler issue
Re-evaluation HOM frequency statistics SNS beam Beam induced signal
Summary
3 Managed by UT-Battellefor the U.S. Department of Energy SPL HOM Workshop at CERN, June 25-26, 2009
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
HEBT
Injection Extraction
RF
Collimators
Liquid Hg Target
4 Managed by UT-Battellefor the U.S. Department of Energy SPL HOM Workshop at CERN, June 25-26, 2009
SNS SRF cavity
Fundamental Power Coupler
HOM CouplerHOMB
HOM CouplerHOMA
Field Probe
Tuner
Helium Vessel
Major Specifications:Ea=15.9 MV/m at =0.81
Ea=10.2 MV/m at =0.61
&Qo> 5E9 at 2.1 K
5 Managed by UT-Battellefor the U.S. Department of Energy SPL HOM Workshop at CERN, June 25-26, 2009
Designed to operate at 2.1 K (superfluid helium)
Fundamental power couplers
Return end can
Helium vessels
Space frame
Supply end can
SNS Cryomodule
11*Medium beta
12*High beta
81 cavities
6 Managed by UT-Battellefor the U.S. Department of Energy SPL HOM Workshop at CERN, June 25-26, 2009
Beam power history
Summer 2007
Winter 2007
Summer 2008
Spring 2007Fall 2006
Winter 2008
Summer2009
7 Managed by UT-Battellefor the U.S. Department of Energy SPL HOM Workshop at CERN, June 25-26, 2009
Parameters DesignIndividually
achieved
Highest production
beam
Beam Energy (GeV) 1.0 1.01 0.93
Peak Beam current (mA) 38 40 38
Average Beam Current (mA) 26 24 24
Beam Pulse Length (s) 1000 1000 670
Repetition Rate (Hz) 60 60 60
Beam Power on Target (kW) 1440 880 880
Linac Beam Duty Factor (%) 6.0 4.0 4.0
Beam intensity on Target (protons per pulse) 1.5 x 1014 1.3 x 1014 1.0 x 1014
SCL Cavities in Service 81 80 80
Major Parameters achieved vs. designed
8 Managed by UT-Battellefor the U.S. Department of Energy SPL HOM Workshop at CERN, June 25-26, 2009
SCL status SCL is providing a very reliable operation for neutron
production following SNS power ramp-up Down time < 5 min/day (<1 trip/day)
930 MeV + 10 MeV (energy reserve)
In-situ plasma processing Initial attempt showed very promising results R&D plan for 1 year
0
2
4
6
8
10
12
14
16
18
1a 2b 3c 5a 6b 7c 9a 10b 11c 12d 13d 14d 15d 16d 17d 18d 19d 20d 21d 22d 23d
Cavity number
Ea
cc
(M
V/m
)
9 Managed by UT-Battellefor the U.S. Department of Energy SPL HOM Workshop at CERN, June 25-26, 2009
At the Design Phase
10 Managed by UT-Battellefor the U.S. Department of Energy SPL HOM Workshop at CERN, June 25-26, 2009
SNS Beam Time-Structure
Macro-pulses
Midi-pulses
Micro-pulsesTb=2.4845 ns (1/402.5MHz)
N=260 micropulses
Tib=645 ns Tg=300 ns
Ti=945 ns (1/1.059 MHz)
M=1,060 mid-pulses
Tmb=1msTG=15.7ms
Tm=16.7ms (1/60Hz)
6e8 particle/micropulse95 pC/micropulse
38mA
26mA
1.56 mA
11 Managed by UT-Battellefor the U.S. Department of Energy SPL HOM Workshop at CERN, June 25-26, 2009
HOM analysis for SNS
Cavity Design Finding HOM’s for the reference
geometry (R/Q, f…)
Linac beam dynamics
Ring Injection;foil, beam loss, &
activation
Finding HOM’sincluding the effects
of manufacturing imperfection
BBU for each HOM’s assuming Q
Compare resultsallowable ?
