Dynamic Multipath Model of Low Angle Passive Radar Tracking with Experimental Evaluation

The problem of multipath propagation encountered in radar tracking of low elevation targets in the presence of reflections from the sea is addressed. A detailed model of the multipath propagation considering both the specular and the diffuse reflection components in target tracking using passive radars is established. Based on the geometry of the specular and the diffuse reflections, expressions for the reflection coefficient and the scattering field are derived. Experiments in the outfield indicate that the model proposed agrees with the test data well, which can provide an accurate prediction of the angle measurement errors in the presence of multipath effects.


Keywords:    Multipath propagation effectslow-altitude target trackingspecular reflectiondiffuse reflection

In tracking low elevation targets, the presence of reflections from the sea (or ground) surface (i.e., multipath propagation) can cause severe errors in the target angle measurement, which brings a great influence on the overall tracking performance. Estimation or prediction of the multipath error is normally a difficult task due to the complexity of the reflection properties of the surface as well as the dependency of this error on a large number of radar parameters.


In the past, multipath effects in radar tracking have been studied by many researchers. Beckman and Spizzichino1, put forward the classic theory applied to the far-field diffuse reflection on rough surface, and established the concept of flashing surface. Then, Barton analysed the radar measurement error due to the diffuse reflection on rough surface, and pointed out that the radar echo is a random variable which complies with a definite probability distribution (usually the Rice distribution)2 . In the early 1990s, Bruder studied the fixed deviation in the indicated target angle due to the specular reflection on the flat surface3. Sletten and Trizna4, et al. carried out an experiment to investigate the multipath propagation over the sea surface in the purpose of analysing its implications for sea-clutter statistics.


Along with the study of the reflection characteristics, a number of different methods including angle averaging, frequency agility, offset angle track were presented and a combination of these methods was suggested to reduce the effects of multipath. For example, the multipath propagation was considered as an estimation/tracking problem and a filtering technique was employed to reduce the multipath effects5. In continuation, the use of frequency agility and the fusion of the tracks obtained with different waveform frequencies were presented6. Then, a maximum maneuver-based filter and a multiple model estimator were proposed to compensate the multipath error in tracking with monopulse radars7. Recently, several new techniques are introduced to reduce the interference of multipath effects, such as orthogonal frequency division multiplexing (OFDM)8-9, blind signal separation10 and Fractional Fourier Transform (FrFT)11. However, due to the complexity of the problem itself, there are still many issues to be studied.


In multipath effects, the modelling of the multipath propagation is a fundamental problem. In earlier works, researchers mainly focus on the reflection characteristics of the rough surface in low-angle radar tracking. For the actual tracking scenes, especially for tracking low elevation targets over the sea, there are few models providing detailed description of the multipath errors due to reflections of the three-dimensional sea surface. In this paper, a dynamic model of the multipath propagation considering both the specular and the diffuse reflection components in target tracking using passive radars is established. The two components of the sea surface reflection are described. A three-dimensional description of the sea surface is introduced based on the sea spectrum model. Then, based on the geometry of the specular and the diffuse reflections, expressions for the reflection coefficient and the scattering field are derived. The result of simulations of the dynamic sea surface is presented. The proposed model is validated by the test data of experiments in the outfield, which indicates that the model provides an accurate prediction of the angle measurement errors in the presence of multipath effects.


When tracking low elevation targets, the presence of reflections from the sea surface can result in a strong interference in target angle measurements. A simple illustration of the geometry of multipath propagation is depicted in Fig 1. There are two separate paths between the target and the passive radar: the direct path and the indirect path via reflections with grazing angle from the sea surface. The incident complementary angle of the direct path is . The surface reflected signal generally consists of two components, namely, specular (coherent) and diffuse (incoherent). The specular reflection is caused by a smooth (mirror-like) surface with grazing anglewhile the diffuse reflection is caused by the surface irregularities. The incident complementary angle and the reflective complementary angle of the diffuse signal are θ1 and θ2, respectively.


Figure 1. Geometry of the multipath propagation.


To study the multipath effects of the sea, a three-dimensional model of the sea surface is required. Then, three components of the received signal of radar antenna (i.e. the direct incident signal, the specular reflection signal and the diffuse reflection signals) need to be calculated. In the calculation of diffuse reflection signals, the sea surface is divided into finite small panels by orthogonal rectangular. Firstly the diffuse signals for each of the small panels are calculated. Then, according to the geometry of the diffuse reflection, whether the reflected signals can be received by the radar antenna is determined. All the diffuse signals which can be received are summed to obtain the total diffuse signal. Finally, the three components of the received signal of radar antenna are vectorially summed to calculate the target angle. The calculation flow chart of the sea multipath propagation is depicted in Fig 2.


Figure 2. Calculation flow chart of sea multipath.


The sea surface is formed by the interactions of the sea wind, the sea gravity and the sea surface tension, while such interactions are nonlinear and changing with time. The sea surface is approximately cyclical in large-scale and superimposed on small-scale ripples. That is to say, it is a blend with both large-scale structure and micro-structure12-13. The methods of simulating the sea surface can be mainly divided into two categories: Fractal simulation and statistical simulation. As the spectrum of fractal function is a negative power-law spectrum, it can only construct a rough surface obeying the negative form of power-law spectrum, while the statistical simulation method can construct any forms of spectrum. Therefore, the statistical methods are more generally used to simulate the sea surface.


