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F.S. Marzano – Microwave Radar Meteorology: foundations and applications
MICROWAVE RADAR METEOROLOGY
Foundations and Applications
MICROWAVE RADAR METEOROLOGY
Foundations and Applications
Frank S. MARZANODept. of Information Engineering
Sapienza University of RomeE-mail: [email protected]
Centre of Excellence CETEMPSUniversity of L’Aquila
E-mail: [email protected]
2F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RAINFALL FORECASTA conceptual diagramRAINFALL FORECASTA conceptual diagram
Satellite Sensors
Hydrogeological Forecast
341 346 351 356 361 366 371 376 381
4677.6
4682.6
4687.6
4692.6
4697.6
4702.6
4707.6
4712.6
4717.6
longitude
latitude
Orografia
AQ
PR
AS
CA
500
1000
1500
2000
2500
Atmospheric Forecast
Rain Gauges
Weather Radars
3F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RAINFALL SENSINGPoints of view
RAINFALL SENSINGPoints of view
Za [dB]Radar(activeMW)
TA [K]Radiometer
(passiveVIS-IR-MW)
Rain gauge
R [mm/h]
4F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR METEOROLOGYLecture’s contents
RADAR METEOROLOGYLecture’s contents
Radar sensor• Pulsed, Doppler, and polarimetric systems• Receiver sensitivity, antenna specifications and radar volume resolution
Radar equation• Atmospheric refraction and attenuation• Radar equation for single and distributed scatterers
Radar signal• Signal statistics and decorrelation• Noise reduction techniques
Radar applications• Clouds and precipitation• Rainfall backscattering and polarimetric measurables
Radar products• Radar measurements and error budget• Examples of radar measurements and estimates
5F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR METEOROLOGYHistorical perspective
RADAR METEOROLOGYHistorical perspective
Radio era• 1886: H. Hertz experiments e.m. wave reflection• 1902: G. Marconi carries out radio-propagation experiments• 1922: object detection with continuous wave instruments• 1932: object detection with pulsed wave instruments
Radar era• 1938: construction of radars for aircraft detection and ranging• 1941: first use of radars for cloud observations• 1960s: use of radars for quantitative rainfall estimation• 1970s: use of Doppler radars at VHF-UHF for turbulence and wind
Computer era• 1980s: impact of computers on data acquisition and processing• 1990s: use of digital receivers and pulse forming• 1990s: use of radars for weather nowcasting• 2000s: spaceborne radars and sensors’ synergy
6F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR METEOROLOGYContext and objectivesRADAR METEOROLOGYContext and objectives
Radar (RAdio Detection and Ranging)• Pulsed incoherent and coherent radars (Doppler or MTI)• Continuous-wave and frequency modulation (FM-CW)
Meteorological radars• Rain (weather) radars: rainfall monitoring from ground and space• Cloud radars: cloud monitoring from ground and space• Stratosphere-Troposphere (ST) radars: wind profiling from ground
Weather (rain) radars• Monitoring of three-dimensional (3-D) structure of rainfall and winds
• Covering large areas (100-400 km) around ground site• Measuring of e.m. backscattering due to cloud hydrometeor volumes
• Advantages with respect to: • optical sensors (e.g, higher penetration, any meteo condition)• radiometers (e.g., ranging capability, )• rain-gauges (e.g., larger effective coverage, rain structure)
• Disadvantages: high power, complexity, maintenance
7F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR METEOROLOGYA system approach
RADAR METEOROLOGYA system approach
Radar Control
Processor
Radar Transm.
Unit
Radar Receiver
Unit
Radar Signal
Processor
Antenna Pedestal
Unit
ServoSystem
Unit
Backup Power Unit
Radar Antenna Unit Sensor Sub-
system
Processor Sub-system Radar
Data Processor
RadarArchive
8F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR METEOROLOGYLecture’s contents
RADAR METEOROLOGYLecture’s contents
Radar sensor• Pulsed, Doppler, and polarimetric systems• Receiver sensitivity• Antenna specifications• Radar volume resolution
Radar equation• Atmospheric refraction and attenuation• Radar equation for single and distributed scatterers
Radar signal• Signal statistics and decorrelation• Noise reduction techniques
Radar applications• Operational problem overview• Clouds and precipitation• Rainfall backscattering and polarimetric measurables• Example of radar measurements and estimates
9F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR SENSORPulsed microwave systems
RADAR SENSORPulsed microwave systems
Principle• Send a train of short, high-power pulse
of e.m. energy at high frequency (GHz)• E.m. energy, captured by atmospheric
objects, is partially absorbed and re-irradiated (scattered) into manydirections among which that of radar (backscattered: radar echo)
• Angular resolution: derived from the antenna pointing direction and limitedby its beam width
• Range resolution: derived from the two-way time employed by radar pulse echo(antenna-object-antenna) and dependingby medium light velocity
Legenda• PRF: Pulse Repetition Frequency• RF: Radio Frequency (f0)• PP: Peak-to-peak power• Pt: Peak power of the transmitter
Tc
10F.S. Marzano – Microwave Radar Meteorology: foundations and applications
Tx
Rx
Antenna
r
t=0t=r/ct=2r/ct=2r/c+
RADAR SENSORPrinciple of pulsed systems
RADAR SENSORPrinciple of pulsed systems