Q threshold
Qex estimation & design basis for HOM coupler
Pre-estimation of heat load as a function of Qext & Qo
YesNoReduce
Q
f measurement of non-SNS cavity Q threshold
12 Managed by UT-Battellefor the U.S. Department of Energy SPL HOM Workshop at CERN, June 25-26, 2009
HOM findings (I)
Monopoles, dipoles, quadrupoles, sextupoles Up to cutoff frequencies of pipes (~3 GHz) Single cavity, Superstructure r/Q’s of all modes as a function of particle velocity
Mechanical imperfection Random geometrical error based on manufacturing
experiences Possibility of having trapped modes
13 Managed by UT-Battellefor the U.S. Department of Energy SPL HOM Workshop at CERN, June 25-26, 2009
HOM findings (II)
0
0.2
0.4
0.6
0.8
1
1.2
-2 -1 0 1 2 3 4 5 6 7
500 mm beam pipe +400 mm conical ends 500 mm beam pipe +
400 mm conical endsStainless Steel Bellows (91 mm)
; FPC sides
0
0.2
0.4
0.6
0.8
1
1.2
-0.8 -0.6 -0.4 -0.2 0 0.2 0.4 0.6 0.8
14 Managed by UT-Battellefor the U.S. Department of Energy SPL HOM Workshop at CERN, June 25-26, 2009
E_2 0 mm
9.00E-01
9.20E-01
9.40E-01
9.60E-01
9.80E-01
1.00E+00
0.00E+00 5.00E-03 1.00E-02 1.50E-02 2.00E-02 2.50E-02
r (m)
n
HOM findings (medium)
1.E-04
1.E-03
1.E-02
1.E-01
1.E+00
1.E+01
1.E+02
1.E+03
0.5 1.0 1.5 2.0 2.5 3.0 3.5frequency (GHz)
Maximu
m R/Q (
Ohm)
1.E-06
1.E-03
1.E+00
1.E+03
1.0 1.2 1.4 1.6 1.8 2.0 2.2 2.4 2.6 2.8 3.0
frequency (GHz)
Maximu
m R/Q (
Ohm/cm
4)
1.80E+00
1.85E+00
1.90E+00
1.95E+00
2.00E+00
2.05E+00
0.00E+00 5.00E-03 1.00E-02 1.50E-02 2.00E-02
r (m )n
n vs. r; radial gradient of the axial electric field (Ezrn)
dipole
quadrupole
1.E-03
1.E-02
1.E-01
1.E+00
0.55 0.57 0.59 0.61 0.63 0.65 0.67 0.69
Beta
R/Q
(o
hm
)
mode 29 mode 30mode 31 mode 32mode 33 mode 34mode 35 mode 36
r/Q vs.
1
1
1
1
15 Managed by UT-Battellefor the U.S. Department of Energy SPL HOM Workshop at CERN, June 25-26, 2009
HOM findings (high)
1.E-04
1.E-03
1.E-02
1.E-01
1.E+00
1.E+01
0.7 0.75 0.8 0.85 0.9beta
R/Q
(O
hm
)
mode 31 mode 32
mode 33 mode 34
mode 35 mode 36
r/Q vs.
1.E-02
1.E-01
1.E+00
1.E+01
1.E+02
1.E+03
0.5 1.0 1.5 2.0 2.5 3.0 3.5Frequency (GHz)
Maxim
um R/Q
(Ohm
)
1.E-03
1.E-02
1.E-01
1.E+00
1.E+01
1.E+02
1.E+03
1.0 1.2 1.4 1.6 1.8 2.0 2.2 2.4 2.6 2.8 3.0Frequency (GHz)
Maxim
um R/Q
(Ohm
/cm2
)
1
1
1
1
16 Managed by UT-Battellefor the U.S. Department of Energy SPL HOM Workshop at CERN, June 25-26, 2009
Geometrical imperfection (for any possible trapped mode)
0Ls
s
0Ls
s
200
1
))/sin()/cos((i
sisi LsibLsia
0 . 2 0 . 4 0 . 6 0 . 8 1
- 2 0
- 1 0
1 0
2 0
Ls
1
-1
0 . 2 0 . 4 0 . 6 0 . 8 1
- 2 0
- 1 0
1 0
2 0
Ls
1
-1
Deviations from the reference geometry
; normal to the surfaceLs; total length along the cavity surface, ~1.9 m for high beta cavityai & bi; random coefficient
An example of the random mechanical perturbation.
