radar signal extraction using correlation - eurasip

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Correlation methods take advantage of the periodic character of radar signals. In such cases, autocorrelation and cross-correlation improve the detection of ...
RADAR SIGNAL EXTRACTION USING CORRELATION   1-2   1   1 ENST-Bretagne, Département Signal et Communication, BP 832, 29285 BREST CEDEX, e-mail : [email protected] 2 THOMSON-CSF, DIVISION RCM, Centre électronique de Brest, 10 Avenue 1ère DFL, 29283 BREST CEDEX, Fax : (33)98312767, Tel : (33)98312705, e-mail : [email protected] 1



amplitude and time of arrival of the pulse. The

In this paper we present post-integration processing

processor deinterleaves pulses and assigns samples to

in order

to

electronic

a pulse train which represents the radar signal. Using

support

measure

Correlation

a database, the processor identifies the emission.

methods take advantage of the periodic character of

Then information is presented to the defence systems.

improve

the

sensitivity

(ESM)

of

receivers.

radar signals. In such cases,

autocorrelation

and

A basic microwave receiver consists of a front-

cross-correlation improve the detection of signals

head filter followed by a detector and a video low-

with high repetition frequency. Furthermore, since

pass filter with Bv bandwidth.

the extraction of radar parameters is necessary to identify received signals, we study three types of estimators : straightforward

method,

interpolation

     !  Those

receivers

always

need

to

improve

the

method and maximum likelihood one. Simulation

probability of detection of radar signals. Using digital

studies with realistic models and real signals are

processing, we can extract signal from noise, keeping

carried

in mind that such a system must provide radar

out

to

validate

performances

of

such

parameters for identification.

processing. With a view to implanting correlation functions,

Sensitivity is defined in terms of the signal-to-

some architectures are studied. The choice of method

noise ratio at the output of the video filter. This paper

is of interest since we need a lot of samples to be

deals with correlation processing. Section 2 discusses

integrated.

the

To conclude, as radar ESM receiver requires most

autocorrelation processing, detection processing of

information on received signals, the enhancement of

those methods and exploitation of the results. Special

the sensitivity using correlation method is of great

attention is paid in section 3 to the application of

interest.

cross-correlation. Some simulations are presented in

support

gain

obtained

at

the

output

of

section 4 to validate the performances. Section 5

  

Electronic

sensitivity

describes

measure

systems

perform

the

function of electromagnetic area surveillance in order to determine the identity and direction of arrival of surrounding radar emitters. Automatic radar ESM

the

complexity

to

implanting

such

processing since many samples should be integrated.

    "

Since the radar signal is periodic, autocorrelation

systems are passive receivers which receive emissions

processing seems to be of interest, because it keeps

from other platforms, measure the parameters of each

the repetitive character with the same pulse repetition

detected pulse and thus sort the emissions to enable

frequency. After quadratic detection, the received

the

signal is a pulse train in additive gaussian noise.

determination

of

the

radar

parameters

and

identification of each emitter. The contribution of our study is to improve the receiver sensitivity using post-integration processing such

as

autocorrelation

and

cross-correlation

methods.

In practice, the amplitude envelope received by the ESM system is a series of pulses modulated by the radar frequency carrier. After detection of radar pulses intercepted by the the

ESM

receiver

Given

takes

digital

measurements of frequency within the pulse, bearing,

a

finite

observation

interval

Ti,

the

autocorrelation is estimated by :

Γ (k ) =

    

antennas,

   # 1



∑ X(i )X(i + k ) 0 ≤ k ≤ N − 1 N − k =  1  Γ  (k ) = ∑ X(i )X(i + k ) N  = Γ  (k ) =

1  − ∑ X(i)X(i + k ) 0 ≤ k ≤ N − 1 N = corr

(1) (2) (3)

where N is the number of samples on the Ti interval. Ti has

to

be

sufficiently

long

for

the

estimated

correlation

to

be

Γ 2

(unbiased) and

accurate.

Both

Γ1

estimators

(biased) use all

the

samples,

frequency (HPRF signal). Furthermore with a low SNRi, the processing gain decreases quickly (Fig.2). 60

whereas the third one works with Ncorr samples out of 2Ncorr (Ncorr is a constant value, Ncorr=N/2). The third

40

estimator carries out the correlation function on a

‘sliding



temporal

window’

but

its

   

decrease by 3dB in comparison with the two previous

Γ

20

performances

0



estimator gives the

- 20

first result when Ncorr samples have been integrated,

- 40

estimators. Despite this, the

3

whereas we have to wait for N samples with the first and

second

functions.

