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PROGRESS IN SAR SHIP PROGRESS IN SAR SHIP DETECTION AND WAKE DETECTION AND WAKE ANALYSIS ANALYSIS J.K.E. Tunaley J.K.E. Tunaley London Research and Development Corporation, London Research and Development Corporation, 114 Margaret Anne Drive, 114 Margaret Anne Drive, Ottawa, Ontario K0A 1L0 Ottawa, Ontario K0A 1L0 1-613-839-7943 1-613-839-7943 http://www.london-research-and-development.com/ http://www.london-research-and-development.com/

PROGRESS IN SAR SHIP DETECTION AND WAKE ANALYSIS J.K.E. Tunaley London Research and Development Corporation, 114 Margaret Anne Drive, Ottawa, Ontario K0A

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Page 1: PROGRESS IN SAR SHIP DETECTION AND WAKE ANALYSIS J.K.E. Tunaley London Research and Development Corporation, 114 Margaret Anne Drive, Ottawa, Ontario K0A

PROGRESS IN SAR SHIP PROGRESS IN SAR SHIP DETECTION AND WAKE DETECTION AND WAKE

ANALYSISANALYSISJ.K.E. TunaleyJ.K.E. Tunaley

London Research and Development Corporation,London Research and Development Corporation,114 Margaret Anne Drive,114 Margaret Anne Drive,Ottawa, Ontario K0A 1L0Ottawa, Ontario K0A 1L0

1-613-839-79431-613-839-7943

http://www.london-research-and-development.com/http://www.london-research-and-development.com/

Page 2: PROGRESS IN SAR SHIP DETECTION AND WAKE ANALYSIS J.K.E. Tunaley London Research and Development Corporation, 114 Margaret Anne Drive, Ottawa, Ontario K0A

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OUTLINEOUTLINE

K-distributionK-distribution– New simple asymptotic approach for large threshold New simple asymptotic approach for large threshold

valuesvalues– Parameter estimation difficulties Parameter estimation difficulties – Implications for ship detectionImplications for ship detection

Ship WakesShip Wakes– Study started at RMC, Kingston using RADARSAT-2 Study started at RMC, Kingston using RADARSAT-2

images, AIS, plus other information.images, AIS, plus other information.– Findings and implications for MDA Findings and implications for MDA

See Web site for papersSee Web site for papers

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K-DistributionK-Distribution

Ships are bright blobs in SAR imagesShips are bright blobs in SAR images– Need statistics of clutter background for CFARNeed statistics of clutter background for CFAR

K-D excellent description of radar clutterK-D excellent description of radar clutter– Basis is modulated complex Gaussian clutterBasis is modulated complex Gaussian clutter

Physical / statistical basis incompletePhysical / statistical basis incomplete– Modulating distribution assumed gammaModulating distribution assumed gamma

Modified Bessel functions of 2Modified Bessel functions of 2ndnd kind. kind.– Computational complexityComputational complexity

Approximation for tail values needed Approximation for tail values needed

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K-D APPROXIMATIONK-D APPROXIMATION

Low PFA: interested in tail of distributionLow PFA: interested in tail of distribution– Represent pdf as an integralRepresent pdf as an integral– Use steepest descentsUse steepest descents

Accurate to better than 0.1% (PFA = 10Accurate to better than 0.1% (PFA = 10-9-9))

Not sensitive to statistics of modulationNot sensitive to statistics of modulation– Implies that K-D has sound physical basisImplies that K-D has sound physical basis

Basic code can be implemented in < 18 Basic code can be implemented in < 18 lines of C# or C++.lines of C# or C++.

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THRESHOLD COMPARISONTHRESHOLD COMPARISON

LOOKSLOOKS L = 1 L = 4

PFA Smoothness

Accurate Approx. Accurate Approx.

10-9 0.5 214.7 214.8 91.59 91.62

10-9 5.0 47.49 47.50 18.796 18.800

10-9 50.0 24.24 24.24 8.841 8.842

10-6 0.5 95.43 95.55 46.40 46.43

10-6 5.0 25.69 25.70 11.263 11.267

10-6 50.0 15.337 15.338 6.128 6.128

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PARAMETER ESTIMATIONPARAMETER ESTIMATION

Need to estimate mean and order Need to estimate mean and order parameterparameter– Number of looks is givenNumber of looks is given

Can estimate optimal performanceCan estimate optimal performance– Uses Fisher information (Cramer Rao)Uses Fisher information (Cramer Rao)

Parameter variance depends on number Parameter variance depends on number of independent samples, Nof independent samples, NNeed to consider biasNeed to consider biasNote: Parameters need not be integerNote: Parameters need not be integer

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OPTIMUM MEAN INTENSITYOPTIMUM MEAN INTENSITYCramer Rao BoundCramer Rao Bound

0.01

0.1

1

0.1 1 10 100

Nu

Sta

ndard

Devia

tion M

u #Samples N = 256

L = 1

L = 4

L = 10

Spiky Rayleigh

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SDs USING MOM: N = 1000SDs USING MOM: N = 1000

0.001

0.01

0.1

1

1 10 100

Nu

Sta

ndar

d D

evia

tion

1/N

u

0.001

0.01

0.1

1

1 10 100

NuS

D 1

/Nu

(MO

M)

Optimum Practical

L = 1 Black; L = 4 Red; L = 10 Yellow

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PRACTICAL THRESHOLDPRACTICAL THRESHOLD

1

10

100

1 10 100

Nu

Det

ectio

n T

hres

hold

(P

FA

=1.