The sea spectrum model is one kind of the statistical simulation methods. This method considers the waves as superimposed results of an infinite number of sine waves with ranged amplitude, frequency, direction and phase. The theory of random process and the linear wave’s theory are used to analyze the sea spectrum. For the actual sea surface, its energy distributes not only in a certain frequency range, but also in a wide direction range. It can be regarded as a superposition of a number of cosine waves, with amplitude an, frequency, original phase and along with the spread direction angle. The expression of the spectrum can be denoted as  

   
f(x,y,t)= n=1 a n cos[ ω n t k n (xcos θ n +ysin θ n )+ ϕ n ] MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqipC0xf9vqqrpepeea0xXdHaVhbbf9v8qqaqFr0xc9pk 0xbba9q8WqFfea0=yr0RYxir=Jbba9q8aq0=yq=He9q8qqQ8frFve9 Fve9Ff0dmeaabaqaciaacaGaaeqabaWaaeaaeaaakeaacaWGMbGaai ikaiaadIhacaGGSaGaamyEaiaacYcacaWG0bGaaiykaiabg2da9maa qahabaGaamyyamaaBaaaleaacaWGUbaabeaaaeaacaWGUbGaeyypa0 JaaGymaaqaaiabg6HiLcqdcqGHris5aOGaci4yaiaac+gacaGGZbGa ai4waiabeM8a3naaBaaaleaacaWGUbaabeaakiaadshacqGHsislca WGRbWaaSbaaSqaaiaad6gaaeqaaOGaaiikaiaadIhaciGGJbGaai4B aiaacohacqaH4oqCdaWgaaWcbaGaamOBaaqabaGccqGHRaWkcaWG5b Gaci4CaiaacMgacaGGUbGaeqiUde3aaSbaaSqaaiaad6gaaeqaaOGa aiykaiabgUcaRiabew9aMnaaBaaaleaacaWGUbaabeaakiaac2faaa a@64FD@          (1)
where is the wave number of the nth component, and.
π θ n π MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqipC0xf9vqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGacaGaaiaabeqaamaabaabaaGcbaGaeyOeI0Iaeq iWdaNaeyizImQaeqiUde3aaSbaaSqaaiaad6gaaeqaaOGaeyizImQa eqiWdahaaa@4088@

When there are only gravity waves, the frequency can also be expressed by the wave number 14 kn
ω n 2 =g k n 2 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqipC0xf9vqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGacaGaaiaabeqaamaabaabaaGcbaGaeqyYdC3aa0 baaSqaaiaad6gaaeaacaaIYaaaaOGaeyypa0Jaam4zaiaadUgadaqh aaWcbaGaamOBaaqaaiaaikdaaaaaaa@3E49@          (2)
The direction spectral density function of the sea spectrum is

S(ω,θ)dωdθ= Δω Δθ 1 2 a n 2 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqipC0xf9vqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGacaGaaiaabeqaamaabaabaaGcbaGaam4uaiaacI cacqaHjpWDcaGGSaGaeqiUdeNaaiykaiaadsgacqaHjpWDcaWGKbGa eqiUdeNaeyypa0ZaaabuaeaadaaeqbqaamaalaaabaGaaGymaaqaai aaikdaaaGaamyyamaaDaaaleaacaWGUbaabaGaaGOmaaaaaeaacqGH uoarcqaH4oqCaeqaniabggHiLdaaleaacqGHuoarcqaHjpWDaeqani abggHiLdaaaa@516C@          (3)

Theoretically, the range of  is . However, actually the energy of waves usually distributes at  which centered on the main spread direction. The direction spectral density function is generally of the following form:

S(ω,θ)=S(ω)G(ω,θ) MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqipC0xf9vqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGacaGaaiaabeqaamaabaabaaGcbaGaam4uaiaacI cacqaHjpWDcaGGSaGaeqiUdeNaaiykaiabg2da9iaadofacaGGOaGa eqyYdCNaaiykaiaadEeacaGGOaGaeqyYdCNaaiilaiabeI7aXjaacM caaaa@4798@          (4)
where is the spectrum function, is the directional distribution function. There have been a number of perfect directional distribution functions. The spectrum function can be expressed using the angular frequency as follows14

S(ω)= a g 2 ω 2 exp[β ( g Uω ) 4 ] MathType@MTEF@5@5@+= feaagKart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqipC0xf9vqqrpepeea0xXdHaVhbbf9v8qqaqFr0xc9pk 0xbba9q8WqFfea0=yr0RYxir=Jbba9q8aq0=yq=He9q8qqQ8frFve9 Fve9Ff0dmeaabaqaciaacaGaaeqabaWaaeaaeaaakeaacaWGtbGaai ikaiabeM8a3jaacMcacqGH9aqpdaWcaaqaaiaadggacaWGNbWaaWba aSqabeaacaaIYaaaaaGcbaGaeqyYdC3aaWbaaSqabeaacaaIYaaaaa aakiGacwgacaGG4bGaaiiCaiaacUfacqGHsislcqaHYoGycaGGOaWa aSaaaeaacaWGNbaabaGaamyvaiabeM8a3baacaGGPaWaaWbaaSqabe aacaaI0aaaaOGaaiyxaaaa@4DAC@          (5)
where U represents the wind speed at the height of 19.5m of the sea, a is a constant which characterizes the height of the waves, a=8.10× 10 3 MathType@MTEF@5@5@+= feaagKart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqipC0xf9vqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGacaGaaiaabeqaamaabaabaaGcbaGaamyyaiabg2 da9iaaiIdacaGGUaGaaGymaiaaicdacqGHxdaTcaaIXaGaaGimamaa CaaaleqabaGaeyOeI0IaaG4maaaaaaa@400F@ , g denotes the acceleration of gravity,  is a constant related with the average cycle U, β=0.74 MathType@MTEF@5@5@+= feaagKart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqipC0xf9vqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGacaGaaiaabeqaamaabaabaaGcbaGaeqOSdiMaey ypa0JaaGimaiaac6cacaaI3aGaaGinaaaa@3B69@ . The spectrum peak can be denoted as. ω m =8.565/U MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqipC0xf9vqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGacaGaaiaabeqaamaabaabaaGcbaGaeqyYdC3aaS baaSqaaiaad2gaaeqaaOGaeyypa0JaaGioaiaac6cacaaI1aGaaGOn aiaaiwdacaGGVaGaamyvaaaa@3F12@      

4.1 Model of Specular Reflection


Figure 3. shows the geometry of the specular reflection from sea, where T denotes the radiant source with the coordinates (0, 0, h1), a1 and a2 represent the passive radar antennas with the baseline which is d meters long, and the altitude of antennas is h2. Taking the antenna a1 for example, the distance between T and a1 is, the angle between the direct signal and the centerline of the radiation beam is , the distances between specular reflection point I and T, a1 are R1 and R2, respectively. The angles between reflection signal and the centerline of the T, a1 are a1 and a1, respectively, the grazing angle of the reflection surface is.

