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![Page 1: The Expanded Very Large Array - National Radio Astronomy · PPT file · Web view · 2002-01-18Preliminary Design Review EVLA 1st and ... Output Power +14 dBm +/- 0.5 db 1st LO YIG](https://reader035.vdocument.in/reader035/viewer/2022062600/5ab627677f8b9a86428d6f0b/html5/thumbnails/1.jpg)
Preliminary Design Review
EVLA1st and 2nd Local Oscillators
![Page 2: The Expanded Very Large Array - National Radio Astronomy · PPT file · Web view · 2002-01-18Preliminary Design Review EVLA 1st and ... Output Power +14 dBm +/- 0.5 db 1st LO YIG](https://reader035.vdocument.in/reader035/viewer/2022062600/5ab627677f8b9a86428d6f0b/html5/thumbnails/2.jpg)
Jim Muehlberg
EVLA LO-IF PDR22-23 January 2002
2
Specifications – 1st LO
• 12-20 GHz– FO = (n*512 MHz +/- FTS) where 23<=n<=40– Tuning Span Fo +/- TBD
• Phase Noise– -90 dBc @ 10 kHz @ 20 GHz (x fs)– -107 dBc @ 100kHz @ 20 GHz (x fs)
• Output Power– +14 dBm +/- 0.5 db
![Page 3: The Expanded Very Large Array - National Radio Astronomy · PPT file · Web view · 2002-01-18Preliminary Design Review EVLA 1st and ... Output Power +14 dBm +/- 0.5 db 1st LO YIG](https://reader035.vdocument.in/reader035/viewer/2022062600/5ab627677f8b9a86428d6f0b/html5/thumbnails/3.jpg)
Jim Muehlberg
EVLA LO-IF PDR22-23 January 2002
3
1st LO YIG
• Electromagnetically Tuned YIG oscillator by Micro-Lambda
• Integrated Drivers• Requires +15 VDC @
700mA and +24 VDC @ 50 mA
• 1.75” Cylinder
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Jim Muehlberg
EVLA LO-IF PDR22-23 January 2002
4
Specifications - 2nd LO
• 10.8 – 14.8 GHz• Fo = n*128 +/- FTS where 84<=n<=116
• Tuning Span: Fo +/- TBD (almost continuous)
• Phase Noise• -90 dBc @ 10 kHz @ 14.8 GHz• -105 dBc @ 100 kHz @ 14.8 GHz
• Output Power• +14 dBm +/- 0.5 dB
![Page 5: The Expanded Very Large Array - National Radio Astronomy · PPT file · Web view · 2002-01-18Preliminary Design Review EVLA 1st and ... Output Power +14 dBm +/- 0.5 db 1st LO YIG](https://reader035.vdocument.in/reader035/viewer/2022062600/5ab627677f8b9a86428d6f0b/html5/thumbnails/5.jpg)
Jim Muehlberg
EVLA LO-IF PDR22-23 January 2002
5
2nd LO YIG
• Permanent Magnet YIG Oscillator by Micro-Lambda
• Integrated Drivers• Requires +/- 12 VDC
@ 365 & 165 mA and +15 VDC @ 50 mA
• ~ 7.2 Watts
1” Cube
![Page 6: The Expanded Very Large Array - National Radio Astronomy · PPT file · Web view · 2002-01-18Preliminary Design Review EVLA 1st and ... Output Power +14 dBm +/- 0.5 db 1st LO YIG](https://reader035.vdocument.in/reader035/viewer/2022062600/5ab627677f8b9a86428d6f0b/html5/thumbnails/6.jpg)
Jim Muehlberg
EVLA LO-IF PDR22-23 January 2002
6
General Functional Description
• Power on reset – report back “OK”• MIB Frequency command• Coarse tune loop (prescaler + MIB)• AGC DAC set to cal data• Loop Closes, Lock to comb +/- FTS• Output tracks FTS• Only monitor data reported back, FTS operates
“autonomously” reducing M/C load & RFI
