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WP06_AntennaIF
equalizer bandpass filter
bandpass filter
equalizer
equalizer bandpass filter
spare
detector
a/d
RFNitro NBB-300
dewar
alternate location for bandpass filter
thermoelectric temperature regulation(if needed)
microcontroller
laser power monitor, laser temp monitorCANbus
SP4Tswitch
80-116 GHz
210-270 GHz
28-36 GHz
CARMA I.F. block diagram v. 2.1Dick Plambeck, 13 Sep 2002
eq
atten 0-30 dB eq
atten 0-30 dB eq
bias tee
DC bias
0 dBmlaser trx
HMC 424
amplifier module
WP06_AntennaIF3 principal modules
• switch
• amplifier (= ATA ‘PAM’)– includes attenuators (0-60 dB), power detector, and bias
tee for the laser transmitter– integrate with CANbus controller?– aluminum box; mount flange to temperature regulated
plate, or if necessary to separate thermoelectric cooler
• laser transmitter (= ATA ‘OTX’)
WP06_AntennaIF: amplifier module = ATA post-amp module
• frequency range 500 MHz – 10 GHz• gain flat within ±3 dB across band• input noise temp < 1200 K• input pwr level –50 dBm to +10 dBm (!)• linearity better than 1%• gain stable to 1 part in 103, if temperature
regulated to 0.1 C
WP06_AntennaIF:prototype ATA PAM
WP06_AntennaIFprototype PAM; gain ~ 50 dB
amplifier module: gain compression ~ 1% at 1.5 dBm output power
output pwr
gain, .02 dB/div
input pwr swept from –60 dBm to –45 dBm
WP06_AntennaIFtemperature dependence of gain
0.3 dB / 20 C 0.4% / C
gain stability of 10-3 requires ±0.1 C temp regulation
high freq ripples due to poor output match
WP06_AntennaIF: optical transmitterNEC NX8560LJ
1550 nm DFB laser + electroabsorption modulator + TEC
WP06_AntennaIF: laser transmitter = ATA OTX module
• includes:– NEC NX8560LJ
• laser• EA modulator• thermoelectric cooler• photodiode power monitor• thermistor
– TEC controller (5 V, ~ 1 amp)– laser current supply– modulator DC bias (bias tee located in amplifier module)
• Photonics Inc will build 700 modules for ATA; cost approx $2.5 K each
WP06_AntennaIFopen questions
• will detector on amplifier module be used for beamswitched continuum measurements?
• if so, will switched-power demodulation be done at the IF CANbus node? how will mirror position be transmitted?
• power supply: requires ~ 1 amp at 5 V; is it necessary to get this from 24 V dc-dc converter
• can RF power damage the electroabsorption modulator; how to protect without compromising linearity?
WP02_LOreference key features
• distributes two reference frequencies (1100-1260 MHz tunable, 10 MHz fixed) from control building to antennas via singlemode optical fiber
• linelength system continuously monitors electrical delay through each fiber to an accuracy of ~0.1 picosec, approx 8° phase at 230 GHz
• 1 pps tick distributed to antennas, as a missing pulse on the 10 MHz reference
• allow for 3 subarrays operating with different reference frequencies
WP02_LOreference:current BIMA system
Agere 3540AAgere 2510B
Agere 2510B
linelength rcvr
NI 6031EI/O
Wavetek synth
8662synth
1100-1260 MHztunable
Ortel 3120A-101-102
10 MHz TTL
f_ref
f_ref+ 10 MHz
1310 nm laser
-20dB
-10dB
1310 nm laser
Agilent HFBR2316T
photoreceiver
10 MHz cleanup osc
4-way opticalpwr splitter
+1 dBm
9.99995 MHzfixed
offsetosc
computer
a/d converter
fiberoptic coupler
10 MHz
10 MHz
missing pulse generator
1 pps tick1 pps tick
10 MHz
1100-1260 MHz
50 Hz sine wave
LO distribution and linelength systems
Dick Plambeck, 8 June 02
pwr splitter12-way optical
WP02_LOreferencephase noise vs optical pwr
optical pwr rms
coax 6.3°
-2 dBm 6.65°
-6 dBm 7.05°
-9 dBm 8.31°
WP02_LOreferencecurrent BIMA fiber distribution
splice tray
weathertight box on
portable stand
az wrap
elev wrap
umbilical
weathertight box on side of
antenna
underground cable
patch panel
rcvr
echo
LO ref out
antenna fiber
lab
FC/APC connector
approx 135 feet (200 nsec) of fiber exposed to outdoor air temp
linelength monitor via roundtrip phase
• 135’ of fiber at outdoor air temp ( = 200 nsec)
~ 2 psec/C
~ 180°/C at 230 GHz
WP02_LOreferencelinelength options
TRX
RX
CPL TRX
RX
CPL
1. echo on 2nd fiber
do fiber lengths track each other?
2. echo on same fiber
temperature coefficients of circulators?
reflections from bad connectors?
optical circulators
WP02_LOreference: 3-fiber test
echo from 1 antenna coupled back on 3 separate fibers: 3 independent measurements
WP02_LOreference: 3-fiber test
0.2 psec glitches during slew
1 psec long term drifts due to cabin temp change
example of linelength correction
raw data linelength-corrected
3c454.3, 86 GHz, baseline 2-8, through sunrise
thermal tests of 10 MHz fiber link from ‘good’ antenna
thermal tests of 10 MHz fiber link from ‘bad’ antenna
slow/fast thermal ramp – phase structure remains the same
probable explanation
fiber photodiode
1. gap acts like Fabry-Perot cavity; increasing temp expands gap, causes periodic variation in laser power at photodiode
2. laser power affects diode capacitance or resistance, hence changes phase of RF signal
substituting APC connector seems to cure the problem
WP02_LOreference
• short term: with 10 MHz thermal problem fixed, reinstall on BIMA in November
• longer term:– test optical circulators?– one laser/antenna to make subarrays easier?– convert to 1550 nm NEC lasers?