11F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR SENSORPrinciple of operation
RADAR SENSORPrinciple of operation
r
2cr
Range resolution
2maxccTr
Maximum unamb. range
1c
r Tf
Repetition frequency
Typical values:f0 3-90 GHz; Pt 100-1000 kWfr 250-2500 Hz; 0.1-2.5 s Time
cdPT
PP tc
tavg
Average TX Power
12F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR SENSORPulsed incoherent scheme
RADAR SENSORPulsed incoherent scheme
sRF
xRF
xIF
xBB
xmix
2|)(|)( tatxBB
13F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR SENSORPulsed incoherent system
RADAR SENSORPulsed incoherent system
Radar components• Master oscillator (MO): system reference oscillator• Modulator: device which determines the form e repetition of RF pulse• Power oscillator: microwave tube (magnetron or klystron amplifier)• Duplexer: 3-port circulator which separates TX from RX signal• Local oscillator (LO): device which controls mixer frequency• Mixer: device which mixes RF signal with LO doing amplification and filtering• Amplifier: band-pass amplifier and filter for noise reduction of IF signal• Video detector: detector of IF envelope power at baseband
Signal processing
22
00
0
0
)()()(
)(2cos)( )(2cos2
)()(
2cos )(2cos)()()(2cos)()(
)()2cos()(
tatxtx
ttftattfbtatx
tffbttftatxttftatx
tfrecttfAts
IFBB
ccIF
cmix
RF
rRF
Transmitted Radio Frequency (i.e., GHz)
Received Radio Frequency
Mixer signals
Intermediate Frequency (i.e., MHz)
Base-band signal (i.e., kHz)
14F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR SENSORDoppler frequency shift
RADAR SENSORDoppler frequency shift
000
cosˆ
uuf rd ru
(a)
(b)
u
u
Range vector
Velocity vector
00
0ˆ22
ru
rd
dRFuf
fff
If leaving target: </2 fd < 0
If approaching target: >/2 fd > 0(a) Stationary source
(b) Moving source
u
(wave movingin directionopposite to thatof the source)
(wave movingin the samedirection asthe source)
Doppler frequency shift
Monostatic Radar Twice a Doppler frequency shift- from radar to target- from target to radar
15F.S. Marzano – Microwave Radar Meteorology: foundations and applications
Per poter determinare la velocità Doppler del bersaglio puntiforme devo usare un
RICEVITORE COERENTE
A cos[t +] Cos[t] (COHO)
/2
I(t) = A/2 cos[] Q(t) = A/2 sen[]
RADAR SENSORPulsed coherent scheme
RADAR SENSORPulsed coherent scheme
16F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR SENSORPulsed coherent scheme
RADAR SENSORPulsed coherent scheme
xBB
sRF
xIF
xmix
)()()(with
)(sin)()()(cos)()(
)(
tjQtItVttatQttatI
txBB
)(2)(
)(2 )(4)(
)(22)(
tutf
tftudt
td
trt
rd
dr
Doppler frequency
17F.S. Marzano – Microwave Radar Meteorology: foundations and applications
• L’eco radar è la somma di tanti contributi elementari del tipo vistoin precedenza (impulso rettangolare a RF)
Bersaglio puntiforme
Bersaglio distribuito
t
t
VRx
• L’atmosfera è un bersaglio distribuito, ossia è costituita da un elevato numero di bersagli elementari (idrometeore)
RADAR SENSORPulsed coherent scheme
RADAR SENSORPulsed coherent scheme
18F.S. Marzano – Microwave Radar Meteorology: foundations and applications
t0
t
VRx
L’eco ricevuto all’istante t0 è la somma dei contributi di tutti i bersagli elementari che si trovano ad una distanza dal radar compresa tra c (t0-)/2 e c t0/2
Il segnale ricevuto viene prima campionato (nel GPM-500C con una frequenza di 2.4 MHz, ossia ogni 417 ns) e quindi i campioni vengono processati.
Ogni campione è rappresentativo di un volume elementare (tronco di cono) con altezza pari a (c )/2
RADAR SENSORPulsed coherent system
RADAR SENSORPulsed coherent system
19F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR SENSORPulsed coherent system
RADAR SENSORPulsed coherent system
Detection of received signal phase
Signal processing
)()()( with
)(sin)()()(cos)()(
)(
]e)e([Re]e[Re2sin)(-2cos)()(
2sin)(sin)(- 2cos)(cos)( )(2cos)()(2cos )()(2cos)()(
)(222cos)()(2cos)()(
)()2cos()())(2cos()(
cj2)(jcj2
00
00
00
tjQtItVttatQttatI
tx
tajQ(t)I(t)tftQtftItx
tfttatfttattftatxtfbttfftatx
trtftattftatx
tfrecttfAtfrecttffAts
BB
tftttfccIF
cccIF
cmix
RF
rrcRF
)(2)( )(2 )(4)(4)( )(22)( tutftftudt
tdrdt
tdtrt rddr
20F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR SENSORDoppler velocity ambiguity
RADAR SENSORDoppler velocity ambiguity
Signal sampling (Shannon) theorem• A signal with a finite energy (a maximum
spectral frequency fM) is reconstructed from its temporal samples if the sampling frequency fs:
Unambiguous Doppler frequency• If maximum frequency is fr:
• Velocity-range limit
Ambiguity reduction techniques• Doppler phase measured between 2 pulses• Dual-PRF: double of unanmbiguos fd• Phase and polarization pulse coding
2
2
sM
sM
TTff
4
2 maxmax
rr
rdd fufff
8/)(]2/)][4/)[maxmax ccTfru crr
21F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR SENSORIssues on coherent systems
RADAR SENSORIssues on coherent systems
Microwave transmitter• MAGNETRON: self-oscillating microwave tube with cylindrical structure (cross-field device), able to
handle high power (up to 2000 kW peak). A high (up to 50 kV) DC voltage is applied to coaxial cathode (+) and anode (-) together with a static magnetic high field (up to 1 A/m). The emitted electron beam is spatially modulated (bunches) and output is coupled into one of ring resonant cavities. The latter determines the radio-frequency (RF) signal. Oscillation condition is governed by Hartree’s curve. Overall efficiency is about 50%.
