Log #DPP16-2016-001807
Abstract Submittedfor the DPP16 Meeting of
The American Physical Society
Sorting Category: 6.1 (E)
Microwave Imaging Radar Reflectometer System Uti-lizing Digital Beam Forming1 FENGQI HU, MEIJIAO LI, CALVINW. DOMIER, XIAOGUANG LIU, NEVILLE C. LUHMANN, JR., Uni-versity of California, Davis — Microwave Imaging Reflectometry is aradar-like technique developed to measure the electron density fluctua-tions in fusion plasmas. Phased Antenna Arrays can serve as electron-ically controlled “lenses” that can generate the required wavefronts byphase shifting and amplitude scaling, which is being realized in the dig-ital domain with higher flexibility and faster processing speed. In thetransmitter, the resolution of the phase control is 1.4 degrees and theamplitude control is 0.5 dB/ step. A V-band double-sided, printed bowtie antenna which exhibits 49% bandwidth (46 - 76 GHz) is employed.The antenna is fed by a microstrip transmission line for easy impedancematching. The simple structure and the small antenna are suitable forlow cost fabrication, easy circuit integration, and phased antenna ar-ray multi-frequency applications. In the receiver part, a sub-array of 32channels with 200 mil spacing is used to collect the scattered reflectedsignal from one unit spot on the plasma cutoff surface. Pre-amplificationis used to control the noise level of the system and wire bondable compo-nents are used to accommodate the small spacing between each channel.After down converting, base band signals are digitized and processed inan FPGA module.1U.S. Department of Energy Grant No. DE-FG02-99ER54531
Prefer Oral SessionX Prefer Poster Session
Fengqi [email protected]
University of California, Davis
Date submitted: 15 Jul 2016 Electronic form version 1.4
F. Hu, M. Li, X. Liu, C.W. Domier, and N.C.Luhmann, Jr.Microwave Imaging Radar Reflectometer Transceiver System Utilizing Digital Beam Forming
Davis MM-wave Research Center (DMRC), University of California at Davis
Antenna Design and Testing
Disadvantages: Slow to adjust; Suffer from reflections from lenses; Lack flexibility
Power Divider
AntennaArray
LO
LO
LO
Pre-amp
55 ~ 75 GHz
0.5 ~ 9 GHz5 MHz
Conceptual Schematic of MIR system
Beam Shaping through Remote Control of Optics in current system
Phased array synthesis integrating optical simulation
Initial complex weight multiply stage with Xillinx 7 hardware co-simulation
Integrated RF board under fabrication
θ1/e’z
z=0
θ1/e
Focal Change
Antenna Array
30 cm
w0
Quadratic wavefront for focused beam
LensCylindrical Lens Optical simulation was used
to obtain the corresponding Gaussian beam waist along with the waist moving range required for refocus. The required array size and corresponding magnitude and phase coefficients for each channel are then calculated for different focusing scenarios
Far field pattern of an N=29 array with Gaussian taper to achieve a Gaussian beam with 22 mm beam waist
Magnitude and phase coefficients for a 10 cm axial focal shift
A 12 channel complex weight multiply stage is modeled in Simulink and programed into Xilinx V707 evaluation board. The plot on the right shows the hardware co-simulation results of the 12 channel array looking at broadside
Optical lenses in current system are used to collect scattered wave from cutoff layer and focus the reflected beam onto the receiving antenna array with the capability of shaping a curved wave-front over a certain spatial range into a flat one.
Microwave Imaging Reflectometry (MIR) is a radar-like system developed to measure electron density fluctuations in fusion plasmas
Multi_Frequency DBF Transmitter/Receiver System
Proof of principle lab test with W band dual dipole antenna
Side view (a) and top view (b) of the receiver optical system
Side view (a) and top view (b) of the transmitter optical system
Advantage of the DBF:
• Flexibility & accuracy• Data memory allowed • Long term stability• Ease of phase & amplitude
adjustment• Easy circuit integration
(a)
𝑊𝑊0
𝐿𝐿0𝐿𝐿1
𝑊𝑊1
𝑊𝑊2
𝑊𝑊3
𝑊𝑊4
𝐿𝐿2
𝐿𝐿3
𝐿𝐿4(b)
HDPE mini lens
Antenna
(a) Antenna geometry (b) Antenna structure with the mini-lens
Antenna’s test setup inside and outside anechoic chamber.
Photograph of the antenna with Zoom in (scale bar 0.5 mm)
-35
-30
-25
-20
-15
-10
-5
0
-30 -20 -10 0 10 20 30
Nor
mal
ized
Rad
iatio
n Pa
ttern
(dB)
Angle (Degrees)
45 GHz55 GHz65 GHz75 GHz
Measured E-plane far-field patterns.
55 GHz ~ 75 GHz
Phase shift
LO
28~32 GHz
Mixer Power Amp
IF1 IF2
Sub harmonic Mixer
Sub harmonic Mixer
Sub harmonic Mixer
Sub harmonic Mixer
65 GHz
16 Elements
0.5 GHz ~ 9 GHz
14 ~ 16 GHz
DDSI Q1 GHz
X2
X21to4 Divider(14-16GHz)
4 of 1to4 Dividers
(28-32GHz)