Figure 3. Geometry of the specular reflection from sea.


The distance R between the radiant source T and the antenna a1 is

R= (x a 1 2 +y a 1 2 + (h a 1 h 1 ) 2 ) MathType@MTEF@5@5@+= feaagKart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqipC0xf9vqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGacaGaaiaabeqaamaabaabaaGcbaGaamOuaiabg2 da9maakaaabaGaaiikaiaadIhacaWGHbWaa0baaSqaaiaaigdaaeaa caaIYaaaaOGaey4kaSIaamyEaiaadggadaqhaaWcbaGaaGymaaqaai aaikdaaaGccqGHRaWkcaGGOaGaamiAaiaadggadaWgaaWcbaGaaGym aaqabaGccqGHsislcaWGObWaaSbaaSqaaiaaigdaaeqaaOGaaiykam aaCaaaleqabaGaaGOmaaaakiaacMcaaSqabaaaaa@49EA@          (6)

The angle between the direct path Ta1 and the beam axis of the radiant source is the coordinates of the specular reflection point I is


ε=60.4j32.4 MathType@MTEF@5@5@+= feaagKart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqipC0xf9vqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGacaGaaiaabeqaamaabaabaaGcbaGaeqyTduMaey ypa0JaaGOnaiaaicdacaGGUaGaaGinaiabgkHiTiaadQgacaaIZaGa aGOmaiaac6cacaaI0aaaaa@4033@
XI= R 1 cosθ (x a 1 2 +y a 1 2 ) x a 1 ,YI= R 1 cosθ (x a 1 2 +y a 1 2 ) y a 1 MathType@MTEF@5@5@+= feaagKart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqipC0xf9vqqrpepeea0xXdHaVhbbf9v8qqaqFr0xc9pk 0xbba9q8WqFfea0=yr0RYxir=Jbba9q8aq0=yq=He9q8qqQ8frFve9 Fve9Ff0dmeaabaqaciaacaGaaeqabaWaaeaaeaaakeaacaWGybGaam ysaiabg2da9maalaaabaGaamOuamaaBaaaleaacaaIXaaabeaakiGa cogacaGGVbGaai4CaiabeI7aXbqaamaakaaabaGaaiikaiaadIhaca WGHbWaa0baaSqaaiaaigdaaeaacaaIYaaaaOGaey4kaSIaamyEaiaa dggadaqhaaWcbaGaaGymaaqaaiaaikdaaaGccaGGPaaaleqaaaaaki aadIhacaWGHbWaaSbaaSqaaiaaigdaaeqaaOGaaiilaiaaykW7caaM c8UaamywaiaadMeacqGH9aqpdaWcaaqaaiaadkfadaWgaaWcbaGaaG ymaaqabaGcciGGJbGaai4BaiaacohacqaH4oqCaeaadaGcaaqaaiaa cIcacaWG4bGaamyyamaaDaaaleaacaaIXaaabaGaaGOmaaaakiabgU caRiaadMhacaWGHbWaa0baaSqaaiaaigdaaeaacaaIYaaaaOGaaiyk aaWcbeaaaaGccaWG5bGaamyyamaaBaaaleaacaaIXaaabeaaaaa@6489@          (7)
α=arccos( x a 1 x a 1 2 +y a 1 2 + (h a 1 h 1 ) 2 ) MathType@MTEF@5@5@+= feaagKart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqipC0xf9vqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGacaGaaiaabeqaamaabaabaaGcbaGaeqySdeMaey ypa0JaciyyaiaackhacaGGJbGaai4yaiaac+gacaGGZbGaaiikamaa laaabaGaamiEaiaadggadaWgaaWcbaGaaGymaaqabaaakeaadaGcaa qaaiaadIhacaWGHbWaa0baaSqaaiaaigdaaeaacaaIYaaaaOGaey4k aSIaamyEaiaadggadaqhaaWcbaGaaGymaaqaaiaaikdaaaGccqGHRa WkcaGGOaGaamiAaiaadggadaWgaaWcbaGaaGymaaqabaGccqGHsisl caWGObWaaSbaaSqaaiaaigdaaeqaaOGaaiykamaaCaaaleqabaGaaG OmaaaaaeqaaaaakiaacMcaaaa@5320@          (8)
The angle between the specular incident component TI and the reflection surface is
θ=arctan( h 1 +h a 1 (x a 1 2 +y a 1 2 ) ) MathType@MTEF@5@5@+= feaagKart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqipC0xf9vqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGacaGaaiaabeqaamaabaabaaGcbaGaeqiUdeNaey ypa0JaciyyaiaackhacaGGJbGaaiiDaiaacggacaGGUbGaaiikamaa laaabaGaamiAamaaBaaaleaacaaIXaaabeaakiabgUcaRiaadIgaca WGHbWaaSbaaSqaaiaaigdaaeqaaaGcbaWaaOaaaeaacaGGOaGaamiE aiaadggadaqhaaWcbaGaaGymaaqaaiaaikdaaaGccqGHRaWkcaWG5b GaamyyamaaDaaaleaacaaIXaaabaGaaGOmaaaakiaacMcaaSqabaaa aOGaaiykaaaa@4E96@          (9)
The angle between the specular incident component TI and the beam axis of the radiant source is
α 1 =arccos( XI X I 2 +Y I 2 + h 1 2 ) MathType@MTEF@5@5@+= feaagKart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqipC0xf9vqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGacaGaaiaabeqaamaabaabaaGcbaGaeqySde2aaS baaSqaaiaaigdaaeqaaOGaeyypa0JaciyyaiaackhacaGGJbGaai4y aiaac+gacaGGZbGaaiikamaalaaabaGaamiwaiaadMeaaeaadaGcaa qaaiaadIfacaWGjbWaaWbaaSqabeaacaaIYaaaaOGaey4kaSIaamyw aiaadMeadaahaaWcbeqaaiaaikdaaaGccqGHRaWkcaWGObWaa0baaS qaaiaaigdaaeaacaaIYaaaaaqabaaaaOGaaiykaaaa@4BC2@          (10)
