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CERN SPS Upgrade
New 200 MHz and 800 MHz amplifiers
Eric MontesinosCERN-RF
15th ESLS-RF Workshop 2
CERN Accelerator Complex
Thursday, 6th October 2011
Protons and Lead Ions to maximum acceleration LINAC2 (proton) or Linac 3 (Lead ions) Booster (protons) or Leir (lead ions) PS (Proton Synchrotron) SPS (Super Proton Synchrotron) LHC (Large Hadron Collider)
Several other experiences : n_TOF – The neutron time-of-flight facility;
a neutron source that has been operating at CERN since 2001
AD – The Antiproton Decelerator; manufacturing antimatter providing low-energy antiprotons for studies of antimatter
ISOLDE – Isotope Separator On-Line; source of low-energy beams of radioactive isotopes
CLIC – the Compact Linear Collider Study; an international collaboration working on a concept for a post LHC machine to collide electrons and positrons head on at energies up to several TeV
Eric MontesinosCERN-RF
3
CERN SPS – the Super Proton Synchrotron
Thursday, 6th October 2011 15th ESLS-RF Workshop
The second largest machine in CERN’s accelerator complex, nearly 7 km in circumference. It was switched on in 1976 (CERN Nobel-prize for discovery of W and Z particles in 1983)
Presently, SPS accelerates particles to provide beams for the: FT (Fixed Target) program (North Area) CNGS project LHC (Large Hadron Collider) And Many Machine Developments
North Experimental area
CNGS : CERN Neutrions to Gran Sasso
SPS as LHC injector
Eric MontesinosCERN-RF
4
200 MHz RF in the SPS
Thursday, 6th October 2011 15th ESLS-RF Workshop
The RF-SPS started up in 1976 with two accelerating cavities
Since 1980, for the new role of SPS as proton-antiproton collider, there are four cavities operating @ 200 MHz
We have 4 lines : 2 x Siemens: 20 x RS2004 2 x Philips: 68 x YL1530
201020001976TWC#1 / TX1 TWC#2 / TX2
19901980
1978TWC#3 / TX3
1979TWC#4 / TX4
1980TWC#1 / TX1+TX2TWC#2 / TX3+TX4TWC#3 / TX5+TX6TWC#4 / TX7+TX8
Transmitter (TXB)
mW Dummy load
Coaxial transmission line(feeder line)125 to 160 meters
Accelerating cavity
Terminating loads
Configuration of one of the four200 MHz power plant
Transmitter (TXA)
Powercombiner
1975
Eric MontesinosCERN-RF
5
Two ‘Siemens’ lines = 20 x RS2004
Thursday, 6th October 2011 15th ESLS-RF Workshop
1WSolid state
100WSolid state
1kWYL1440 tube
10kWYL1520 tube
100kWRS2004 tubeTXA
4 x 125kWRS2004 tubes
One line (input cavity ~125/140 m away)
1WSolid state
100WSolid state
1kWYL1440 tube
10kWYL1520 tube
100kWRS2004 tube
Ø G
From Beam Control
TXB4 x 125kW
RS2004 tubes
1WSolid state
100WSolid state
1kWYL1440 tube
10kWYL1520 tube
100kWRS2004 tubeTXA
4 x 125kWRS2004 tubes
One line (input cavity ~125/140 m away)
1WSolid state
100WSolid state
1kWYL1440 tube
10kWYL1520 tube
100kWRS2004 tube
Ø G
From Beam Control
TXB4 x 125kW
RS2004 tubes
Eric MontesinosCERN-RF
6
Two ‘Philips’ lines = 68 x YL1530
Thursday, 6th October 2011 15th ESLS-RF Workshop
One line (input cavity ~160/180 m away)
1WSolid state
100WSolid state
1kWYL1440 tube
35kWYL1530 tube
Ø G
From Beam Control
1WSolid state100WSolid state
1kWYL1440 tube
TXA16 x 35kW
YL1530 tubes
TXB16 x 35kW
YL1530 tubes
35kWYL1530 tube
One line (input cavity ~160/180 m away)
1WSolid state
100WSolid state
1kWYL1440 tube
35kWYL1530 tube
Ø G
From Beam Control
1WSolid state100WSolid state
1kWYL1440 tube
TXA16 x 35kW
YL1530 tubes
TXB16 x 35kW
YL1530 tubes
35kWYL1530 tube
Eric MontesinosCERN-RF
7
Travelling Wave Cavities
Thursday, 6th October 2011 15th ESLS-RF Workshop
One section = 11 drift tubes