0E-9

)

L = 4

N = 10000

N = 100

N = 1000

Ideal

Spiky Rayleigh

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CONCLUSIONS (1)CONCLUSIONS (1)

K-distribution approximation will reduce computational K-distribution approximation will reduce computational complexity for ship detectioncomplexity for ship detectionMethodology adds support to use of K-distributionMethodology adds support to use of K-distribution– Insensitivity to modulating distributionInsensitivity to modulating distribution

Mean of K-distribution can be estimated as usualMean of K-distribution can be estimated as usualParameter variance may bias detection thresholds by Parameter variance may bias detection thresholds by large factors if N < 1000large factors if N < 1000– Very important in spiky clutterVery important in spiky clutter– Without correction, PFA may increase by orders of magnitudeWithout correction, PFA may increase by orders of magnitude– If corrected, probability of ship detection is reducedIf corrected, probability of ship detection is reduced– Adaptive pixel block size (N) is desirable in variable clutter Adaptive pixel block size (N) is desirable in variable clutter

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SHIP WAKESSHIP WAKES

Turbulent wake study with Dan Roy at Turbulent wake study with Dan Roy at RMCRMC– RADARSAT-2 imagesRADARSAT-2 images– AISAIS– Other ship information about propulsion Other ship information about propulsion

system (Ship owners, Internet, etc.)system (Ship owners, Internet, etc.)

Analysis (60 ships) includesAnalysis (60 ships) includes– Twin screws/single screwTwin screws/single screw– Left/right handed screwsLeft/right handed screws

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RMC RESULTSRMC RESULTS

Wakes not usually visible when wind Wakes not usually visible when wind speed U > 6 m/sspeed U > 6 m/sShip speed V is important: if U < 6 m/s && Ship speed V is important: if U < 6 m/s && V > 5 m/s, 80% of wakes are visibleV > 5 m/s, 80% of wakes are visibleBright line on side of wake consistent with Bright line on side of wake consistent with propeller flows (swirling and axial) and propeller flows (swirling and axial) and wind directionwind direction– Wakes from shallow twin screws tend to be Wakes from shallow twin screws tend to be

visiblevisible

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RSAT-2: QUEEN OF ALBERNIRSAT-2: QUEEN OF ALBERNI

Data supplied by MDA Corporation

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Q of A ParametersQ of A ParametersParameter

Length (m) 139

Maximum Beam (m) 27.1

Mean Draft (m) 5.5

Maximum Draft (Prop. Tip, m) 5.72

Block Coefficient (estimated) 0.6

Number of Propellers 1

Number of Blades 4

Propeller Shaft Depth (m) 3

Propeller Diameter (m) 5

Propeller Type CPP

Service Speed (knots) 19

Propeller Speed @ 19 knots (rpm) 170

Maximum Power (MW) 8.83

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COMBINED SWIRLING AND COMBINED SWIRLING AND AXIAL WAKEAXIAL WAKE

Consider both linear and angular Consider both linear and angular momentum in propeller wakemomentum in propeller wake– Modify Prandtl’s approach to theoryModify Prandtl’s approach to theory– Estimate fluid linear and angular momentum Estimate fluid linear and angular momentum

using standard engineering methodsusing standard engineering methods

Apply to Queen of Alberni (BC Ferries)Apply to Queen of Alberni (BC Ferries)

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Q of A Wake DiameterQ of A Wake Diameter

1

10

100

10 100 1000 10000

Distance (m)

Wake D

iam

ete

r(m

)

Axial

Swirling

Combined

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Queen of Alberni Maximum Queen of Alberni Maximum Surface Flow SpeedSurface Flow Speed

0.01

0.1

1

10

10 100 1000 10000

Distance (m)

Sur

face

Spe

ed (

m/s

)

Swirling

Axial

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Deep Screw CaseDeep Screw CaseMaximum Flow SpeedMaximum Flow Speed

0.01

0.1

1

10

10 100 1000 10000

Distance (m)

Sur

face

Spe

ed (

m/s

)

Axial

Swirling

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CONCLUSIONS (2)CONCLUSIONS (2)

Surface flows in the turbulent wake can be large Surface flows in the turbulent wake can be large compared with Bragg group velocitycompared with Bragg group velocity– Expect significant radar wake visibility for long Expect significant radar wake visibility for long

distancesdistances

Swirling component dominates axial flow Swirling component dominates axial flow immediately astern and especially when screws immediately astern and especially when screws are deepare deepWake characteristics can be used to verify shipWake characteristics can be used to verify shipNote:Note:– Hydrodynamic wake width is only one factor in radar Hydrodynamic wake width is only one factor in radar

wake width. Others are flow speeds, ambient wind wake width. Others are flow speeds, ambient wind and waves, radar effects and geometry.and waves, radar effects and geometry.

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ENDEND

Thank You All!Thank You All!