500 MHZ Solid State Amplifier Design Progress Report
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Transcript of 500 MHZ Solid State Amplifier Design Progress Report
Paul Scherrer Institut • 5232 Villigen PSI 5th CWRF Conference - CERN - 3/2008 M. Gaspar
500 MHZ Solid State Amplifier Design Progress Report
M. Gaspar, M. Pedrozzi
Paul Scherrer Institut • 5232 Villigen PSI 5th CWRF Conference - CERN - 3/2008 M. Gaspar
Comissioning of 4KW Validation Prototype
PC Master Controller: 2 Available (PSI Design)
Power Supply Controller: 25 Boards Available (Programmed and Tested) (PSI Design)
Power Splitter: 2 8-Way Prototypes Working (PSI Design)
250W Amplifier Module: 12 Modules Available (Already tested). 10 Ready for Tests (PSI Design)
Cooling Bar: Ready to Accommodate New DC-DC Converter.
High Power Coupler: 1 Piece Available and Calibrated (Industry)
New Design in Progress (PSI Design)
Output Power Combiner: 2 18-Way Combiners Ready (Finished and Tested) (PSI Design)
Cables: Waiting for Delivery (1 or 2 weeks more) (Industry)
Watter Cooled Load: 1 Piece Available (Industry)
Paul Scherrer Institut • 5232 Villigen PSI 5th CWRF Conference - CERN - 3/2008 M. Gaspar
4KW Amplifier Configuration
Paul Scherrer Institut • 5232 Villigen PSI 5th CWRF Conference - CERN - 3/2008 M. Gaspar
4.5KW Basic Components( 3D Conceptual View – Not To Scale )
+
+
2x
18x
18x
+
+
=
5KW max!
Paul Scherrer Institut • 5232 Villigen PSI 5th CWRF Conference - CERN - 3/2008 M. Gaspar
250W Amplifier Module
Key Performance Parameters
3D-View of 500MHz Amplifier Module
Output Power (with Circulator)
250W 280W
Gain 22dB 20dB
Efficiency ~ 54% ~ 50%
Operation Max
Pout(W) vs Pin(W)
0
50
100
150
200
250
300
0 0.2 0.4 0.6 0.8 1 1.2 1.4 1.6 1.8 2
Pin(W)
Po
ut(
W)
Pout (dBm)
Phase(S21) (°) vs Pout(W)
80.00
90.00
100.00
110.00
120.00
130.00
140.00
150.00
0 50 100 150 200 250 300
Pout(W)
Ph
as
e(S
21
) (°
)
Phase (°)
Paul Scherrer Institut • 5232 Villigen PSI 5th CWRF Conference - CERN - 3/2008 M. Gaspar
250W Amplifier Module
Pout(W) x Pin(W)
0
50
100
150
200
250
300
0 0.5 1 1.5 2 2.5
Pin(W)
Pout
(W)
M#1
M#2
M#3
M#4
M#5
M#6
M#7
M#8
M#9
M#10
Efficiency(%) x Pout(W)
0.0
10.0
20.0
30.0
40.0
50.0
60.0
0 50 100 150 200 250 300
Pout(W)
Effic
iency
(%)
M#1
M#2
M#3
M#4
M#5
M#6
M#7
M#8
M#9
M#10
Output Power versus Input Power
Efficiency versus Output Power
Performance of first 10 RF Modules
Paul Scherrer Institut • 5232 Villigen PSI 5th CWRF Conference - CERN - 3/2008 M. Gaspar
250W Amplifier Module
Mag(S21) (dB) x Pout(W)
0
5
10
15
20
25
0 50 100 150 200 250 300
Pout(W)
Mag
(S21
) (dB
)
M#1
M#2
M#3
M#4
M#5
M#6
M#7
M#8
M#9
M#10
Phase(S21) (°) x Pout (W)
0
20
40
60
80
100
120
140
160
180
200
0 50 100 150 200 250 300
Pout (W)
Phas
e(S21
) (°)
M#1
M#2
M#3
M#4
M#5
M#6
M#7
M#8
M#9
M#10
Gain versus Output Power
Phase Delay versus Output Power
Performance of first 10 RF Modules
Paul Scherrer Institut • 5232 Villigen PSI 5th CWRF Conference - CERN - 3/2008 M. Gaspar
250W Amplifier Module
K - Stability Factor
0
10
20
30
40
50
60
70
80
0.00E+00 5.00E+08 1.00E+09 1.50E+09 2.00E+09 2.50E+09 3.00E+09 3.50E+09 4.00E+09 4.50E+09
f (Hz)
db
(K)
db(K)
B1 - Stability Factor
0
0.5
1
1.5
2
2.5
0.00E+00 5.00E+08 1.00E+09 1.50E+09 2.00E+09 2.50E+09 3.00E+09 3.50E+09 4.00E+09 4.50E+09
f (Hz)
B1 B1
Amplifier is Unconditionally Stable
Paul Scherrer Institut • 5232 Villigen PSI 5th CWRF Conference - CERN - 3/2008 M. Gaspar
250W Amplifier Module
Pout(W) x Vdd(V)
150
170
190
210
230
250
270
290
22 24 26 28 30 32 34
Vdd(V)
Pout
(W) Pin=1.77W
Pin=1.65W
Phase(S21) (°) x Vdd(V)
120
121
122
123
124
125
126
127
128
129
130
22 24 26 28 30 32 34
Vdd(V)
Phas
e(S2
1) (°
) Pin=1.77W
Pin=1.65W
Output Power Variation due to Forced Compression
Phase Delay Variation due to Forced Compression
1. Since our Power Supply Controllers allow the Power Supply Voltage (Vdd) to be changed remotely we use Forced Compression to equalize the output powers of all amplifiers and then maximize the Combining Efficiency.