2 x 4 sections Siemens plants 2 x 5 sections Philips plants
4 Main Power Couplers 2 input couplers 2 output couplers
2 x 550 kW terminating power loads
One 4 sections cavity
One section: 11 drift tubes
Eric MontesinosCERN-RF
8
200 MHz limitations
Thursday, 6th October 2011 15th ESLS-RF Workshop
With present 4 cavities configuration we will have problems at ultimate LHC current
The increased number of shorter cavities with 2 extra power plants should significantly improve the RF performance for ultimate LHC intensities
The best compromise is 6 cavities: 4 x 3 sections cavities with 1.0 MW 2 x 4 sections cavities with 1.4 MW
Total voltage possible on the flat top vs beam current with :
4 cavities (present situation) with 1.0 MW 5 cavities with 1.0 MW RF 6 cavities with 4 x 1.0 MW + 2 x 1.4 MW Dashed lines are at nominal and ultimate
beam currents.
Courtesy of Elena
Shaposhnikova
Eric MontesinosCERN-RF
9
Cavities redistribution
Thursday, 6th October 2011 15th ESLS-RF Workshop
2011 : 4 cavities
2 x 4 sections
2 x 5 sections
+ 3 spare sections
2018 : 6 cavities
2 x 4 sections
4 x 3 sections
+ 1 spare section
Eric MontesinosCERN-RF
10
First upgrade: Present amplifiers
Thursday, 6th October 2011 15th ESLS-RF Workshop
Ratings Present Future
CW5 seconds 650 kW 700kW
Pulsed43 kHz 900 kW 1100 kW
BW-3dB 2.6 MHz 2.3 MHz
Tubes per year 6 + 16 7 + 18
HVPS need a full re-cabling and an air cooling improvement to allow higher pulsed mode
Tetrodes:Present lifetime statistics, operating ~650 kW cw:
RS2004 : 20’000 hrs: 6 tubes per year
YL1530 : 25’000 hrs: 16 tubes per
year
HVPS need a full re-cabling and air cooling improvement to allow higher pulsed mode
Eric MontesinosCERN-RF
11
New RF power plant
Thursday, 6th October 2011 15th ESLS-RF Workshop
New RF Amplifier
LSS3 Tunnel integration
New RF Building
RF amplifier
1 mW
Coaxial transmission line150 meters
Accelerating cavity
1.7 MW
RF amplifier
1 mW
Accelerating cavity
1.7 MW
New RF Building
Eric MontesinosCERN-RF
12
2018 : two new power amplifiers
Thursday, 6th October 2011 15th ESLS-RF Workshop
Must be reliable: 24/24 hours 300/365 days
(2 months winter Technical stop) 20 years of operation,
with 3 years of operation + 1 year off cycle
Pulse mode: 1.7 MW max
Average: 850 kW (thermal limitation)
2 x 1.7 MW Klystron
2 x 4 x 450 kW Diacrodes
2 x 8 x 225 kW IOTs
2 x 8 x 225 kW tetrodes Equivalent to ‘Siemens’
2 x 16 x 110 kW tetrodes Equivalent to ‘Philips’
2 x 1700 x 1 kW SSA
Eric MontesinosCERN-RF
13
1.7 MW amplifier, i.e 1.4 MW cavity
Thursday, 6th October 2011 15th ESLS-RF Workshop
To have 1.4 MW available at the cavity input, 1.7 MW at the Final output are needed
Taking advantage of the long experience we have with tetrodes and combiners, a possible solution could be a 16 x tetrodes combined through 3 dB combiners
A major improvement to present systems would be to have individual SSA drivers per tetrodes
Four contracts : Drivers (SSA) Finals (SSA or Tetrodes) Combiners (3 dB above 100 kW) Transmission lines (coaxial, 345 mm
outer)
Drivers16 SSAFinal16 Tubesor SSA
3 dBcombinersand power loads
120 m and 180 mCoaxial lines
To cavity input 120 m away
From Beam Control
1/16 splitter
1.7 MW
-0.6 dB total
1.5 MW
-0.2 dB
1.4 MW
Eric MontesinosCERN-RF
15th ESLS-RF Workshop 14
SSA vs Tetrodes
Thursday, 6th October 2011
Overdesign requirements : 14/16 tubes shall provide full power,
i.e. each tube shall deliver up to 138 kW
SSA are more ‘reliable’: 2000/2048 of the total number of devices shall deliver full power