0.130
0.135
0.140
0.145
0.150
0.155
0.160
0.165
0.170
0.080 0.090 0.100 0.110 0.120
z (m)
r (m
)
ref. shape ref. Geometry (MAFIA) P1 (MAFIA)
Trapped mode is unlikely up to quadrupole modes
17 Managed by UT-Battellefor the U.S. Department of Energy SPL HOM Workshop at CERN, June 25-26, 2009
Properties of HOM frequency (R. Sundelin’s study at Cornell) HOM frequency Centroid Error between analysis & real
ones Fractional error; (fanalysis-freal,avg)/fanalysis< 0.0038 SNS used 0.8 % (for conservative analysis)
put frequency centroid on the highest spectral line in the range
HOM frequency spread
fo; fundamental frequency, fn; HOM frequency For beam dynamics 20 % of this value were used for
conservative analysis
Non-pi fundamental mode
000109.0 ff n
027.0mod
mod
calculatede
e
calculated
calculatedmeasured
ff
f
f
ff
, 0.0675 was used for analysis
18 Managed by UT-Battellefor the U.S. Department of Energy SPL HOM Workshop at CERN, June 25-26, 2009
Bunch Tracking (I)JLab; R. Sundelin, L. Merminga, G. Krafft, B. Yunn, J. Delayan SNS; D. Jeon, J. Wei, M. Doleans, S. Kim Transverse
Cumulative effects True instability; can occur at almost any frequency
No transverse instabilities for Q<108 (20% of for f spread) Error magnification; worst when an HOM frequency
differs by of the order of 1 cavity bandwidth from a beam spectral lines Error magnification~10.00062 (0.8 % centroid error)
Longitudinal Instability
Bunch energy error, bunch-to-bunch variation Can occur at almost any frequency Non-pi fundamental passband can excite oscillations
No instability & significant of energy error at Q<108
19 Managed by UT-Battellefor the U.S. Department of Energy SPL HOM Workshop at CERN, June 25-26, 2009
Bunch Tracking (II) Bunch output energy errorWith artificially high r/Q for 5/6 mode
All quads are turned off for benchmarkingBeam injection; 1 mm off axis
HOM centroids; switched to the most dangerous placeBeam current; 50 mA, 1 mm off-axis injectionHOM’s Q=108
20 Managed by UT-Battellefor the U.S. Department of Energy SPL HOM Workshop at CERN, June 25-26, 2009
HOM induced power
Individual cavity issue
Function of HOM f, r/Q, Q
Same logic is applied for centroid
Both analytic & numeric calculation
Find the possible peak HOM induced power
21 Managed by UT-Battellefor the U.S. Department of Energy SPL HOM Workshop at CERN, June 25-26, 2009
Beam induced HOM Power (I)
1.E-091.E-081.E-071.E-061.E-051.E-041.E-031.E-021.E-01
1.E+001.E+011.E+02
2.8075E+09 2.8115E+09 2.8155E+09 2.8195E+09 2.8235E+09 2.8275E+09f (Hz)
402.5 MHz micro-bunch resonance1.059 MHz (1/945 ns) midi-pulseresonance
1.55 MHz (1/645 ns) midi-pulsewithout gap anti-resonance
Qex=106
f (Hz)
Tim
e A
vera
ged
HO
M
Po
wer
/(r/
Q),
[W
/Oh
m)
100
1
0.01
In continuous frequency domain
1.E-02
1.E-01
1.E+00
1.E+01
1.E+02
1.E+03
1.E+04
1.E+05
1.E+01 1.E+04 1.E+07 1.E+10
Qex
Tim
e A
ve
ra
ge
d H
OM
Po
we
r/(
R/Q
) a
t 2
.81
75
GH
z
(m
icro
-p
uls
e r
es
on
an
ce
),
[W
/Oh
m]
Micro-pulse
Midi-pulse
Macro-pulseexQQr
tVtP
2)()(
Tt
tavg dttPT
P1
1)(
1
HOM Power
Time AveragedHOM Power
22 Managed by UT-Battellefor the U.S. Department of Energy SPL HOM Workshop at CERN, June 25-26, 2009
Beam induced HOM Power (II)
1.E-01
1.E+00
1.E+01
1.E+02
1.E+03