The angle between the specular reflection component Ia1 and the beam axis of the antenna a1> is:
α 2 =arccos( x a 1 XI (x a 1 XI) 2 + (y a 1 YI) 2 +h a 1 2 ) MathType@MTEF@5@5@+= feaagKart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqipC0xf9vqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGacaGaaiaabeqaamaabaabaaGcbaGaeqySde2aaS baaSqaaiaaikdaaeqaaOGaeyypa0JaciyyaiaackhacaGGJbGaai4y aiaac+gacaGGZbGaaiikamaalaaabaGaamiEaiaadggadaWgaaWcba GaaGymaaqabaGccqGHsislcaWGybGaamysaaqaamaakaaabaGaaiik aiaadIhacaWGHbWaaSbaaSqaaiaaigdaaeqaaOGaeyOeI0Iaamiwai aadMeacaGGPaWaaWbaaSqabeaacaaIYaaaaOGaey4kaSIaaiikaiaa dMhacaWGHbWaaSbaaSqaaiaaigdaaeqaaOGaeyOeI0IaamywaiaadM eacaGGPaWaaWbaaSqabeaacaaIYaaaaOGaey4kaSIaamiAaiaadgga daqhaaWcbaGaaGymaaqaaiaaikdaaaaabeaaaaGccaGGPaaaaa@5A9F@          (11)
The Fresnel reflective coefficient of the vertical polarization incident wave is
ρ 0 (θ)= εsinθ (ε cos 2 θ) εsinθ+ (ε cos 2 θ) MathType@MTEF@5@5@+= feaagKart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqipC0xf9vqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGacaGaaiaabeqaamaabaabaaGcbaGaeqyWdi3aaS baaSqaaiaaicdaaeqaaOGaaiikaiabeI7aXjaacMcacqGH9aqpdaWc aaqaaiabew7aLjGacohacaGGPbGaaiOBaiabeI7aXjabgkHiTmaaka aabaGaaiikaiabew7aLjabgkHiTiGacogacaGGVbGaai4CamaaCaaa leqabaGaaGOmaaaakiabeI7aXjaacMcaaSqabaaakeaacqaH1oqzci GGZbGaaiyAaiaac6gacqaH4oqCcqGHRaWkdaGcaaqaaiaacIcacqaH 1oqzcqGHsislciGGJbGaai4BaiaacohadaahaaWcbeqaaiaaikdaaa GccqaH4oqCcaGGPaaaleqaaaaaaaa@5DF7@          (12)
The dielectric constant of sea water for the X-band incident waves is .
The specular reflection factorcharacterizes the attenuation rate of amplitude of the specular reflection due to the rough reflecting surface, and it has the following relationship with roughness factor Γ of reflecting surface15.
Consequently, the total specular reflection coefficient can be calculated by
ρ(θ)= ρ 0 (θ) ρ s (θ) MathType@MTEF@5@5@+= feaagKart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqipC0xf9vqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGacaGaaiaabeqaamaabaabaaGcbaGaeqyWdiNaai ikaiabeI7aXjaacMcacqGH9aqpcqaHbpGCdaWgaaWcbaGaaGimaaqa baGccaGGOaGaeqiUdeNaaiykaiabeg8aYnaaBaaaleaacaWGZbaabe aakiaacIcacqaH4oqCcaGGPaaaaa@4768@          (13)


4.2 Model of Diffuse Reflection


The model of the diffuse reflection of the sea is presented on the basis of three-dimensional model of the sea surface. Firstly, the effective reflection region between the radiant source and the radar antenna are divided by finite two-dimensional orthogonal rectangles. Consequently, the actual terrain is reduced to a series of small panels with random gradient and random height. Then the diffuse signal of each of the small panels is calculated, which will be summed to obtain the total diffuse signal. The geometry of the diffuse reflection from sea is shown in Fig. 4.

Figure 4. Geometry of the diffuse reflection from sea.


For the scattering of large-scale gravity waves, its dispersion field can be calculated by the Kirchhoff Approximate (KA) method, that is to say, the field of any point on the rough surface can be approximated by the field of the partial tangent plane around the scattering point. The area of panels can be approximately replaced by the projection ds on the plane when the panels are small enough.
The scattering field of the radar wave of the unit sea surface can be represented as follows16