Tetrodes tube costs over 20 years will be added : 20 year * 3/4 * 335 * 24 = 120’000
total hours With 20’000 hours per tube = ~ 200
tubes Reduced by warranty lifetime
SSA obsolescence shall be integrated: i.e. 20% additional transistors, not
module, single chips (still under discussion, need experts inputs)
Wall plug efficiency will be part of the adjudication HVPS included (Tetrodes) Losses in all SSA combiners,
circulators and loads included
Final Tetrodes(gain = 12
dB)
SSA(Gain = 20
dB)
Nominal ratings
16 x 106 kW = 1700 kW
2048 x 830 W = 1700 kW
Maximum ratingsFor 1400 kW at cavity input
Maximum2 faulty tubes14 x 138 kW = 1932 kW
Maximum48 faulty modules2000 x 891 W = 1782 kW
Maximum ratingsDriver
16 x 8.7 kW 16 x 1.1 kW
Eric MontesinosCERN-RF
15
New RF building
Thursday, 6th October 2011 15th ESLS-RF Workshop
Only possible location is between two existing buildings
Maximum ‘RF’ foot floor will be
2 x 450 m2 Whatever the solution, SSA or
Tetrodes, the same building, no impact on the choice
RF workshop
Siemens
Philips
800 MHz
Faraday Cage
Eric MontesinosCERN-RF
16
Draft schedule
Thursday, 6th October 2011 15th ESLS-RF Workshop
Install
Build new hardware
Year 4Year 3Year 2Year 1 Year 5
Building
Services
RF :
Building:
20172014201320122011 2015 2016 2018Year 6 Year 7
Tendering
Commissioning
Authorizations
Tunnel :
Build New hardwareInstallation phase 1
(pickups + dampers + CV + EL + …)
Installation phase 2(cavities)
Cavities re-arrangement within a LS ( > 6
months)
Studies (amplifiers, couplers, cavities)
MS
Studies
Studies
Eric MontesinosCERN-RF
17
200 MHZ upgrade Conclusions
Thursday, 6th October 2011 15th ESLS-RF Workshop
We will have two new 1.7 MW pulsed / 850 kW average RF power amplifiers
Building will be the same, no impact
The less expensive solution beetween SSA and Tetrode will be selected !
Eric MontesinosCERN-RF
18
800 MHz RF in the SPS
Thursday, 6th October 2011 15th ESLS-RF Workshop
The proton beams for the LHC are intense and unless careful precautions are taken they become unstable in the SPS and cannot be accepted by the LHC
One of the most important systems in the SPS used to keep the beams stable and of the highest quality is the 800 MHz RF system acting at the second harmonic of the main accelerating 200 MHz RF system
This 800 MHz system in the SPS is essential for maintaining stability of the LHC beams. It is required at every point in the cycle from injection to extraction. It works by increasing the synchrotron frequency spread in the beam
Stability is problematic above 1/5 nominal without the 800 MHz
By applying RF voltages of ~ 1 MV (about 1/7 of the main RF system) via two cavities in the SPS ring this “Landau Damping” system increases the natural spread of synchrotron frequencies in the individual proton bunches, prevents them acting together, and thus ensures stability
The RF power source and its ancillary equipment for this 800 MHz system must be of the highest reliability to ensure beams are available for the LHC at all times
Eric MontesinosCERN-RF
19
Old 800 MHz system (1)
Thursday, 6th October 2011 15th ESLS-RF Workshop
Since 1980, the system is composed of :
2 Travelling Wave Cavities
2 transmitters of 225 kW each connected via ~ 120m waveguides to the TWC
4 x 56 kW klystrons Valvo YK1198 per transmitter combined using 3 dB hybrids
Eric MontesinosCERN-RF
20
Old 800 MHz system (2)
Thursday, 6th October 2011 15th ESLS-RF Workshop
Unfortunately, that system has not been used for a very long time and has not been properly maintained.
