On the Improvement of the Phased Array Weather Radar Data
- Advantage and Disadvantage -
Tomoo Ushio, H. Kikuchi, T. Mega (Tokyo Metropolitan University, Osaka University)
- S. Satoh, T. Iguchi (NICT), F. Mizutani, M. Wada (Toshiba)
On the Improvement of the Phased Array Weather Radar Data - - - PowerPoint PPT Presentation
On the Improvement of the Phased Array Weather Radar Data - Advantage and Disadvantage - Tomoo Ushio, H. Kikuchi, T. Mega (Tokyo Metropolitan University, Osaka University) S. Satoh, T. Iguchi (NICT), F. Mizutani, M. Wada (Toshiba) Phased Array
Scan system Elevation: Electronic scan Azimuth: Mechanical scan Coverage 3D scan (100 elevations) / 10 sec (- 1 min) Parameters Zh, vh, σvh (single-polarization)
Antenna (Patch Antenna with RF-CMOS) Control/Signal Processing Units (MMSE algorithm) Terminal data Internet Toshiba NIED etc Warning Users Real time Transfer MP-PAWR Dome
Parabolic Radar Phased Array Radar
→mechanically scanning both in elevation and azimuth
in a certain elevation angle PARABOLIC TYPE ・Fan beam → electrically scan in elevation PHASED ARRAY TYPE
気象学会2018年度秋季大会 C460 5
Zh V Zdr φdp Kdp ρhv
Zh Vh Zdr ρhv
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Clear Sky (2018/08/02 12:00) Rainy (2018/07/28 16:00)
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Clear Sky (2018/08/02 12:00) Rainy (2018/07/28 16:00)
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The received signal from precipitation is seriously contaminated by the relatively high received power from ground and strong precipitation echoes near by through the side lobes of the 2 way beam pattern.
Strong Ground Clutter
Transmitting Broad Beam
High side lobe level from the two way beam pattern
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1 , 1 , 1 , ´
N T l M l l l
1 , 1 , 1 , ´
M T l M l l l
T d M j d j
l p q l p
cos ) 1 ( 2 cos 2
unknown known
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M N N ´
2 1
1 ´
N
unknown known
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1 , 1 , 1 ,
´
M l M l l l
1 1 1 ´
N N m
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m m
m
n
m n
Origin Amplitude Phase Shifter
2
H MMSE m m
m
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Lower sidelobes
m
2
m H MMSE H MMSE m m
m m
(λ: Lagrange Multiplier)
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Lower sidelobes Preserve power in main lobe
m
m
1 1 m m H m MMSEm
v H x
x
v
2
m H MMSE H MMSE m m
m m
18
1 1 m m H m MMSEm
v H x
x
v
2
m H MMSE H MMSE m m
m m
19
1 1 m m H m MMSEm
v H x
x
l H BF BF
m m l
,
v
Beam former method
2
m H MMSE H MMSE m m
m m
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1 1 m m H m MMSEm
v H x
x
1 ) ( 1 ) ( ) ( m i m H m i MMSE i
m
v
2
m H MMSE H MMSE m m
m m
21
l H BF BF
m m l
,
l MMSE i i MMSE
m H l
) ( ) (
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1 1 m m H m MMSEm
v H x
x
1 ) ( 1 ) ( ) ( m i m H m i MMSE i
m
v
2
m H MMSE H MMSE m m
m m
22
l H BF BF
m m l
,
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1) Initialization (i=0) As a prior information, FR solution is calculated.
, 1 , 1 ,
l M l l l
m m FR m
, l H m l m
2) Determination of MMSE weights
1 2 m v H i x i m i m
4) Computation of MMSE solution and Re-iteration
1 , 1 , 1 , 1
+
i l M l l i l
1 , l i H m i l m
+
3) Gain control
i m i m
1
DBF Results
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MMSE-4 MMSE-1 Capon (CP) Fourier (FR) Truth Precipitation Clutter
MMSE FR method Corrected MMSE
FR:elv=0° FR:elv=3° FR:elv=5° MMSE:elv=0° MMSE:elv=3° MMSE:elv=5° MMSE with correction elv=0° MMSE with correction elv=3° MMSE with correction elv=5°
MMSE method FR method Corrected MMSE Clear Sky Rainy Condition
Filtered image (0 deg. ) 除去なし
Original image
Kikuchi et al. IEEE TGRS, 2017
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