E mn = f t ( θ t ) f r ( θ r )( n ^ q ^ )exp[j w c (t t s )]ΔxΔy 4π R a R b n z V( θ 1 ) MathType@MTEF@5@5@+= feaagKart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqipC0xf9vqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGacaGaaiaabeqaamaabaabaaGcbaGaamyramaaBa aaleaacaWGTbGaamOBaaqabaGccqGH9aqpdaWcaaqaaiaadAgadaWg aaWcbaGaamiDaaqabaGccaGGOaGaeqiUde3aaSbaaSqaaiaadshaae qaaOGaaiykaiaadAgadaWgaaWcbaGaamOCaaqabaGccaGGOaGaeqiU de3aaSbaaSqaaiaadkhaaeqaaOGaaiykaiaacIcadaqiaaqaaiaad6 gaaiaawkWaaiabgwSixpaaHaaabaGaamyCaaGaayPadaGaaiykaiGa cwgacaGG4bGaaiiCaiaacUfacaWGQbGaam4DamaaBaaaleaacaWGJb aabeaakiaacIcacaWG0bGaeyOeI0IaamiDamaaBaaaleaacaWGZbaa beaakiaacMcacaGGDbGaeyiLdqKaamiEaiabgs5aejaadMhaaeaaca aI0aGaeqiWdaNaamOuamaaBaaaleaacaWGHbaabeaakiaadkfadaWg aaWcbaGaamOyaaqabaGccaWGUbWaaSbaaSqaaiaadQhaaeqaaaaaki aadAfacaGGOaGaeqiUde3aaSbaaSqaaiaaigdaaeqaaOGaaiykaaaa @6CC6@          (14)

where Lx represents the horizontal distance between the radiant source and the radar, h1 is the height of the radiant source, h2 is the height of the radar antenna. For a point on the sea, the height of the waves is represented by f(x,y), according to the results of three-dimensional simulation of the sea.


The angle between the incident component and the beam axis of the radiant target is , the angle between the diffuse reflection component and the beam axis of passive radar is , the pattern factors of the target’s antenna and the radar antenna are  and  respectively; the incident complementary angle of the signal on the unit sea surface is, similarly,is the reflective complementary angle; denotes the angle between the incident waves and the x-y plane,  denotes the angle between the reflective waves and the x-y plane; is the scattering coefficient of the sea, ,are the distances betweenand the target and radar, respectively, Rab is the distance between the target and radar; ,are the lengths of the two sides of the panels, is the unit normal vector of the panels, k is wave number, is the normal vector of the incident component, is the normal vector of the reflective component, and .


The model parameters above are calculated as follows:
The diffuse reflection coefficient of sea  
V( θ 1 )= P 1 ^ n ^ cos 2 θ 1 { V V cos(2 θ 1 )( n ^ P 2 ^ )sin θ 1 V V ( α ^ P 2 ^ ) } MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqipC0xf9vqqrpepeea0xXdHaVhbbf9v8qqaqFr0xc9pk 0xbba9q8WqFfea0=yr0RYxir=Jbba9q8aq0=yq=He9q8qqQ8frFve9 Fve9Ff0dmeaabaqaciaacaGaaeqabaWaaeaaeaaakeaacaWGwbGaai ikaiabeI7aXnaaBaaaleaacaaIXaaabeaakiaacMcacqGH9aqpdaWc aaqaamaaHaaabaGaamiuamaaBaaaleaacaaIXaaabeaaaOGaayPada GaeyyXIC9aaecaaeaacaWGUbaacaGLcmaaaeaaciGGJbGaai4Baiaa cohadaahaaWcbeqaaiaaikdaaaGccqaH4oqCdaWgaaWcbaGaaGymaa qabaaaaOWaaiWaaeaacaWGwbWaaSbaaSqaaiaadAfaaeqaaOGaci4y aiaac+gacaGGZbGaaiikaiaaikdacqaH4oqCdaWgaaWcbaGaaGymaa qabaGccaGGPaGaeyyXICTaaiikamaaHaaabaGaamOBaaGaayPadaGa eyyXIC9aaecaaeaacaWGqbWaaSbaaSqaaiaaikdaaeqaaaGccaGLcm aacaGGPaGaeyOeI0Iaci4CaiaacMgacaGGUbGaeqiUde3aaSbaaSqa aiaaigdaaeqaaOGaeyyXICTaamOvamaaBaaaleaacaWGwbaabeaaki abgwSixlaacIcadaqiaaqaaiabeg7aHbGaayPadaGaeyyXIC9aaeca aeaacaWGqbWaaSbaaSqaaiaaikdaaeqaaaGccaGLcmaacaGGPaaaca GL7bGaayzFaaaaaa@742F@          (15)

The incident complementary angle of the signal on the unit sea surface θ 1 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqipC0xf9vqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGacaGaaiaabeqaamaabaabaaGcbaGaeqiUde3aaS baaSqaaiaaigdaaeqaaaaa@3875@ is


sin( θ 1 )= α ^ n ^ MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqipC0xf9vqqrpepeea0xXdHaVhbbf9v8qqaqFr0xc9pk 0xbba9q8WqFfea0=yr0RYxir=Jbba9q8aq0=yq=He9q8qqQ8frFve9 Fve9Ff0dmeaabaqaciaacaGaaeqabaWaaeaaeaaakeaaciGGZbGaai yAaiaac6gacaGGOaGaeqiUde3aaSbaaSqaaiaaigdaaeqaaOGaaiyk aiabg2da9iabgkHiTmaaHaaabaGaeqySdegacaGLcmaacqGHflY1da qiaaqaaiaad6gaaiaawkWaaaaa@4525@       (16)

The normal vector of the incident wave α ^ MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqipC0xf9vqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGacaGaaiaabeqaamaabaabaaGcbaWaaecaaeaacq aHXoqyaiaawkWaaaaa@3839@   is denoted by:



α ^ =(cos θ 1 coas φ 1 ,cos θ 1 sin φ 1 ,sin θ 1 ) MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqipC0xf9vqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGacaGaaiaabeqaamaabaabaaGcbaWaaecaaeaacq aHXoqyaiaawkWaaiabg2da9iaacIcaciGGJbGaai4BaiaacohacuaH 4oqCgaqbamaaBaaaleaacaaIXaaabeaakiGacogacaGGVbGaaiyyai aacohacqaHgpGAdaWgaaWcbaGaaGymaaqabaGccaGGSaGaaGjbVlGa cogacaGGVbGaai4CaiqbeI7aXzaafaWaaSbaaSqaaiaaigdaaeqaaO Gaci4CaiaacMgacaGGUbGaeqOXdO2aaSbaaSqaaiaaigdaaeqaaOGa aiilaiaaysW7cqGHsislciGGZbGaaiyAaiaac6gacuaH4oqCgaqbam aaBaaaleaacaaIXaaabeaakiaacMcaaaa@5C82@       (17)