We still only have : 2 simultaneous klystrons available
on 1 cavity 6 operational klystrons 10 broken klystrons (could be
repaired for 100’000 $ each)
We also had major difficulties with power converter transformers : 9/9 burnt 4 repaired
Eric MontesinosCERN-RF
21
Upgrade proposal
Thursday, 6th October 2011 15th ESLS-RF Workshop
Replace Klystron Transmitters with IOT Transmitters and re-use all existing peripherals
Maximum power will be slightly increased up to 240 kW CW
BW-1dB will be increased: 1.0 MHz with Klystrons 6.0 MHz with IOTs
New transmitters will include: RF power amplifiers chain Final amplifier IOT based Individual power converters
Individual Monitoring and control compatible with CERN interface
In total it will be 8 + 1 transmitters
One 800 MHz LineLayout
One 240 kW TransmitterLayout Attenuator
RF Power Amplifier 60 kW cw
RF Power Amplifier 60 kW cw
RF Power Amplifier 60 kW cw
RF Power Amplifier 60 kW cw
Sp
litte
r
Monitoringand
Controls
Amplifiers
Power converters
Monitoringand
Controls
Amplifiers
Power converters
Monitoringand
Controls
Amplifiers
Power converters
Monitoringand
Controls
Amplifiers
Power converters
3d
B C
om
bin
er
3d
B C
om
bin
er
3d
B C
om
bin
er
Power load
Power loadCavity Terminating load
Cavity and TransmitterMonitoring and Controls
(CERN)Power load
Ø shifter
AttenuatorØ shifter
AttenuatorØ shifter
AttenuatorØ shifter
waveguide line(125 meters )
Eric MontesinosCERN-RF
22
Selected supplier : Electrosys
Thursday, 6th October 2011 15th ESLS-RF Workshop
Two companies per member state have been contacted (40 companies)
Six companies have been compliant to our specifications
Electrosys has been selected
‘Quasi’ off the shelves Transmitter
Possibility to have Thales or e2v trolleys and tubes for the same price
Eric MontesinosCERN-RF
23
Factory Acceptance Tests:various operational modes
Thursday, 6th October 2011 15th ESLS-RF Workshop
Continuous operation 24/24 hours CW for 10 months continuously
24 hours made prior to our visit. 4 hours made with us
Very Long Pulses operationFc = 800.888 MHz +/- 0.5 MHz :100% from 0 to 240kW with rise and fall time < 0.5 µs5 seconds ON / 5 seconds OFF
One hour made with us
AM modulation #1Fc = 800.888 MHz +/- 0.5 MHz :100% from 0 to 240kW with rise and fall time < 0.5 µsRepetition time 10 µs (100kHz)
One hour made with us
AM modulation #2Fc = 800.888 MHz +/- 0.5 MHz :0 to 240kW with 4 MHz triangle AM 25 % in powerRise and fall time < 0.5 µsFlat top pulse and off pulse length of 11 usRepetition time 23 µs (43kHz)This cycle for 20 second then 1 second OFF.
One hour made with us
time
Power
5 s
0.5 us 0.5 us
240 kW
0 kW
10 s
time
Power
10 us
0.5 us0.5 us
240 kW
0 kW
time
Power
11 us
0.5 us 0.5 us
240 kW
0 kW
11 us
23 us
20 s 1 s
4 MHz triangle
25 %
Eric MontesinosCERN-RF
24
Factory Acceptance Tests:Bandwidth
Thursday, 6th October 2011 15th ESLS-RF Workshop
Power Amplifier (Driver + Final)
Operating frequency :
800.888 MHz
Bandwidth at -1dB :
6.0 MHz (+/- 3.0 MHz)
CW output minimum power :
60 kW
Amplifier meets all requirements 790
796.