• When input voltage is pulsed (as in radars), no inter-pulse coeherence is guaranteed (even though phase information may be retained by injecting a CW signal).
• KLYSTRON: microwave-tube amplifier with a linear (linear-field) structure, able to handle medium power (up to 1000 kW). An electron beam is formed by an electron gun (thermoionic emission by cathode-anode at > 1000 K), passes trhough 2 or more resonant cavities in succession and is collected on a collector. Electric field of first cavity gaps induce electron bunches whose are “focused” on (load) resonant cavities which produce output RF signal.
• Within pulsed radars, klystron is used as an amplifier excited by a local microwave oscillator. These scheme guarantees a high phase purity (low phase noise) and an inter-pulse coherence.
Base-band detection• Amplitude: logarithmic detector in order to deal with large amplitude (i.e., a’(t)) dynamics.• Phase: linear detector to extract in-phase I(t) and quadrature Q(t) components
22F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR SENSORE.m. wave polarization
RADAR SENSORE.m. wave polarization
Polarization statesCurve described in 3-D space by the free end of the mono-chromatic wave vector• Horizontal H (w.r.t. ground)• Vertical V• Circular (LHC, RHC)
Linear polarizations
)(2cos)(),( 00 ttftEtrE p
xtEtEztEtE
hh
vv
ˆ)()(ˆ)()(
00
00
23F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR SENSORIssues on polarimetric radars
RADAR SENSORIssues on polarimetric radars
Configuration• Alternate transmission
• Single-transmitter and single-receiver• Alternate transmission between H and V fields Single receiver Anomalous propagation removal Polarization switching H and V non-contemporary data
• Simultaneous transmission• Single transmistter and dual receiver• Simultaneous transmission of H and V fields No polarization switching (costly and loss) No delay in H and V acquisition data Fast scanning (half time w.r.t. alternate trans.) Cross-polarization effects in received data Dual receiver and limitation in polarimetric features
Receiver• Digital receiver at IF stage
• Sampling of IF signal (A/D digitizers) • Digital processing of binary I/Q sequences
E0V
E0H
Time
H V H V H V
Time
H,V H,V H,VH,V H,V H,V
E0V
E0H
E045
24F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR SENSORAlternate polarim. system
RADAR SENSORAlternate polarim. system
H/V Orth. Transd.
H/V ChannelDigital Receiver
Microwave TX
Coh. Oscill.
V channel H channel
Elevation rotary joint (V)
Elevation rotary joint (H)
Azimuth rotary joint
IF Mixer
Co-processor (vm, v, ZH, ZDR, DP, HV, LDR)
Antenna reflector
Feed
H/V Polariz. Switch
Circulator
I(H,V) Q(V,H)
25F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR SENSORSimultaneous polarim. system
RADAR SENSORSimultaneous polarim. system
H/V Orth. Transd.
V ChannelDigital Receiver
H ChannelDigital Receiver
Microwave TX
Coh. Oscill.
V channel H channel
Elevation rotary joint (V)
Elevation rotary joint (H)
Azimuth rotary jointV channel H channel
Circulator
IF Mixer IF Mixer
Co-processor (vm, v, ZH, ZDR, DP, HV )
Antenna reflector
Feed
CirculatorPh./Amp. Contr. Ph./Amp. Contr.3-dB Power Div.
Q(V)I(V) Q(H)I(H)
26F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR SENSORReceiver sensitivity
RADAR SENSORReceiver sensitivity
Noise sources• cosmic, artificial (human) and atmospheric emission (H20, 02 at MW)• internal, due to electron thermal mobility (white Gaussian noise at MW).
Internal noise of receiver• Receiver input power with a resistance load at T0 and bandwith Bn: Ni=kT0Bn• Noise figure Fn or equivalent noise temperature Te: Te=T0(Fn-1)
Minimum detectable signal• Minimum signal detectable over the noise receiver (e.g., -110 dBm = 10-11 mW)
• Matched filters to increase S/N: for square pulses. Bn1/ and triangular shape
N0=Fn(GNi )= k(T0+ Te)BnNi=kT0Bn Radar receiverG, T0 , BnSi S0 =GSi
Minnn
MininiMin
iin N
SBkTFNSNFS
NSNSF
0
00
0
0
00)(
//
27F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR SENSORAperture antenna basics
RADAR SENSORAperture antenna basics
Radar antennas• Parabolic reflector antenna• Prime-focus feeder (horn)• Optional radome protection• Optional polarization capability
Antenna radiation• Radiation pattern function
• Irradiated eletric far-field (for rL2/)
• Power flux density [W/m2]
),(),( yxEFFTf a
refErE
jkr ),(),,( 0
22
0
02
0),(
2),,(
21),,(
f
rErErP
L
28F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR SENSORAntenna parameters
RADAR SENSORAntenna parameters
Directivity and Gain
Effective area
Beamwidth (reflector antennas)
Polarization capability• Ortho-Mode Transducer (H/V) at horn feeder• Low sidelobes (<30 dB) similar for H/V patterns• Isolation between H/V patterns (no cross-pol.)