While the unit normal vector of the panels n ^ MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqipC0xf9vqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGacaGaaiaabeqaamaabaabaaGcbaWaaecaaeaaca WGUbaacaGLcmaaaaa@378D@ is: 


n ^ =( K 1 1+ K 1 2 + K 2 2 ,  K 2 1+ K 1 2 + K 2 2 ,  1 1+ K 1 2 + K 2 2 ) MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqipC0xf9vqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGacaGaaiaabeqaamaabaabaaGcbaWaaecaaeaaca WGUbaacaGLcmaacqGH9aqpdaqadaqaamaalaaabaGaam4samaaBaaa leaacaaIXaaabeaaaOqaamaakaaabaGaaGymaiabgUcaRiaadUeada qhaaWcbaGaaGymaaqaaiaaikdaaaGccqGHRaWkcaWGlbWaa0baaSqa aiaaikdaaeaacaaIYaaaaaqabaaaaOGaaiilaiaaykW7caqGGaWaaS aaaeaacaWGlbWaaSbaaSqaaiaaikdaaeqaaaGcbaWaaOaaaeaacaaI XaGaey4kaSIaam4samaaDaaaleaacaaIXaaabaGaaGOmaaaakiabgU caRiaadUeadaqhaaWcbaGaaGOmaaqaaiaaikdaaaaabeaaaaGccaGG SaGaaeiiamaalaaabaGaaGymaaqaamaakaaabaGaaGymaiabgUcaRi aadUeadaqhaaWcbaGaaGymaaqaaiaaikdaaaGccqGHRaWkcaWGlbWa a0baaSqaaiaaikdaaeaacaaIYaaaaaqabaaaaaGccaGLOaGaayzkaa aaaa@595F@      (18)     

The slopes K1, K2 of point (x, y) on the tangent plane towards x-axis and y-axis can be approximated by


K 1 = z x z( x m+1 , y n )z( x m1 , y n ) 2dx K 2 = z y z( x m , y n+1 )z( x m , y n1 ) 2dy MathType@MTEF@5@5@+= feaagKart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqipC0xf9vqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGacaGaaiaabeqaamaabaabaaGceaqabeaacaWGlb WaaSbaaSqaaiaaigdaaeqaaOGaeyypa0JaeyOeI0YaaSaaaeaacqGH ciITcaWG6baabaGaeyOaIyRaamiEaaaacqGHijYUcqGHsisldaWcaa qaaiaadQhacaGGOaGaamiEamaaBaaaleaacaWGTbGaey4kaSIaaGym aaqabaGccaGGSaGaamyEamaaBaaaleaacaWGUbaabeaakiaacMcacq GHsislcaWG6bGaaiikaiaadIhadaWgaaWcbaGaamyBaiabgkHiTiaa igdaaeqaaOGaaiilaiaadMhadaWgaaWcbaGaamOBaaqabaGccaGGPa aabaGaaGOmaiaadsgacaWG4baaaaqaaiaadUeadaWgaaWcbaGaaGOm aaqabaGccqGH9aqpcqGHsisldaWcaaqaaiabgkGi2kaadQhaaeaacq GHciITcaWG5baaaiabgIKi7kabgkHiTmaalaaabaGaamOEaiaacIca caWG4bWaaSbaaSqaaiaad2gaaeqaaOGaaiilaiaadMhadaWgaaWcba GaamOBaiabgUcaRiaaigdaaeqaaOGaaiykaiabgkHiTiaadQhacaGG OaGaamiEamaaBaaaleaacaWGTbaabeaakiaacYcacaWG5bWaaSbaaS qaaiaad6gacqGHsislcaaIXaaabeaakiaacMcaaeaacaaIYaGaamiz aiaadMhaaaaaaaa@774D@      (19)
Substituting Eqns. (17), (18) and (19) into Eqn (16), the incident complementary angle can be denoted by:
sin( θ 1 )= cos θ 1 ( K 1 cos φ 1 + K 2 sin φ 1 )+sin θ 1 1+ K 1 2 + K 2 2 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqipC0xf9vqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGacaGaaiaabeqaamaabaabaaGcbaGaci4CaiaacM gacaGGUbGaaiikaiabeI7aXnaaBaaaleaacaaIXaaabeaakiaacMca cqGH9aqpcqGHsisldaWcaaqaaiGacogacaGGVbGaai4CaiqbeI7aXz aafaWaaSbaaSqaaiaaigdaaeqaaOGaaiikaiaadUeadaWgaaWcbaGa aGymaaqabaGcciGGJbGaai4BaiaacohacqaHgpGAdaWgaaWcbaGaaG ymaaqabaGccqGHRaWkcaWGlbWaaSbaaSqaaiaaikdaaeqaaOGaci4C aiaacMgacaGGUbGaeqOXdO2aaSbaaSqaaiaaigdaaeqaaOGaaiykai abgUcaRiGacohacaGGPbGaaiOBaiqbeI7aXzaafaWaaSbaaSqaaiaa igdaaeqaaaGcbaWaaOaaaeaacaaIXaGaey4kaSIaam4samaaDaaale aacaaIXaaabaGaaGOmaaaakiabgUcaRiaadUeadaqhaaWcbaGaaGOm aaqaaiaaikdaaaaabeaaaaaaaa@62ED@      (20)