5
797.
25 798
798.
75
799.
5
800.
25
800.
888
801.
5
802.
25 803
803.
75
804.
5
805.
25 806
0
10
20
30
40
50
60
70
Pout vs frequency
Frequency [MHz]
Pout
[kW
]
Pmax = 61.0 kW
Pmax -1dB = 47.5 kW
BW-1dB = 7.0 MHz (-3/+4 MHz)
Eric MontesinosCERN-RF
25
Factory acceptance tests:Phase stability
Thursday, 6th October 2011 15th ESLS-RF Workshop
Carrier f0 at mid power (30 kW)with additional - 20 dB power sweep
Fully fulfill specification
Measurements to be made with each Power AmplifierAND
with the whole Transmitter (i.e. four Power Amplifiers combined together)
Measurements with a 800.888 MHz carrier at Pmax/2 and a frequency sweep 20dB below carrier :
Non linear phase distortionat +/-3.0 MHz: max. +/- 10°
Passband at -1 dB: 5.0 MHzPassband at -15 dB: 8.0 MHz
Eric MontesinosCERN-RF
26
Factory acceptance tests:Power Sweep
Thursday, 6th October 2011 15th ESLS-RF Workshop
Measurements to be made with each Power Amplifier
AND
with the whole Transmitter (i.e. four Power Amplifiers combined together)
With four PA : Po = 240 kW
With one PA : Po = 60 kW
Pout vs Pin must be monotonic from zero to Po
Small signal differential gain g = dPout/dPin, in the range 0.1 Po to 0.9 Po
Local slope variation max +/-15%
Can vary by 3 dB maximum.
Gain saturation curve
Small signal differential gain in the range 0.1 Po to 0.9 Po:
Local slope variation +/- 5% (+/- 2% averaged)
Vary by 2.0 dB maximum
Non linear phase distortion (CW):
Δ φmax < 10º
Non linear phase distortion curve
Phase distortion < 3°
Pout
0.9 Po
0Pin
0.1 Po
3 dB maximum
g
gmax
gmin
Pin
g = dPout/dPin
Phase shift
Pin
Δ Φ max < 10ºAt Pin for Po
-25.
0-2
3.8-2
2.6-2
1.4-2
0.2-1
9.0-1
7.8-1
6.6-1
5.4-1
4.2-1
3.0
19.0020.0021.0022.0023.0024.0025.00
-80-78-76-74-72-70
Gain Phase
Drive in [dBm]
IoT G
ain
[dB
]
Phase [
deg]
-25.
0-2
3.8-2
2.6-2
1.4-2
0.2-1
9.0-1
7.8-1
6.6-1
5.4-1
4.2-1
3.0
2527293133
f(x) = − 0.002588706 x² + 0.232314847 x + 25.76504335
differential TX gain
Diff
ere
nti
al gain
[d
B]
-6-4-202468
10
Local slope
Local slo
pe
vari
ati
on
[%]
0.1 Pmax 0.9 Pmax
Eric MontesinosCERN-RF
27
Factory Acceptance Tests:conclusion
Thursday, 6th October 2011 15th ESLS-RF Workshop
All factory acceptance tests have shown compliance respect to the specification, and even better : Linearity Monotonous Phase stability Maximum output power
All requirements were fulfilled (we repeated all the tests twice to confirm the results)
We checked modularity of the equipments
We controlled noise level
We checked protections: driver output reflected power operated while making tests (due to over range
power sweep) Water cooling, air temperature, current limits, etc …
Eric MontesinosCERN-RF
28
CERN Acceptance Tests
Thursday, 6th October 2011 15th ESLS-RF Workshop
Pre-series Amplifier has been integrated within CERN operational area
All tests cycles have been done for 4 hours each, no trouble has been discovered
Eric MontesinosCERN-RF
29
Long duration tests:CW mode
Thursday, 6th October 2011 15th ESLS-RF Workshop
When we launch CW long duration tests, difficulties arose
While doing the test over six weeks, we were not able to obtain a stable operation
Maximum time slots were : 115 hours : 1 66 hours: 2 33 hours: 5 < 24 hours : 18
→ Not stable enough in CW mode
41 2 0.50.50.15
50.50.50.52.5
13
0.5
16
4
33 33 33
20
710
32
11
60
115
34
8
0.5
14 16
5
66
19
50.5
23 24
1620
13
26
1512
1512 12 12
25
1410 9
0.020.02
84
31
8
32
47
0
20
40
60
80
100
120
140
Ca
lib
ra
te
dir
ecti
on
el
co
up
leu
r
-7 a
pril
Ne
wch
arg
e 2
50
kW
-4
ap
ril
Ad
juste
me
nt
tub
e b
y p
ho
ne
wit
h M
r.