• Azimuthally symmetric radiation pattern at H/V• Effects of supporting struts and radome paneling
),(),( ,4/
),(4/
),,(),(2
2
DG
Wf
rWrPD r
TT
22
),(),(4),,(
),(
nM
i
Re fDD
rPWA
23
32
3 )(4 ,70 5.0),2/(
dBMdBdBn D
Lf
29F.S. Marzano – Microwave Radar Meteorology: foundations and applications
Example: Radar GPM-500C
Cassegrain dual-offset
- fascio di 0.9° (a -3 dB)- velocità max 30 deg/s- lobi secondari molto bassi- ottima simmetria tra H e V
RADAR SENSORAntenna parameters
RADAR SENSORAntenna parameters
30F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR SENSORAntenna diagramRADAR SENSORAntenna diagram
Example: Radar GPM-500C
Cassegrain dual-offset
- fascio di 0.9° (a -3 dB)- velocità max 30 deg/s- lobi secondari molto bassi- ottima simmetria tra H e V
31F.S. Marzano – Microwave Radar Meteorology: foundations and applications
(c )/2
RADAR SENSORVolume resolutionRADAR SENSOR
Volume resolution
32F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR SENSORVolume resolutionRADAR SENSOR
Volume resolution
Spatial resolution• Capability of discriminating 2 objects in space (range,
zenith and azimuth in spherical coordinates)
Radial resolution• Resolution in range:
• Matched receivers have a lower radial resolution• Use of pulse compression to increase spatial res.
Transverse resolution• Resolution in zenith-azimuth:
• Affected by side lobes contribution.
2cr
3dB22
2 rrSrS
rr
3dB
S
Pulse volume resolution
• Volume varies with range (for 1° and 1 s, at 100 km r=150 m and S=17452 m2 )• Energy volume distribution can be not uniform in range (e.g., matched filters) and in
transverse direction (e.g., directivity angular variation)
dBdBbin rcrcSrV 332
3dB2 )2/(
4)2/(
3dB
33F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR METEOROLOGYLecture’s contents
RADAR METEOROLOGYLecture’s contents
Radar sensor• Pulsed, Doppler, and polarimetric systems• Receiver sensitivity• Antenna specifications• Radar volume resolution
Radar equation• Atmospheric refraction and attenuation• Radar equation for single and distributed scatterers
Radar signal• Signal statistics and decorrelation• Noise reduction techniques
Radar applications• Operational problem overview• Clouds and precipitation• Rainfall backscattering and polarimetric measurables• Example of radar measurements and estimates
34F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR EQUATIONAtmospheric refraction
RADAR EQUATIONAtmospheric refraction
Atmospheric refractivity• Refractive index:
• Refractivity:
Optical rays• Geometrical optics equation:
with ray curvature.• If standard atmosphere, dN/dz=-40 [N/km]
• Earth effect. radius Re=4/3RT=4/3(6370)=8500 • Rays are rectilinear and Earth flatter
Specific attenuation• For two-way path, the attenuation factor L:
Atmosphere with N0=313 and H=7 km
HzeNN(z)dzdN
n/
0
6 ,cos101
z
x
njnvcn r
)/,/(10)1( 26 TeTpfnN
)() 2 20
020 rLWeWW(rWdrdW drr
35F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR EQUATIONSingle scatterer form
RADAR EQUATIONSingle scatterer form
Power flux density upon scatterer
Backscattering radar cross section
Received power
Radar equation for a single scatterer
• For a point target, fn=1 and WR1/r4. Constant C1 depends on radar specs.
)(),(4
),,( 22 rLfG
rWrP nM
Ti
),,(),,(4),,,( 2
rPrPr
i
rb
Pi
b
WT,GM
Pr
WR, fn
L
rreRnMTb
ib
r GPPAWLfGr
WLr
Pr
rP
4444
22
222 ),(),,(
r
r4r)4(),(
42
14
2
2
22
4
2
3
242b
RberT
bnMT
R LCWLr
AWLfGWW
36F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR EQUATIONEffect of distributed scatterer
RADAR EQUATIONEffect of distributed scatterer
Distributed scatterers• Set of a large number Npart of equal-size scatterers, simultaneously
present in the same resolution volume Vbin with randomlydistrubuted phase and totally filling the volume ( e.g. raindrops).
• Volumetric reflectivity [m-1]
Particle and total received power
Pi
Pr
WR, fn
LWT,GM dV
dVdV
dV
partpartpart Ni bi
N
ibi
Ni bi
1
1
1 Vbin
RVn
VRRtot
nN
ibi
nN
ibi
nN
iRiR
bin
binMT
Ri
WdVLf
CdWW
dVLf
CdVdVL
fCL
fCdWdW
Lf
CfGWdW
bin
partpartpart
24
24
1
24
1
24
1
244
3
22
4
4444i
4i4i
r ),( r ),(r ),(r ),( r ),(r ),()(
37F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR EQUATIONDistributed scatterer form
RADAR EQUATIONDistributed scatterer form
Distributed scatterers• Set of a large number of scatterers, simultaneously present in the
same resolution volume Vbin with randomly distrubuted phase and totally filling the volume ( e.g. raindrops).