This

note

achieves

-8

-6

-4

-2

0

2

4

6

8

10

 

a

ρ= 0.5

compromise between SNR gain and extraction of

ρ= 0.2

ρ= 0.1

ρ= 0.01

ρ= 0.001

  Variation of SNR with SNR and ρ (Ν=20000).

samples in a prominent position.

   !  $  #

45 40

The output process of a radar signal without noise is

35

as follows :

30



25



5J

ρ.)

A



Γ(τ)   

2

20 15 10 5

AUTOCORRELATION

-8

-6

-4

-2

0

2

4

6

8

10

 

J

29

29

241

241

Input



τ

Output   Output signal where PRI = pulse repetition interval, PW = pulsewidth.

% &  ''( ) Fig.4

variance and Bv bandwidth.

 

noise with zero mean,

σ

Γ  (τ) = 0 .

Γ (τ ) = Γ (τ ) + Γ (τ )

very low in comparison with Ti, thus low compared with

Γ S ( τ) .

Γ N (τ )

is very

2

2

where SNRi=A /σ - N 

(5)

= π.B .T = π.B .N.T =

of

  







  

   

  



  





  

 Probability of detection with SNR and N (P=1e-5).

# *   

The aim of an ESM receiver is to identify emissions,

At a peak of correlation, the output SNR (SNRo) is :

N ρ SNR  SNR =  1 + 2ρSNR 

peak



(4)

As we suppose that the noise correlation duration is

a





, the output process is :

of

 

X(t ) = S(t ) + N( t)

detection



greater than PRI in order to decrease the error of the

Given

the

 

whole number of PRI.

determines



Furthermore, the observation interval should be much output signal since we integrate samples during a non

 

correlation.

Signal and noise will not correlate then

 

  Variation of SNR with SNR and N (ρ=0,2).

The signal is mixed with an additive gaussian 2



number

so the system has to define its characteristics exactly. There are three parameters to estimate : amplitude, PW and PRI. We study three estimators. The sampling frequency (1/Ts) of the autocorrelation function is the same as the signal one. Indeed, the

of independent samples.

autocorrelation function of the signal with a band

The SNR gain depends on the integration window

limited spectral density, has the same limited band

(Fig.3), the duty cycle of the pulse train (ρ = PRI / PW) (Fig.2). That is why such processing is of interest for radar signals with high pulse repetition

since

Fourier

transform

of

the

autocorrelation

function is the power spectral density. In that case

Shannon’s

theorem

applied

to

the

signal

or

its

correlation function gives the same sampling rate.

     Studying the output samples, we get : PRI = interval between two peaks. PW = width at the halfway up of a triangle of correlation.

amplitude = maxρ

 $' .( "   +-,   +-,   +-, */ .0 */ .0 */ .0

  +, E

1 1 2%3 2#3

0

0,5

0,4

0,6

0,3

0,5

5,7

3,8

3,3

2,4

2,3

2,5

13,8

7,2

10,7

6,5

5,5

6,6

13,9

7,1

10,1

6,3

5,6

5,5

  PW and peak correlation accuracy.

(max is the peak value).

The parameter accuracy is defined as follows :

   !    At each triangle of correlation, we have to estimate

E[parameter ]

ε% =

variance  

the two slopes in the mean-square criterion: PW

=

a  b

− a b 

and amplitude

2a  a 

%  2 "

2a  a  PRI

=

a

− a

The purpose of such a method is to recognise an a prior known signal Y(k) in the received noisy signal.

y(i)

The cross-correlation estimators are the y1(i) = a1.i + b1

Γ (k ) =

J −1

MAX



^

MV

=

i = J − k 29

 =# − PW # −

 =# −  PW

= #

i = J − k 29

T  PW (i − J ) + 1 y  T   PW (i − J ) + 1 S

S

i 2

 =

∑ Y(i )X(i + k )

(6)

= N  ρSNR 

(7)

interval and of the duty cycle. Thus we obtain a



constant improvement (Fig.6).