1.E+04
2.817499E+09 2.817500E+09 2.817501E+09
f (Hz)
Tim
e A
vera
ged
HO
M P
ow
er/(R
/Q),
[W/O
hm
]
23 Managed by UT-Battellefor the U.S. Department of Energy SPL HOM Workshop at CERN, June 25-26, 2009
Dangerous Modes at around main spectral lines within the centroid error range (Medium beta cavity)
0
0.2
0.4
0.6
0.8
1
1.2
-0.6 -0.4 -0.2 0 0.2 0.4 0.6
0
0.1
0.2
0.3
0.4
0.5
0.6
-3 -2 -1 0 1 2 3
0
0.2
0.4
0.6
0.8
1
1.2
-3 -2 -1 0 1 2 3
1.E-03
1.E-02
1.E-01
1.E+00
0.55 0.57 0.59 0.61 0.63 0.65 0.67 0.69
Beta
R/Q
(o
hm
)
mode 29 mode 30mode 31 mode 32mode 33 mode 34mode 35 mode 36
Mode f (Hz) Qo (due to SS Bellows)
31-1 2.800995E+09 1.5660E+07
31-2 2.800834E+09 1.6235E+07
31-3 2.800863E+09 1.5158E+07
32-1 2.820670E+09 1.9979E+07
32-2 2.820575E+09 1.8349E+07
32-3 2.820466E+09 1.9049E+07
36-1 3.230296E+09 3.5576E+04
24 Managed by UT-Battellefor the U.S. Department of Energy SPL HOM Workshop at CERN, June 25-26, 2009
Dangerous Modes at around main spectral lines within the Centroid Error range (High beta cavity)
0
0.2
0.4
0.6
0.8
1
1.2
-0.8 -0.6 -0.4 -0.2 0 0.2 0.4 0.6 0.8
0
0.2
0.4
0.6
0.8
1
1.2
-0.8 -0.6 -0.4 -0.2 0 0.2 0.4 0.6 0.81.E-04
1.E-03
1.E-02
1.E-01
1.E+00
0.7 0.75 0.8 0.85 0.9beta
R/Q
(O
hm
)
mode 25 mode 26
mode 27 mode 28
mode 29 mode 30
1.E-04
1.E-03
1.E-02
1.E-01
1.E+00
1.E+01
0.7 0.75 0.8 0.85 0.9beta
R/Q
(O
hm
)
mode 31 mode 32
mode 33 mode 34
mode 35 mode 36
Modes f (Hz) Qo (due to SS Bellows)
25-1 2.41389E+09 < 2.0E+6 (FPC)
25-2 2.41406E+09 < 2.0E+6 (FPC)
25-3 2.41394E+09 < 2.0E+6 (FPC)
25-4 2.41327E+09 < 2.0E+6 (FPC)
35-1 2.81540E+09 7.942E+06
35-2 2.81576E+09 4.206E+06
35-3 2.81555E+09 4.314E+06
35-4 2.81556E+09 2.772E+06
36-1 2.83064E+09 5.508E+06
36-2 2.83046E+09 2.655E+06
36-3 2.83016E+09 2.086E+06
36-4 2.83008E+09 2.224E+06
25 Managed by UT-Battellefor the U.S. Department of Energy SPL HOM Workshop at CERN, June 25-26, 2009
Maximum HOM power of each mode in the Centroid Error range for Maximum r/Q
1.E-08
1.E-07
1.E-06
1.E-05
1.E-04
1.E-03
1.E-02
1.E-01
1.E+00
1.E+01
1.E+02
5 10 15 20 25 30 35 40
mode number
Tim
e A
ve
rag
ed
HO
M P
ow
er
pe
r
Ca
vit
y f
or
the
ma
x R
/Q [
W]
Qex=10^3 Qex=10^4Qex=10^5 Qex=10^6Qex=10^7 Qex=10^8
1.E-07
1.E-06
1.E-05
1.E-04
1.E-03
1.E-02
1.E-01
1.E+00
1.E+01
1.E+02
1.E+03
5 10 15 20 25 30 35 40
mode number
Tim
e A
vera
ged
HO
M P
ow
er p
er
Cav
ity fo
r th
e m
ax R
/Q [W
]
Qex=10 3̂ Qex=10 4̂Qex=10 5̂ Qex=10 6̂Qex=10 7̂ Qex=10 8̂
Beam pipe mode;~ out of concern
FPC coupling;Less concern
Damping requirement; Medium beta cavity 10^6 High beta cavity 10^5
26 Managed by UT-Battellefor the U.S. Department of Energy SPL HOM Workshop at CERN, June 25-26, 2009
The decision for SNS HOM
No Beam dynamics issue
Centroid error, f spread & location of cavities; in question
When Q>105, 106, there’s a concern. HOM power ~ fundamental power dissipation but the probability is very low even under the conservative
assumptions
Extra insurance SNS is the first pulsed proton SC linac Any issues were treated in a very conservative way
Ex. Piezo tuner; we’ve never used them
27 Managed by UT-Battellefor the U.S. Department of Energy SPL HOM Workshop at CERN, June 25-26, 2009
SNS HOM Coupler