Total (average) received power
Radar equation for volume scattering
Pi
Pr
WR, fn
LWT,GMVbin
volumeresolutionradardrdrdV
df
rLGWdVf
LGWWbinbin V
nMTV
nMTR :V ),( where r ),()(r ),()(
bin24
2
42
3
2242
3
22
44
)( lnr ),( correction Jones-Probert2 281 33
2
4
dBdBV
n
rd
f
281
433
22
3
22 ln)( dBdBMTR r
rLGWW
22
2 rLCWR
38F.S. Marzano – Microwave Radar Meteorology: foundations and applications
Q
I
RADAR SIGNALSignal fluctuations
RADAR SIGNALSignal fluctuations
Power fluctuations of radar echo• Complex envelope due to i-th scatterer:
• Total complex envelope due to distributed scatterers:
• In-phase and quadrature components
Radar echo power
• From one pulse to next, power fluctuation Wac are related to scatterer random displacement (velocity or Doppler frequency).
• It results <Wac>=0 and Wac decreases doing averages on independent samples (such that displacement > ). For estimating , samples must be correlated to avoid ambiguity.
iiitij
ii trteAtV /)(4)( ,)( )(
)()( )()()()()( tji
tijii i etAeAtVtjQtItV
IQartgQIA
ttAtVtQttAtVtI
, with )(sin)()](Im[)()(cos)()](Re[)( 22
RR
RacRdcji
rrjjii iR WW
WWeAAkAktAtVtkV(t)W ji ~)()()( ))(/(* 422
39F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR SIGNALStatistics of power fluctuations
RADAR SIGNALStatistics of power fluctuations
Distribution of I, Q• For the central limit, V(t) is Gaussian so that I and Q• A and are independent random variables with uniformly distributed in 0-2
Marginal distribution of A,
Square-law detector statistics of received power
AdAddIdQdAdApp(I,Q)dIdQeQIp QI ,),( ,2
1),(22/)22(
2
pdf Uniform 2/1)(
pdfRayleigh 2
)(
2),(
22/2
22/2
p
eAApeAAp
AA
pdf tial Exponen2
1)p(W p(A)dA)dWp(W ,2 ,22/
2RRR2
RW
RR eAdAdWAW
40F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR SIGNALDecorrelation time
RADAR SIGNALDecorrelation time
Dopppler spectrum• Duration td needed to ensure sample
independence depends on volume and wavelength
• Doppler spectrum is of Gaussian type for uniform regions:
• Time autocorrelation function:
Decorrelation time tinc
u fepf rdfdf )/2( ;)p(22/2
0d
uft
tdtd eRR(t
)/2(21
21,)
22/20
vincinc tRR(t /2 02.0/) 0
Snow: u=0.5 m/sRain: u=1 m/s
41F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR SIGNALTime-space data integration
RADAR SIGNALTime-space data integration
Signal variance reduction• For meteorological appliatio, Wdc is of
interest so that Wac must be reduced• How many independent samples of received
power must be averaged to accurately estimate Wdc=<W> using a square-law detector?
• The final pdf is almost Gaussian for k>10• For k=30, <W> error estimate is about 1 dB
Spatial integration• For fast scannig, spatial averaging is
performed together with time integration• Reduction of measurement spatial
resolution (e.g., range similar to transverse)
)()()( with 22
1
1nnkk
k
nRnk AdApdJJpW
kJ
42F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR METEOROLOGYLecture’s contents
RADAR METEOROLOGYLecture’s contents
Radar sensor• Pulsed, Doppler, and polarimetric systems• Receiver sensitivity• Antenna specifications• Radar volume resolution
Radar equation• Atmospheric refraction and attenuation• Radar equation for single and distributed scatterers
Radar signal• Signal statistics and decorrelation• Noise reduction techniques
Radar applications• Operational problem overview• Clouds and precipitation• Rainfall backscattering and polarimetric measurables• Example of radar measurements and estimates
43F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR APPLICATIONSClouds and precipitationRADAR APPLICATIONS
Clouds and precipitation
Genus Sym. Region Species RR (mm/h)
Cumulus Cu Vert. develop.(0-6 Km)
MediocrisCongestusIncus
0< 30< 60
Cumulonimbus Cb Vert. develop.(0-12 km)
10÷100
Stratus St low(0-2 km)
< 2
Stratocumulus Sc low(0-2 km)
< 5
Nimbostratus Ns middle(2-6 km)
< 15
Altostratus As middle(2-6 Km)
< 2
Altocumulus Ac middle(2-6 km)
0
Cirrostratus Cs high(6-12 km)
0
Cirrocumulus Cc high(6-12 km)
0
DYNAMIC METEOROLOGYAir mass flows and windsDYNAMIC METEOROLOGYAir mass flows and winds
44F.S. Marzano – Microwave Radar Meteorology: foundations and applications
DYNAMIC METEOROLOGYCirculating cells
DYNAMIC METEOROLOGYCirculating cells
45F.S. Marzano – Microwave Radar Meteorology: foundations and applications
DYNAMIC METEOROLOGYCyclones and anticyclonesDYNAMIC METEOROLOGYCyclones and anticyclones
46F.S. Marzano – Microwave Radar Meteorology: foundations and applications
CLOUD GENERAWarm fronts
CLOUD GENERAWarm fronts
47F.S. Marzano – Microwave Radar Meteorology: foundations and applications
CLOUD GENERACold fronts
CLOUD GENERACold fronts
48F.S. Marzano – Microwave Radar Meteorology: foundations and applications
CLOUD FRONTSCold, warm and occluded
CLOUD FRONTSCold, warm and occluded
49F.S. Marzano – Microwave Radar Meteorology: foundations and applications
50F.S. Marzano – Microwave Radar Meteorology: foundations and applications
PRECIPITATING CLOUDSTime and space scales
PRECIPITATING CLOUDSTime and space scales
CHARACTERISTIC TIME1 day- 1 month 1 hour – 1 day 1 hour – 1 minute
200 - 2000 km - Fronts- Hurricanes(tens of days)
Meso- scale
20 - 200 km - Squall lines- Cloud clusters- Mountain andlake disturbances(2 hours to 1 day)
Meso- scale
2 - 20 km - Thunderstorms(tens of minutes tohours)
Meso- scale
0.2 - 2 km - Tornadoes- Deep convection(few minutes to 1hour)
Micro- scale
0.02 - 0.2 km - Thermals(few minutes)
Micro- scale
HORIZONTAL
SCALE 0.001 - 0.02 km - Plumes
- Turbulence(less than afew minutes)
Micro- scale
51F.S. Marzano – Microwave Radar Meteorology: foundations and applications
Melting
Ice formation
PRECIPITATING CLOUDSStratiform process
PRECIPITATING CLOUDSStratiform process
Aggregation0° C
1 km
0.5-1 kmHei
ght
Cloud Top~ 4-7 km
Surface
Rainfall
52F.S. Marzano – Microwave Radar Meteorology: foundations and applications
As for droplets (condensation/evaporation), ice crystals can initially grow by vapor deposition and evaporate by sublimation. The probability of presence of ice particles in a cloud increases with decreasing temperature below zero. At -10ºC the probability to find ice is around 50%, while at -20 ºC it raises to 95%.