2. Notice that the Phase Delay is not very much influenced by variations in Power Supply Voltage. So Forced Compression is a viable method.
Forced Compression as a Useful Method
Paul Scherrer Institut • 5232 Villigen PSI 5th CWRF Conference - CERN - 3/2008 M. Gaspar
250W Amplifier Module
• Total 22 Modules Produced Now (18 for Amplifier, 4 Spares).
• 12 Modules Fully Tested.
• 10 Modules Assembly Finished But Not Yet Tested .
• Performance Agrees With Previous Results from Prototype.
• Remote Monitoring Working all right.
Paul Scherrer Institut • 5232 Villigen PSI 5th CWRF Conference - CERN - 3/2008 M. Gaspar
18 Way Combiner – 500MHz
BW > 10MHz (S11 < -30dB)
Precision Required for 18 Ways Realized with no Extra Costs
Efficiency > 99.6% (Overall Loss < 20W @ Pout=4.5KW)
Key Performance Parameters
Measurement
HFSS Simulation
PSI development
Paul Scherrer Institut • 5232 Villigen PSI 5th CWRF Conference - CERN - 3/2008 M. Gaspar
RF Switch
RF Rise Time/Fall Time: 1us
Operating Frequency: 500MHz
On/Off Switching Time: < 20ns
Remote Controlled Through Network
RF Limitter/Protection Included
External Interlock Reaction Time: < 100ns
In/Out Isolation: 80dB
Insertion Loss: 0.5
Main Performance Parameters
Design Finished All Components Available
Construction to Start Soon
Status
Paul Scherrer Institut • 5232 Villigen PSI 5th CWRF Conference - CERN - 3/2008 M. Gaspar
Power Supply Controller(and Complete Monitoring System)
RS485Network
Power SupplyOutput
AmplifierMonitoring
Extra DigitalI/Os
Extra AnalogI/Os
DC/DC Converter
High Voltage Input and Filtering
Output Power: 600W
Output Voltage Range: 16.7V to 33.5V
Input Voltage Range: 200V to 400V
Efficiency: ~ 90%
Can be Remotely Programmed and Monitored
Extra Analog and Digital I/Os
Multi-tasking Script Operating System (SOS)
Interlock Reaction Time: ~ 1uS
Full Monitoring Loop Time: ~ 150mS
Main Features
25 Pieces Available Now
LEDs for Interlock and operation
Design Finished
Paul Scherrer Institut • 5232 Villigen PSI 5th CWRF Conference - CERN - 3/2008 M. Gaspar
• Total 25 Boards Produced Now (18 for Amplifier, 7 Spares).
• Operating System Installed.
• All Tests Completed (Power and Monitoring).
• Boards Ready To Use.
Power Supply Controller
Paul Scherrer Institut • 5232 Villigen PSI 5th CWRF Conference - CERN - 3/2008 M. Gaspar
SOS (Save Our Souls)(Originally: Script Operating System)
Runs ASCII Scripts: No Need for Previous Compilation
Available Commands for Analog and Digital I/O
Simplified IBM BSC Protocol implementation for Network Applications
Can also be used in Autonomous Applications (No Network)
Optimized for Data Acquisition
Multi-tasking Environment: Allows Monitoring and Data Taking Simultaneously
Precise Time-Base for Timing Applications: 1mS
Almost all Code Portable to other Microcontrollers
Designed in House: No Commercial Licen$e Needed
Main Features
Actual Version: SOS v2.97.4Programmed in All Power
Supply Controllers
Paul Scherrer Institut • 5232 Villigen PSI 5th CWRF Conference - CERN - 3/2008 M. Gaspar
Power Supply Controller
and Monitoring System Tests
Power Supply Output
High VoltageInput
(220Vac)
RFin
Amplifier Monitoring
RS485Network
RFout
Cooling Plate
Paul Scherrer Institut • 5232 Villigen PSI 5th CWRF Conference - CERN - 3/2008 M. Gaspar
Status• Voltage Stabilizer not Yet Available (2 to 3 weeks more).
• RF Components all Available.
• RF Switch in Progress.
• Power Supply Controllers Ready.
• High Power Output Directional Coupler: Prototype Tests OK, Design in Progress.
• RF Cables waiting for Delivery.
• Monitoring and DAQ Software in Preparation (Linux).
Conclusions• Rf Module Design proven and working. Unconditional Stability proven. High Gain and High Power available.
• All monitoring is working all right as designed.
• Available parameters for monitoring per RF module:
Output Forward Power, Input Forward Power, Output Reflected Power, Transistor Temperature, Power Supply Current, Power Supply Voltage.
• Power Supply Voltage can be set remotely.
• Power Supply controller heavily tested. Monitoring and Data Acquisition concept proven.
• Whole 5KW Prototype will be ready and operational soon.