28 Managed by UT-Battellefor the U.S. Department of Energy SPL HOM Workshop at CERN, June 25-26, 2009
SNS HOM Coupler
Coaxial type notch filter scaled from TTF was chosen
end-cell
HOM can
HOM antenna
HOMFeedthrough
gap
-100
-90
-80
-70
-60
-50
-40
-30
-20
-10
0
300 800 1300 1800 2300 2800 3300 3800
Frequency [MHz]
S12
[d
B]
29 Managed by UT-Battellefor the U.S. Department of Energy SPL HOM Workshop at CERN, June 25-26, 2009
HOM coupler development
Identification of all HOM modes; very good agreement
Low power tests confirmed its functionality (JLab) Damping; dangerous modes to have Q<~10^5
0
0.2
0.4
0.6
0.8
1
1.2
-0.6 -0.4 -0.2 0 0.2 0.4 0.6
z [m]
E2
-0.3
0.7
1.7
2.7
3.7
4.7
5.7
0.0 5.0 10.0 15.0 20.0 25.0 30.0
Time [s]
Ph
ase
[de
g]
Without FPC f=2812.366 MHz With FPC (5mm penetration) f=2812.131 MHz
FPC side
calculation
30 Managed by UT-Battellefor the U.S. Department of Energy SPL HOM Workshop at CERN, June 25-26, 2009
Fundamental mode thru HOM coupler
Normal waveform of fundamental mode from HOM ports (y-axis; log scale)
HOMA
HOMB
Fundamental mode couplingHigh 1010~ 1012
< a few W during pulse
31 Managed by UT-Battellefor the U.S. Department of Energy SPL HOM Workshop at CERN, June 25-26, 2009
Abnormal HOM coupler signals (RF only, no beam)
1~5 Hz 10 Hz 30 Hz
~’0’ coupling and rep. rate dependent signals
Electron activities (MP & discharge; observations under close attention)
32 Managed by UT-Battellefor the U.S. Department of Energy SPL HOM Workshop at CERN, June 25-26, 2009
Problems (II)
33 Managed by UT-Battellefor the U.S. Department of Energy SPL HOM Workshop at CERN, June 25-26, 2009
Problems while running RF onlyAny electron activity (multipacting, burst of field emitter, etc)Destroy standing wave pattern (or notching characteristics)Large fundamental power couplingFeedthrough/transmission line damage (most of attenuators were blown up)Irreversible
Electric Field
Magnetic field
Gonin, N. Solyak
34 Managed by UT-Battellefor the U.S. Department of Energy SPL HOM Workshop at CERN, June 25-26, 2009
Turn-on and High power commissioning First turn on must be closely watched and controlled
(possible irreversible damage) Initial (the first) powering-up, pushing limits, increasing rep.
rate (extreme care, close attention) Aggressive MP, burst of FE possibly damage weak
components Similar situation after thermal cycle (and after long shut down
too) behavior of the same cavity can be considerably different from run to run
Subsequent turn-ons (after long shut-down) also need close attention: behavior of the same cavity can be considerably different from run to run gas re-distribution
Cryomodules/strings must be removed and rebuilt if vented/damaged
35 Managed by UT-Battellefor the U.S. Department of Energy SPL HOM Workshop at CERN, June 25-26, 2009
Large fundamental mode coupling 11b; repaired at JLab but non-operable from the beginning, no
notch 19b; March 06 turned off (10 W coupling at 1 MW/m) 3 cavities; operable but limited by HOM power
Not related with damage, just worse location of notching freq.
6 cavities; abnormal waveforms about ‘0’ coupling Seems to be a (partial) disconnection in feedthrough/cable in CM May have leak
beam line vacuum leak CM12
Largest field emission Feedthrough damaged?