The normal polarization vectors of the incident wave and the reflective wave are


P 1 ^ n ^ = sin θ 1 ( K 1 cos φ 1 + K 2 sin φ 1 )+cos θ 1 1+ K 1 2 + K 2 2 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqipC0xf9vqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGacaGaaiaabeqaamaabaabaaGcbaWaaecaaeaaca WGqbWaaSbaaSqaaiaaigdaaeqaaaGccaGLcmaacqGHflY1daqiaaqa aiaad6gaaiaawkWaaiabg2da9maalaaabaGaci4CaiaacMgacaGGUb GafqiUdeNbauaadaWgaaWcbaGaaGymaaqabaGccaGGOaGaam4samaa BaaaleaacaaIXaaabeaakiGacogacaGGVbGaai4CaiabeA8aQnaaBa aaleaacaaIXaaabeaakiabgUcaRiaadUeadaWgaaWcbaGaaGOmaaqa baGcciGGZbGaaiyAaiaac6gacqaHgpGAdaWgaaWcbaGaaGymaaqaba GccaGGPaGaey4kaSIaci4yaiaac+gacaGGZbGafqiUdeNbauaadaWg aaWcbaGaaGymaaqabaaakeaadaGcaaqaaiaaigdacqGHRaWkcaWGlb Waa0baaSqaaiaaigdaaeaacaaIYaaaaOGaey4kaSIaam4samaaDaaa leaacaaIYaaabaGaaGOmaaaaaeqaaaaaaaa@61AF@      (21)
n ^ P 2 ^ = sin θ 2 ( K 1 cos φ 2 K 2 sin φ 2 )+cos θ 2 1+ K 1 2 + K 2 2 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqipC0xf9vqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGacaGaaiaabeqaamaabaabaaGcbaWaaecaaeaaca WGUbaacaGLcmaacqGHflY1daqiaaqaaiaadcfadaWgaaWcbaGaaGOm aaqabaaakiaawkWaaiabg2da9iabgkHiTmaalaaabaGaci4CaiaacM gacaGGUbGafqiUdeNbauaadaWgaaWcbaGaaGOmaaqabaGccaGGOaGa am4samaaBaaaleaacaaIXaaabeaakiGacogacaGGVbGaai4CaiabeA 8aQnaaBaaaleaacaaIYaaabeaakiabgkHiTiaadUeadaWgaaWcbaGa aGOmaaqabaGcciGGZbGaaiyAaiaac6gacqaHgpGAdaWgaaWcbaGaaG OmaaqabaGccaGGPaGaey4kaSIaci4yaiaac+gacaGGZbGafqiUdeNb auaadaWgaaWcbaGaaGOmaaqabaaakeaadaGcaaqaaiaaigdacqGHRa WkcaWGlbWaa0baaSqaaiaaigdaaeaacaaIYaaaaOGaey4kaSIaam4s amaaDaaaleaacaaIYaaabaGaaGOmaaaaaeqaaaaaaaa@62AC@      (22)
α ^ P 2 ^ =cos θ sin θ 2 cos( φ 1 + φ 2 )sin θ 1 cos θ 2 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqipC0xf9vqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGacaGaaiaabeqaamaabaabaaGcbaWaaecaaeaacq aHXoqyaiaawkWaaiabgwSixpaaHaaabaGaamiuamaaBaaaleaacaaI YaaabeaaaOGaayPadaGaeyypa0JaeyOeI0Iaci4yaiaac+gacaGGZb GafqiUdeNbauaaciGGZbGaaiyAaiaac6gacuaH4oqCgaqbamaaBaaa leaacaaIYaaabeaakiGacogacaGGVbGaai4CaiaacIcacqaHgpGAda WgaaWcbaGaaGymaaqabaGccqGHRaWkcqaHgpGAdaWgaaWcbaGaaGOm aaqabaGccaGGPaGaeyOeI0Iaci4CaiaacMgacaGGUbGafqiUdeNbau aadaWgaaWcbaGaaGymaaqabaGcciGGJbGaai4BaiaacohacuaH4oqC gaqbamaaBaaaleaacaaIYaaabeaaaaa@5F80@      (23)

Finally, the total diffuse signal can be calculated by summing all the diffuse signals which can be received by the radar antenna


S d i f f = m = 1 M n = 1 N E m n MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqipC0xf9vqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGacaGaaiaabeqaamaabaabaaGcbaGaam4uamaaBa aaleaacaWGKbGaamyAaiaadAgacaWGMbaabeaakiabg2da9maaqaha baWaaabCaeaacaWGfbWaaSbaaSqaaiaad2gacaWGUbaabeaaaeaaca WGUbGaeyypa0JaaGymaaqaaiaad6eaa0GaeyyeIuoaaSqaaiaad2ga cqGH9aqpcaaIXaaabaGaamytaaqdcqGHris5aaaa@49F9@      (24)

where M, N are the numbers of the effective panels towards x-axis and y-axis, respectively.


 

All the simulations in this section are implemented using MATLAB on an Intel Pentium 3GHz Dual-Core CPU, and 2GB RAM computer, while the test data are obtained by the experiments in the outfield using an X-band passive radar.


5.1   Dynamic Sea Surface


According to the wind speed of the sea surface, generally the sea surface can be classified as six kinds: wavelet, light waves, middle waves, big waves, billows and fierce waves. Based on the three-dimensional model of the sea, two typical situations of the sea (wavelet, light waves) are compared with simulations.


Figure 5. shows the simulation results of the dynamic sea surface under two wind speeds (5 m/s and 10 m/s). The parameters of the simulations are as follows: the ranges of the frequency are 1.2~6.0 rad/s and 0.4~2.5 rad/s, respectively. The stepping frequency intervalsare 0.2 rad/s and 0.1 rad/s, respectively. The numbers N of harmonics are 24 and 21, respectively, while the simulation regions of the sea surface are both.