∑ (y  − max)(i − J ) − ∑ (y  − max)(i − J )

  



The gain is a linear function of the observation # +  PW

= # # +  PW

J −1



SNR

∑ (i − J ) + ∑ (i − J ) 

1 N−k

With same working hypothesis as 2.2, we get :

 Slopes of the triangle interpolation. # −

as

%   !  $  #

i

" #$ %  &    

same

those of autocorrelation where :

y2(i) = a2.i + b2

PW !" = maxT

.100

J + k 29  + ∑  i =J  J + k 29  − ∑  i =J 

T  PW (i − J ) − 1 y T  PW (i − J ) − 1

45

40

S



i



35



2

 

S

 

30

25

where JTs is the time of arrival of the peak, yi the signal value at iTs, kLI the number of samples used in

20 -8

-6

-4

-2

a slope. We check that the pulsewidth estimator and

0

2

4

6

8

10

 

the peak value one are both efficient in the maximum

  

  

  

  

  Variation of SNR with SNR and N (ρ=0,2).

likelihood criterion.

 ' ( )% *   +, !      $ %  &   )    %*   %   * -". (   /   )  *   *!   *  !            *   %!% !) **  ) * 0% 1  ))%%*

% &  .44 (  1

 0,8   

 0,6    

 0,4 

0,2

  %  A computer simulation was conducted to compare the

0 0,05

0,15

0,25

method is the easiest one to implant, whereas the last estimator

has

the

best

accuracy

thanks

to

the

0,35

0,45

0,55

0,65

0,75

 

performances of the different estimators. The first   

  

  

  

  Detection probability with SNR and N (P=10e-5).

maximum likelihood principle as can be seen in

Fig.7 shows that the more samples we integrate, the

Table 1.

easier the detection of a signal with additive noise is.

%% 5&(   &2&(  &.  The

use

of

cross-correlation

function

provides

) *"  6  " 7 

) ( &( 5&5 X(i)

X(N)

X(0)

sensitivity gain, but special attention is given to such

*

applications. Indeed, the operator of the ESM system

k weighting

has no information on the received signal. That is why the aim of this method is to search for a given radar in the surrounding area in order to perform the

X(N+k)

X(k)

  Classical structure.

warning function.

#   "  *   "

) &5 ! 5&5 

Simulation studies with realistic models and real

calculus (Eq.8-9) :

signals were conducted to corroborate the theoretical

Γ(k ) =

performance predictions. The

scenario

Γ(k)

* *

presented

here

(Fig.

8-9-10)

is

a

mixture of three signals.

Each correlation sample is the result of a recursive

( )

R N

(8)

N

( ) = R (N − 1) + X(N )X(N + k )

where R  N The

(9)



recursive

method

uses

one

multiplier-

accumulator cell (Fig.12) per correlation point. The correlator is designed as a macrocell.

X(i)

k

Γ (k)

weighting

+

*

CLK

  Recursive structure.

)% 87 &( 9 5&5

   

 

 

  Input signal with S1 : HPRF signal with SNR=0dB; ρ=0,1 -

S2 : LPRF (low PRF) signal with SNR=13dB; ρ=5,1.1e-4 - S3 : LPRF signal with SNR=13dB; ρ=6.1e-4 - σ=1 - N=2000.

Using a Fourier transform, we compare correlation and convolution (Eq.10 ) :

&Γ (τ ) = S( t ) * S, ( t ) ← → γ (υ ) = γ (υ )γ I

I

I

*

I

(υ )

(10)

The advantage of such method is the use of a Fast Fourier transform algorithm.

  "  

To conclude, as the function of a radar ESM receiver is surveillance to determine radar activity, the system Y(t)

requires most information on received signals. So the

) )  *) % 

enhancement of sensitivity achieved by correlation methods is of interest. Those functions contribute to the increased detection of HPRF signals with low time

$%& '(

SNR. This processing also carries out parameter +%& '(

  Autocorrelation output signal.

estimation of radar signals. Future ESM system could incorporate such functions.



Z(t)

time

HPRF

  Cross-correlation output signal.

1 V. ALBRIEUX, ‘Compilateur de la fonction de corrélation’,   , Vol.1, 1989, p.319-322. 2 M. BELLANGER,           , 4° édition, MASSON, 1990. 3 T.G. KINCAID, ‘Estimation of periodic signals in noise’, ., Vol.46, n°6, 1969, p.1397-1403. 4 J. MAX,                   , Tome 1, MASSON, 1981, p.173-181. 5 A. PAPOULIS,  !    "        , Mc GRAW-HILL BOOK COMPANY, 1965. 6 R.G. WILEY, #            , ARTECH HOUSE Inc., 1982.

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