Limited by Fundamental mode in HOM coupler
36 Managed by UT-Battellefor the U.S. Department of Energy SPL HOM Workshop at CERN, June 25-26, 2009
Re-evaluation
37 Managed by UT-Battellefor the U.S. Department of Energy SPL HOM Workshop at CERN, June 25-26, 2009
Re-evaluation of necessities for HOM couplers
Same arguments on BBU and instability Stainless steel bellows and fundamental power
coupler Q < 108
What is the possibility that one can have high HOM induced power? HOM verifications
HOM statistics
Beam induced signal
38 Managed by UT-Battellefor the U.S. Department of Energy SPL HOM Workshop at CERN, June 25-26, 2009
HOM frequency measurementat 4.4 K (between HOMA & HOMB)
Frequency measurement of the dangerous modes for all cavities in the linac tunnel
Medium beta cavity High beta cavityassumption for analysisMode 31 32 25 35 36
Average (GHz) 2.81197 2.83017 2.41587 2.81383 2.83018
Sigma (MHz) 3.19626 3.33151 1.54211 2.09127 2.71721
Analysis (GHz) 2.80100 2.82050 2.41400 2.81550 2.83030
sigma/(fn-fo) 0.00159 0.00165 0.00096 0.00104 0.00134 0.00022
fractional centroid error -0.00392 -0.00343 -0.00077 0.00059 0.00004 0.008
In addition, to have an estimation of HOM frequency shift at 2K, tests have been done for some high beta cavities by changing tuner position (~60 kHz)Frequency changes less than ~400 kHz
Out of concern2.8175 GHz
Out of concern2.8175 GHz
39 Managed by UT-Battellefor the U.S. Department of Energy SPL HOM Workshop at CERN, June 25-26, 2009
Zoom-in
1.E-06
1.E-05
1.E-04
1.E-03
1.E-02
1.E-01
1.E+00
1.E+01
1.E+02
1.E+03
1.E+04
2.815 2.8155 2.816 2.8165 2.817 2.8175 2.818 2.8185 2.819 2.8195 2.82f (GHz)
Pow
er/
(r/Q
) (W
/Ohm
)
Peak valueat the end of pulse
Time averaged
The Q’s of modes are less than about ~107 due to the damping on the SS bellows, there’s no macro-pulse resonance.Peak value is more meaningful.
In following pages frequency distributions are plotted on the peak power spectral lines.Beam current (38 mA peak) in the following examples
40 Managed by UT-Battellefor the U.S. Department of Energy SPL HOM Workshop at CERN, June 25-26, 2009
1.E-06
1.E-05
1.E-04
1.E-03
1.E-02
1.E-01
1.E+00
1.E+01
1.E+02
2.8150 2.8155 2.8160 2.8165 2.8170 2.8175 2.8180 2.8185 2.8190 2.8195 2.8200f (GHz)
Peak
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Zoom-in (Mode 31 Medium beta)
Peak power at maximum r/Q (~0.3 Ohm)
Only 5 cavities have mode 31 in +/-2.5 MHz from main spectral line (2.8175 GHz).(Mode 25 of other 28 cavities are below 2.815 GHz) out of concern.Q’s <~10^7 (with HOM couplers 10^4)Only main spectral line will be a concern.Presently all HOM’s are far away from the dangerous beam spectral line.
Red dots just show the frequency locations
10^7
10^6
10^5
41 Managed by UT-Battellefor the U.S. Department of Energy SPL HOM Workshop at CERN, June 25-26, 2009
Zoom-in (Mode 25 High beta)
1.E-06
1.E-05
1.E-04
1.E-03
1.E-02
1.E-01
1.E+00
1.E+01
1.E+02
1.E+03
2.4110 2.4120 2.4130 2.4140 2.4150 2.4160 2.4170 2.4180 2.4190f (GHz)
Peak
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Peak power at maximum r/Q (~0.35 Ohm)
All Mode 25’s are within +/-3.5 MHz from main spectral line (2.415 GHz).FPC coupling at most 10^5 (with HOM coupler 10^3)The main spectral line and the neighboring ones will be a concern Presently all HOM’s are far away from the dangerous beam spectral line.
Red dots just show the frequency locations
10^6
10^5
42 Managed by UT-Battellefor the U.S. Department of Energy SPL HOM Workshop at CERN, June 25-26, 2009
1.E-06
1.E-05
1.E-04
1.E-03
1.E-02
1.E-01
1.E+00
1.E+01
1.E+02
1.E+03
2.8150 2.8155 2.8160 2.8165 2.8170 2.8175 2.8180 2.8185 2.8190 2.8195 2.8200f (GHz)
Peak
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Zoom-in (Mode 35 High beta)Peak power at maximum r/Q (~0.4 Ohm)
Red dots just show the frequency locations
10^6
10^5
10^7
16 cavities have mode 35 in +/-2.5 MHz from main spectral line (2.8175 GHz).Q’s <10^7 (with HOM coupler 10^4)Only first midi-pulse sub spectral line will be a concern.Presently all HOM’s are far away from the dangerous beam spectral line.