Figure 5. Simulation results of the dynamic sea surface (a) wind speed - 5 m/s and (b) wind speed - 10 m/s.


From the comparisons between the results of the dynamic sea surface under two wind speeds, it can be seen that the conditions of the sea change significantly with the wind speed, which will result in different influence on the multipath effects. The undulant extent of the sea surface is small with relatively stable waves when the wind speed is 5 m/s, while the undulant extent is increasing when the wind speed is 10 m/s and the waves are wandering in the wave crest and trough. The simulation results illustrate that the low-frequency spectrum of waves are significant increasing when the wind speed increases which is consistent with the actual situations of the sea.


5.2  Results in the Outfield


In the outfield experiment, an X-band passive radar which is placed on the seawall is used to take measurements of the microwave radiant source placed on the target ship. The target ship moves from near to far relative to the detector (the X-band radar). The microwave interferometer is used to measure the angle of the target. The length of baseline between two antennae of the passive radar is 0.146 m. The gain of the antenna is 20 dB. The 3 dB width of the microwave radiant source and the radar antenna are 17°and 60°, respectively. The initial distance between the microwave radiant source and the radar is 1km, while the total test distance is 14km. The wind speed on the sea is 7 m/s (light waves) and the speed of the ship is 5m/s. The heights of the radar antenna and the microwave radiant source are 8.2 m and 4.1 m, respectively. The radar works under the low-elevation tracking state. The experiment scenery in the outfield is illustrated in Fig. 6.


Figure 6. Experiment scenery in the outfield.


In the experiment, the power – range curve of the received signal is given in Fig. 7. A spectrum analyzer placed on the seawall is used to measure the power of the received signal. The unit of the signal power is dBmw. The measurements indicate that during the experiment, the power of the received signal encountered two significant drops: one is at 2 km due to the influence of multipath effects and the other is after 9 km which is caused by the serious signal loss.


Figure 7. Power – range curve of the received signal.


5.3   Evaluation of the Model of Multipath Propagation


The outfield test data measures the power of the signals received by the passive radar. In the test radar, there is a fixed ratio between the voltages of received signal and the angle of target, which is 0.3 volts per degree. According to such a ratio, the angle measurement of the target can be calculated by the power of the received signals, while the true angle of the target can be calculated from the geometry of the experiment. On the other hand, the estimation or prediction results of the multipath propagation can be obtained based on the model proposed in this paper. Therefore, the model can be validated by the test data.


Comparison between the results of predictions of the multipath propagation based on the multipath model and the results of experiments are presented. Fig. 8. gives three simulated components of the signals received by two antennae of the passive radar. The signals of each radar antenna are vectorially summed to calculate the target angle. Figures 9 - 11 give three comparisons between the predictions of the target angle in the presence of the multipath reflections from the sea and the angles measured in the experiment. The three comparisons consider only specular reflection, diffuse reflection and all the two components of reflections, respectively. The x-axis in the figures denotes the distance between the target and the radar antenna, while the y-axis denotes the elevation angle of the radiant source (in degrees).


Figure 8. The three components of the signals received by two antennae of the passive radar.


In the simulations,Fig. 9. shows that the angle simulated according to the proposed model has a big drop at 2 km when only the specular reflection is considered, which agrees with the test data well. It changes gently at the other regions and has no oscillations. Fig. 10. shows that the angle simulated is consistent with the measured angle of target when only the diffuse reflection is considered. There is no fixed bias. However, the diffuse reflection component causes oscillations to the angle measurement, and reduces the measurement accuracy. Fig. 11. shows that when all the two components are considered, the model provides an accurate prediction of the angle measurement errors in the presence of multipath effects.


Figure 9. Results considered only specular reflection.


Figure 10. Results considered only diffuse reflection.


Figure 11. Results considered all of the reflection components.


The three simulations presented above indicate that the specular reflection causes large peak errors followed by an approximately constant bias in tracking low elevation targets in the presence of multipath reflections, while the diffuse reflection has random variations on the average a bias. In other words, while the specular reflection coefficient is a deterministic number depending on several unknown parameters, the diffuse reflection has a random nature. Generally, the sea surface is perturbed by small irregularities. Therefore, both reflection components are present. In practice, the specular reflective component has greater impact than the diffuse reflection and will cause a great angle measurement error. The impact of diffuse component is limited to oscillations which have little big deviation but it will reduce the angle measurement accuracy. According to test results, there are two big regional power drops during the test which are well predicted by the proposed model of the multipath effects. The results indicate that the first drop at about 2 km is mainly caused by the signal interference between the specular reflective component and direct wave component, while the second drop after 9 km is mainly because the target is far away and the signal is weaker.

A detailed model of the multipath propagation of low elevation target tracking using passive radars was presented in this paper. It had taken into account both types of reflections (the specular and the diffuse reflection components). The effect of multiple reflections from the sea surface was analyzed. Based on the geometry of the specular and the diffuse reflections, expressions for the reflection coefficient and the scattering field were derived. Experiments in the outfield indicate that the model proposed agrees with the test data well, which can provide an accurate prediction of the angle measurement errors in the presence of multipath effects. The result provides a reference to the detection and tracking of ship-borne radiation sources using anti-ship missile passive radar seekers.

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Dr Yuliang Qin received his MS and PhD (Information and Communication Engineering) from the National University of Defense Technology (NUDT), Changsha, China, in 2004 and 2008 respectively. He is currently working as an Associate Professor in the School of Electronic Science and Engineering, NUDT. His research interests are : Radar signal processing and radar systems.

Dr Yongqiang Cheng received his BS, MS, and PhD (Information and Communication Engineering) from NUDT, Changsha, China, in 2005, 2007, and 2012, respectively. He is currently working as a Lecturer at NUDT, China. His research interests include: Information geometry and statistical signal processing.