Main ice crystal shapes are: (a) columnar or prismatic, (b) disc, (c) dendrite
PRECIPITATING CLOUDSIce crystals
PRECIPITATING CLOUDSIce crystals
53F.S. Marzano – Microwave Radar Meteorology: foundations and applications
PRECIPITATING CLOUDSConvective process
PRECIPITATING CLOUDSConvective process
Evolutiontime
O° C
t0 t1 t2 t3 t4 t5
Updrafts Downdrafts
~5 kmscale
Particletrajectory
Dissipation~10-15 kmheight
SurfacetN
Evaporation
tN-1
Anvil
54F.S. Marzano – Microwave Radar Meteorology: foundations and applications
Natural graupels (boxes are 2 mm on a side)
GRAUPEL FORMATION BY RIMING •Ice crystals fall through supercooled cloud droplets•Supercooled droplets, that hit ice crystals, freeze to it•Eventually the frozen droplet can hide the original shape•Due to strong updrafts, hailstones can form
PRECIPITATING CLOUDSGraupel particles
PRECIPITATING CLOUDSGraupel particles
55F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR APPLICATIONSDrop size distributionsRADAR APPLICATIONSDrop size distributions
Modified Gamma distribution
Moments of order n:
• Drop concentration [#/m3]:
• Equivalent water content [g/m3]:
• Median volumetric diameter [m]:
• Precipitation intensity [mm/h]:
parameters:,,N diameter; drop: with )( 00 DeDNDN D
10
0
)1()(
n
nn
nNdDDNDm
0mNT
3)6/( mM
2/0 MD
mm/h][m/s )6/(/ )(
][kg/m ])()[()6/(
3
2
0
3
b
bt
t
amRRaDDu
sdDwDuDNDR
56F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR APPLICATIONSExamples of size distributions
RADAR APPLICATIONSExamples of size distributions
57F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR APPLICATIONSAtmospheric attenuationRADAR APPLICATIONS
Atmospheric attenuation
[dB/km] )()(4343.00
dDDNDk aa
g: atmospheric gasesc: cloud and icep: rain and graupel (precipitating)t = g + c + p
H20
O2
58F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR APPLICATIONSRadar reflectivity
RADAR APPLICATIONSRadar reflectivity
Volumetric reflectivity of particles with different size
Rayleigh reflectivity and reflectivity factor
Mie reflectivity and equivalent reflectivity factor
• Dielectric factor K Water |K|2=0.930Ice |K|2=0.176Melt |K|2=0.208
m1 )()()()()()(
01
11 dDDNDDNDdV
DNDdV b
Ni iib
Ni ipib
Ni bi D
Dpart
0
6
0
64
25
)( Z )( :D dDDNDdDDNDK
Se
0
25
4
ee4
25)()( Z :D dDDND
KZ
KSe b
59F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR APPLICATIONSExamples of radar reflectivity
RADAR APPLICATIONSExamples of radar reflectivity
Power-law relation: Z=aRb
=
60F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR APPLICATIONSHydrologic relationshipsRADAR APPLICATIONS
Hydrologic relationships
61F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR APPLICATIONSPolarized measurementsRADAR APPLICATIONS
Polarized measurements
Backscattering matrix• The scattering field is related to the incident one by:
• The S matrix is the complex backscattering matrix, whose terms are:
Interpretation and Symmetry• Diagonal terms SHH and SVV represent linear co-polarized components
• SHH : H transmission, H reception• Off-diagonal terms are cross-polarized components
• SVH : H transmission, V reception• For a spherical particles, the cross-polarized terms are zero.• The cross-pol. terms are equal for reciprocity (unless medium is anysotropic).
iv
ih
VVVH
HVHHrj
sv
sh
E
ESSSS
re
E
E
ppjpppp eSS
H-pol.
V-pol.