43 Managed by UT-Battellefor the U.S. Department of Energy SPL HOM Workshop at CERN, June 25-26, 2009
1.E-06
1.E-05
1.E-04
1.E-03
1.E-02
1.E-01
1.E+00
1.E+01
1.E+02
1.E+03
2.81620 2.81625 2.81630 2.81635 2.81640 2.81645 2.81650 2.81655 2.81660f (GHz)
Peak
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Another concerns
10^6
10^5
10^7
More zoom-in (Mode 35 High beta)
1.E-101.E-091.E-081.E-071.E-061.E-051.E-041.E-031.E-021.E-011.E+001.E+011.E+02
2.8160E+09 2.8165E+09 2.8170E+09 2.8175E+09 2.8180E+09 2.8185E+09 2.8190E+09f (Hz)
Tim
e-a
vera
ge
d H
OM
po
we
r/(R
/Q),
[W
/Oh
m]
800 MeV
1000 GeV
1300 MeV
Q~10^6~80 kHz (Beam current)^2
44 Managed by UT-Battellefor the U.S. Department of Energy SPL HOM Workshop at CERN, June 25-26, 2009
w/ Beam (no measurable HOM signals from beam was observed)
Direct wakefield, just showing beam time-structure including frequencies higher than the cut-off frequency
45 Managed by UT-Battellefor the U.S. Department of Energy SPL HOM Workshop at CERN, June 25-26, 2009
Decision in 2007
Take out feedthrough as needed
46 Managed by UT-Battellefor the U.S. Department of Energy SPL HOM Workshop at CERN, June 25-26, 2009
19b TDR measurement & comparison; almost shorted Trace of discharge Dimension looks OK but large coupling HOM feed through removed Very aggressive electron activity at the HOM coupler Recovered; back in the tunnel in Feb. 08
CM12; beam line vacuum leak 12a and 12d had leaks at the feedthroughs (four out of eight)
HOM feedthroughs are removed and back to service in Feb. 09
Repair (so far 2 CMs were taken out from the tunnel)
47 Managed by UT-Battellefor the U.S. Department of Energy SPL HOM Workshop at CERN, June 25-26, 2009
SNS beam
48 Managed by UT-Battellefor the U.S. Department of Energy SPL HOM Workshop at CERN, June 25-26, 2009
Bunch fluctuation Best conservative guessing; ~0.3 % (1% will be
enough for analysis)
49 Managed by UT-Battellefor the U.S. Department of Energy SPL HOM Workshop at CERN, June 25-26, 2009
SNS beam time-structure
50 Managed by UT-Battellefor the U.S. Department of Energy SPL HOM Workshop at CERN, June 25-26, 2009
Chopper imbalance
Every 4th midi pulse; rising is slower
51 Managed by UT-Battellefor the U.S. Department of Energy SPL HOM Workshop at CERN, June 25-26, 2009
40-50 dB less than main line; negligible
52 Managed by UT-Battellefor the U.S. Department of Energy SPL HOM Workshop at CERN, June 25-26, 2009
Beam Experiences
Beam loss Much Less than 1 W/m in average Not a show stopper
Energy jitter ~1 MeV (from other sources)
No dependencies on beam loss Beam current Pulse length Pulse repetition rate As tuning is getting better, less loss/C
53 Managed by UT-Battellefor the U.S. Department of Energy SPL HOM Workshop at CERN, June 25-26, 2009
Summary
SNS HOM concerns & history Beam breakup & instability; no issue HOM power is the main reason for SNS to have HOM coupler
Availability & Reliability; Most Important Issue HOM couplers in SNS have been showing deterioration/failure as reported Reliability & availability of SNS SRF cavities will be much higher w/o HOM
coupler
More realistic analysis with actual frequency distributions measured. Probabilities for hitting dangerous beam spectral lines are much less.
Future concerns HOM feedthroughs will be taken out as needed PUP cryomodule
At least will not have HOM feedthroughs for cavities we already have Will not have HOM couplers for new cavities