Be
l -1
5 a
pril
Cle
an
ing
filt
er
-6 M
ay
Ad
juste
me
nt
tub
e w
ith
M.
Be
l -1
2 M
ay
HV iInhibit & HVPS Over
Voltage64%
HV Inhibit18%
Inverter Fault18%
CW Alarm repartition
Eric MontesinosCERN-RF
30
Air temperature sensitivity
Thursday, 6th October 2011 15th ESLS-RF Workshop
Transmitter has shown to be Temperature sensible : Water Temp = 26.4 +/- 0.5 Air Temps = 22.1 +/- 2.6 Driver Gain = 6.7 % Cold IOT = + 7.5 % to - 38 % Hot IOT = +/- 4.9 %
Drivers are inverse temp, while IOT is direct Temp
Restart a cold IOT must be done readjusting the drive within the first three minutes
CERN LLRF will manage these variations
Temp waterTemp air
Temp water Temp airRelative gain IOT
Eric MontesinosCERN-RF
31
Long duration tests:Super Cycle mode
Thursday, 6th October 2011 15th ESLS-RF Workshop
41 2 0.50.50.15
50.50.50.52.5
13
0.5
16
4
33 33 33
20
710
32
11
60
115
34
8
0.5
14 16
5
66
19
50.5
23 24
1620
13
26
1512
1512 12 12
25
1410 9
0.020.02
84
31
8
32
47
0
20
40
60
80
100
120
140
Ca
lib
rate
dir
ecti
on
el
co
up
leu
r -7
ap
ril
Ne
wch
arg
e 2
50
kW
-4
ap
ril
Ad
juste
me
nt
tub
e b
y p
ho
ne
wit
h M
r.
Be
l -1
5 a
pril
Cle
an
ing
filt
er
-6 M
ay
Ad
juste
me
nt
tub
e w
ith
M.
Be
l -1
2 M
ay
010203040506070
0 3000 6000
Pout
[kW
]
Time [ms]
To reduce average power and be closer to machine operation, we launched Super Cycle long duration tests, new difficulties arose
While doing the test over four weeks, we were not able again to obtain a stable operation
Time slots were mainly between 12 to 24 hours
The main fault is always the same ‘IGBT 4 gate D’, even with no amplifier connected !
We are convinced the tube itself is not part of the trouble
Eric MontesinosCERN-RF
32
HVPPS instabilities
Thursday, 6th October 2011 15th ESLS-RF Workshop
We tried a 50% RF signal instead of our super cycle, varying the repetition rate
The HVPPS stability is function of the repetition rate !