62F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR APPLICATIONSPolarimetric definitionsRADAR APPLICATIONSPolarimetric definitions
Polarimetric form of radar equation• Radar equation can be generalized to polarimetric form• Complex envelope V will be polarization dependent, i.e. Vpp
Co-polar radar reflectivity (mm6m-3)
Differential reflectivity
Linear Depolarization Ratio (LDR)
)||/( ,)||/( 22542254 VVVVHHHH SKZSKZ
2
210
VV
HHDR
SSLogZ
2
210
HH
VH
SSLogLDR
63F.S. Marzano – Microwave Radar Meteorology: foundations and applications
Oblate ZDR > 0Sphere ZDR = 0Prolate ZDR < 0
RADAR APPLICATIONSPolarimetric examplesRADAR APPLICATIONSPolarimetric examples
2
210
VV
HHDR
SSLogZ
64F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR APPLICATIONSPolarimetric definitionsRADAR APPLICATIONSPolarimetric definitions
Correlation coefficient
Differential propagation-phase shift (°/km)
hvjhv
VVHH
HHVVHV e
SS
SS ||22
*
*
0
0
arg
')'(2
)()]()([Re180
HHVVhv
hv
r
DPDP
D
VVHHDP
SS
drrK
dDDNDfDfK
• Oblate particles tend to slow down H-pol. waves with respect to V-pol. ones• This effect is larger for liquid than ice particles• is due to particle-induced phase shift
65F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR APPLICATIONSPolarimetric definitionsRADAR APPLICATIONSPolarimetric definitions
Specific attenuation (1/km)
One-way path attenuation
• Application
),(Im
efHHHH DS4180102 3
r
HHHH drrrA0
')'()( Attenuation of
backscattered power (due to a range bin)
along the path
Range bin
22
2
22
2
rrZeC
rrZrLCW
HHrA
HHHHRh
HH)(
)()()(
66F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR APPLICATIONSPolarimetric theory
RADAR APPLICATIONSPolarimetric theory
Differential reflecivity vs. ellipsoid axial ratio
Particle density
67F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR APPLICATIONSPolarimetric features
RADAR APPLICATIONSPolarimetric features
68F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR APPLICATIONS Polarimetric advantagesRADAR APPLICATIONS
Polarimetric advantages
69F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR APPLICATIONS Rainfall polarimetric estimators
RADAR APPLICATIONS Rainfall polarimetric estimators
)(
),(),(
dp
drdp
drh
KRR
ZKRRZZRR
),( drh ZZRR From single-pol.
To dual-pol. retrieval
70F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR APPLICATIONMeasurement issues
RADAR APPLICATIONMeasurement issues
h
Zxx(r,,)
Radarbeam
Volumebin
Zsurf(h)?
),,(,,,,
,),,(),,( ),,(),,(φθ22
2
1
φθφθ
φθ1φθ
rAvRhVVHH
R
M
iviRh
pulsevRh
VVHH
pulse
erWrCrZ
NrWM
rW
Dual-pol. radar equation
where PR: received power at h or v pol.C: radar constant, r: rangeA: path attenuation at h or v pol.Z: reflectivity at h-h or v-v pol. NR: noise levelM: number of pulses
Groundclutter
Path attenuation
V pol
H pol
71F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR APPLICATIONSOperational issues
RADAR APPLICATIONSOperational issues
Calibration objective• Determine with precision and accuracy the instrumental constant C in
radar equation equation• Transmistter power, loss of radiofrequency chain (e.g., guides, mixers, couplers)• Noise level in the receiver chain, receiver gain and linear dynamics (no distortions)
Calibration techniques• Internal calibration: measurement of each radar component and module
• Suitable instrumentation (e.g., synthetic pulse generator, network analyzer)• Periodic controls (antenna, TX) vs. frequent controls (oscillators, noise)
• External calibration: measurement of reference radar targets• Large metallic spheres such that b is equal to the geometric section• Rain-gauge time-series data• Difficult measurement set up and ambiguities
• Overall calibration obtainable: 1 dB Ground-clutter contamination
• Spurious echoes backscattered by ground and obstacles• Spectral, statistical and static removal techniques• Coupling with beam occulation, anomalous propagation, reflectivity gradients
72F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR PRODUCTSAn overview
RADAR PRODUCTSAn overview
73F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR PRODUCTSComparison among instruments
RADAR PRODUCTSComparison among instruments
Rete della Regione Piemonte
Rain gauges Meteosat IR
74F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR PRODUCTSComparison among instruments
RADAR PRODUCTSComparison among instruments
Meteosat IR C-band Radar (ARPA-FVG)
75F.S. Marzano – Microwave Radar Meteorology: foundations and applications
Rain field spatially interpolated from rain gauges
Rain field derived from ARPAP C-band radar Range = 125 km
Range = 30 km
RADAR PRODUCTSComparison among instruments
RADAR PRODUCTSComparison among instruments
76F.S. Marzano – Microwave Radar Meteorology: foundations and applicationsx
y
z
elevation12
RADAR PRODUCTSPolar volume scanning
RADAR PRODUCTSPolar volume scanning
Height
E
N
W
Slant Range
S
SCANNING STRATEGYElevation angle : 0-20 with variable stepAzimuth angle : 0-360° with 1° step
77F.S. Marzano – Microwave Radar Meteorology: foundations and applications
x
y
z
1
RADAR PRODUCTSPlan Position Indicator (PPI)
RADAR PRODUCTSPlan Position Indicator (PPI)
Projection on the ground plane of radar 3-D polar data acquired upon a conical surface (constant elevation, azimuth betwen 0° and 360°)
78F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR PRODUCTSExample of PPI
RADAR PRODUCTSExample of PPI
H-pol. Reflectivity at 2° elevation Radial velocity at 2° elevation
79F.S. Marzano – Microwave Radar Meteorology: foundations and applications
x
y
z
N.B. A vertical Section can be obtained by re-processing a 3-D polar volume as well. In this case it is called “Vertical Cut”.