![Page 7: The Expanded Very Large Array - National Radio Astronomy · PPT file · Web view · 2002-01-18Preliminary Design Review EVLA 1st and ... Output Power +14 dBm +/- 0.5 db 1st LO YIG](https://reader035.vdocument.in/reader035/viewer/2022062600/5ab627677f8b9a86428d6f0b/html5/thumbnails/7.jpg)
Jim Muehlberg
EVLA LO-IF PDR22-23 January 2002
7
Reference
• Herotek Comb Generator – 128 or 512 MHz @ 0 dBm
input– Integrated driver amplifier,
+15 VDC @ 200mA– “Like” GC526, GC100
• Equalizer (Custom Matched)
• Band Pass Filter• Splitter (2 or 4-way)
![Page 8: The Expanded Very Large Array - National Radio Astronomy · PPT file · Web view · 2002-01-18Preliminary Design Review EVLA 1st and ... Output Power +14 dBm +/- 0.5 db 1st LO YIG](https://reader035.vdocument.in/reader035/viewer/2022062600/5ab627677f8b9a86428d6f0b/html5/thumbnails/8.jpg)
Jim Muehlberg
EVLA LO-IF PDR22-23 January 2002
8
Block Diagram
• YIG• Isolator• Prescaler Coupler• AGC Amplifier• Output Coupler• Output Splitter• Mixer L port
• Mixer R Port– Comb Generator– Equalizer– BPF– Splitter (2 or 4 Way)
![Page 9: The Expanded Very Large Array - National Radio Astronomy · PPT file · Web view · 2002-01-18Preliminary Design Review EVLA 1st and ... Output Power +14 dBm +/- 0.5 db 1st LO YIG](https://reader035.vdocument.in/reader035/viewer/2022062600/5ab627677f8b9a86428d6f0b/html5/thumbnails/9.jpg)
Jim Muehlberg
EVLA LO-IF PDR22-23 January 2002
9
Block Diagram
• Mixer I port• Band Pass Filter (128
MHz)• IF Amplification• Band Pass Filter• Divider
– Lock Detector– Phase Detector
• Phase Detector• Loop Filter• FM Coil Driver• (Loop Closed)
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Jim Muehlberg
EVLA LO-IF PDR22-23 January 2002
10
Design Considerations
• MIB handles most functions• Onboard SRAM holds cal data, etc.• No Mechanical Adjustments• SPI bus devices – DAC’s, ADC’s and
digital potentiometers• Design in flexibility in prototype – “EVB”
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Jim Muehlberg
EVLA LO-IF PDR22-23 January 2002
11
RFI Considerations
• Comb line filtered at source• Continuous wire mesh gaskets• Front panel ??• Prescaler • Non – RF connectors minimally sized
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Jim Muehlberg
EVLA LO-IF PDR22-23 January 2002
12
Monitor and ControlPoints
• Monitor– O/P Power– FTS Power– Lock– YIG Heater I– PLL V and I– Frequency (1 MHz)– Temperature
• Control– YIG Main Tune– AGC– Reset– FTS Parameters– Various Calibration
capabilities (NO MECHANICAL!)
![Page 13: The Expanded Very Large Array - National Radio Astronomy · PPT file · Web view · 2002-01-18Preliminary Design Review EVLA 1st and ... Output Power +14 dBm +/- 0.5 db 1st LO YIG](https://reader035.vdocument.in/reader035/viewer/2022062600/5ab627677f8b9a86428d6f0b/html5/thumbnails/13.jpg)
Jim Muehlberg
EVLA LO-IF PDR22-23 January 2002
13
Front Panel
• Lock indicator (not uP dependant)• Frequency • FTS Sample• Reference / Clock Sample• FM coil Voltage / (selectable)
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Jim Muehlberg
EVLA LO-IF PDR22-23 January 2002
14
Questions