010203040506070
0 50 100
Pout
[kW
]
Time ON [%]
0
100
200
300
400
500
600
700
800
900
1000
0.1 0.5 1 5 10 50 100 500 1000 1500 1600 1700 1800 2000 2100 2500
Sta
bil
ity
[se
co
nd
s]
Repetition rate [Hz]
Power converter stability vs Repetition rate
20 hours10 hours
10 hours20 hours
100 hours
Eric MontesinosCERN-RF
33
800 MHZ upgrade Conclusions
Thursday, 6th October 2011 15th ESLS-RF Workshop
First tests were very promising, but…
Long duration tests shown lack of HVPPS stability
We asked for a conventional linear Power Converter (with thyratron crowbar)
Installation is foreseen next week …
Many thanks
For your attention, and for inviting me to your workshop
Eric MontesinosCERN-RF
35
RF Group at CERN
Thursday, 6th October 2011 15th ESLS-RF Workshop
RF group is 170 colleagues operating RF over all machines
A. Cobas, L. DupontGroup Secretaries
a d i o – r e q u e n c y G r o u pE. Jensen
Dpt. E. Ciapala
Beamsand RFCavityServos
& ControlsInterfaceRF Feedbacks
& BeamControlKlystrons
& SC CavitiesLinacsRF Synchrotrons RF
BR FB LR
E. ShaposhnikovaDpt. T.Bohl
A. Butterworth Dpt. L. Arnaudon
W. HöfleDpt. P. Baudrenghien
O. Brunner Dpt. G. Mcmonagle
M. VretenarDpt. F. Gerigk
E. MontesinosDpt. C. Rossi
T. Argyropoulos(DOCT)F. CaspersJ. Esteban Muller (FELL)S. Federmann (DOCT)L.Ficcadenti (FELL)S. HancockR.M. Holz (TECH)H. Timko (FELL)J. Tückmantel
M.E. AngolettaP. Baudrenghien
A. K. Bhattacharyya(FELL)J. Ferreira-BentoG. HagmannT. MastoridisJ. NoirjeanD. Stellfeld
A.BlasA. Bullitt (UPAS)H. DamerauA. FindlayJ. Fox (UPAS)M . Hernandez-Flano (FELL)P. Leinonen(FELL)T. Levens(FELL)J. Lollierou(FELL)R. LouwerseD. PerreletT. TruszcynskiD. ValuchU. Wehrle
L. ArnaudonD. LandreS. Totos
F. DubouchetM.JaussiJ. MolendijkM. Naon(UPAS)A. Pashnin (FELL)A. ReyF. Weierud
D. GlenatP. Martinez-YanezP. Maesen
G. Pechaud
G. McmonagleS. CurtG. Rossat
A. Benoit (Stagiaire) I. Mondino(FELL)C. NicouS. Mikulas(TECH)M .PasiniJ. PradierG. RavidaN. Schwerg(FELL)M. Therasse(FELL)W. Weingarten
J. Chambrillon(FELL)T. Junginger(DOCT)C. Liao (FELL)H. Vennekate(TECH)
J. BroereV. CobhamS. Doebert
A. Andersson W. Farabolini(UPAS)J-W. Kovermann(FELL)R. L. Lillestol (DOCT)S. LivesleyJ. MonteiroS. ReyR. Ruber(UPAS)H.S. Shaker (PJAS)L. TimeoT. Wiszniowski
F. GerigkN. Alharbi(UPAS)M. Schuh(UPAS)P. Ugena-Tirado (FELL)R. Wegner
G. GeschonkeJ.M. GiguetJ. Marques BalulaS. Ramberger K. Schirm
A. Boucherie S. CalvoG. Cipolla C. JulieN. Jurado F. KillingC. Marrelli (FELL) M. PaoluzziC. Renaud C. Vollinger
G. RiddoneA. Acker (UPAS) M.Filippova (PJAS)A. French (PJAS) N. Gazis(DOCT)D. Gudkov(PJAS) I. Kossyvakis(TECH)A.Olyunin(UPAS) P. Piirainen(FELL)F. Rossi (FELL) A. Samoshkin (UPAS)V. Soldatov(UPAS)A. Solodko (UPAS)J. Vainola(UPAS)
W. WuenschM. Dehler (PDAS)N. Shipman (DOCT)I. SyratchevA. Grudiev
A. D’Elia (UPAS) G. De Michele (UPAS)V. Khan (FELL) O. Kononenko(FELL)J. Shi(FELL) K. Sjoebaek(PJAS)H. Zha(UPAS)
C. RossiV. Bretin V. DesquiensM. Haase G. LobeauA. Marmillon M. MorvilloS. TavaresRego(UPAS)
DOCT = Doct. Student FELL = Fellow SUMM=Summer Student TECH = Techn. Student PDAS= Paid Ass. UPAS = Unpaid Ass. PJAS= Project Ass. Underlined = Supervisors
September2011