RADAR PRODUCTSRange Height Indicator (RHI)
RADAR PRODUCTSRange Height Indicator (RHI)
RHI: Vertical scan for constant azimuth angle
80F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR PRODUCTSExample of RHI and VCut
RADAR PRODUCTSExample of RHI and VCut
taglio dall’originetaglio dall’origine
taglio qualsiasi
81F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR PRODUCTSConstant Altitude PPI
RADAR PRODUCTSConstant Altitude PPI
0
2000
4000
6000
8000
10000
12000
1 11 21 31 41 51 61 71 81 91 101 111 121 131 141 151 161 171 181 191 201 211 221 231 241
range (km)
heig
ht (m
)
-0.1
0.4
1.2
2.03.04.45.87.410.015.028.5
CAPPI: Horizontal cut of polar volume at a constant altitude
82F.S. Marzano – Microwave Radar Meteorology: foundations and applications
H eight
E
N
W
Slant Range
S
N
E
S
W
H eight
Y
X
H
Volume polare
Volumecartesiano
RADAR PRODUCTSCAPPI processingRADAR PRODUCTSCAPPI processing
83F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR PRODUCTSExample of CAPPIRADAR PRODUCTSExample of CAPPI
84F.S. Marzano – Microwave Radar Meteorology: foundations and applications
0
2000
4000
6000
8000
10000
12000
1 11 21 31 41 51 61 71 81 91 101 111 121 131 141 151 161 171 181 191 201 211 221 231 241
range (km)
heig
ht (m
)
-0.1
0.4
1.2
2.03.04.45.87.410.015.028.5
RADAR PRODUCTSHor.-Vertical Maximu Intensity
RADAR PRODUCTSHor.-Vertical Maximu Intensity
HVMI: Horizontal-vertical projection (3 axes) of maximum reflectivity
85F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR PRODUCTSExample of VMI
RADAR PRODUCTSExample of VMI
86F.S. Marzano – Microwave Radar Meteorology: foundations and applications
78
1. Inhomogenheity of rain cloud withinthe radar beam
2. Evaporation of rainfall below theradar beam
3. Understimation due to orographiceffects on rainfall process
4. Bright-band effects due to meltinglayer
5. Path attenuation due clear-air gases(water vapor and oxygen) and rain
6. Anamolous propagation due to airrefractivity – second-trip echoes
7. Beam screening due to presence ofobastacles (hills, mountains)
8. Calibration erros within the radarsystem
RADAR PRODUCTS Errors in rainfall retrieval
RADAR PRODUCTS Errors in rainfall retrieval
87F.S. Marzano – Microwave Radar Meteorology: foundations and applications
Bright band
Secondary lobes effect
Anomalous propag. Multiple reflections
Ground clutter
RADAR PRODUCTSExamples of radar artifacts (1)
RADAR PRODUCTSExamples of radar artifacts (1)
88F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR PRODUCTS Examples of radar artifacts (2)
RADAR PRODUCTS Examples of radar artifacts (2)
stratiform
convective
stratiform
convective
Profilo verticale di riflettività
Bright Band
Estimate of surface rainfall from stratiform or convective Z-R relation ?
89F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR PRODUCTS Examples of radar artifacts (3)
RADAR PRODUCTS Examples of radar artifacts (3)
Max. unamb. velocoty: umax= ±16m/sMode: single PRF=1180 Hz
Max. unamb. velocoty: umax= ±32m/sMode: dual PRF=1180 Hz, 787 Hz
90F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR PRODUCTS Examples of radar artifacts (4)
RADAR PRODUCTS Examples of radar artifacts (4)
C-band radar: affected by rain path attenuation S-band radar: immune to rain path attenuation
91F.S. Marzano – Microwave Radar Meteorology: foundations and applications
radar volume rain rate estimation
Clutter, ana-prop., vel.correction
VPR, atten. correction
raingauge data spatial interpolation
ErrorEstimation
RADAR PRODUCTSRadar data processing
RADAR PRODUCTSRadar data processing
92F.S. Marzano – Microwave Radar Meteorology: foundations and applications
Radial velocity
Z uncorrected Z corrected
Spectral filter
RADAR PRODUCTSExample of data processing
RADAR PRODUCTSExample of data processing
93F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR PRODUCTSSurface rainfall C-band retrieval
94F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR PRODUCTSRetrieval expected accuracy
RADAR PRODUCTSRetrieval expected accuracy
S-band radar
sim
simest
R
RRFSE
2/12ˆ
Algorithms:R1=M-PR2=WSR-88DRdp= G. et al. (rob)R1(Kdp)=S-ZR2(Kdp)=G-S (lin)Rdp1=G-S (rob)Rdp2=R-Z (log)
Fractional Standard Error
95F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR PRODUCTS Path attenuation mitigation
RADAR PRODUCTS Path attenuation mitigation
S-band radar: immune to rain path attenuation C-band radar: corrected for rain path attenuationusing fully polarimetric data (Zh, Zdr, Kdp)
96F.S. Marzano – Microwave Radar Meteorology: foundations and applications
RADAR PRODUCTSHydrometeor classification
Hailstorm in Florida observed by S-band polarimetric radar
... and derived hydrometeor classification