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Impact of Elevated M-inversions on the UHF/EHF Field Propagation beyond the Horizon

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Explore the impact of elevated M-inversions on UHF/EHF field propagation beyond the horizon, examining atmospheric effects and anomalous radio frequency behavior.

The elevated refractive layer, the so-called M-inversion, is frequently associated with an anomalousy high level of the received signal at UHF frequencies over the horizon. It is apparent that the methods of prediction of either the parameters of the elevated layer or the signal level are needed in many applications, such as radar, surveillance and communications.

The methods of the analytical solutions to the problem of wave propagation in the presence of elevated M-inversion are less well developed than those applied to propagation in an evaporation duct. The major reason for this is that such a waveguide has a multi-mode or multi-ray nature that, in turn, may require a different approach to obtaining the analytical solution, depending on the geometry of the problem (positions of the transmitter and receiver relative to the elevated duct “boundaries”, range and frequency).

For instance, when the transmitter and receiver are based close to the ground with the distance between them
x22aZi,
see Figure 1, where Zi is the height of the minimum in the M-profile of the refractivity, the most effective approach is to apply the method of multiple reflections, that, in turn leads to the approximation of the geometrical optic with k → ∞. In contrast, at longer distances, the most effective method uses normal waves providing the modal representation of the wave field.

In a sub-tropical region of the world’s oceans both evaporated and elevated ducts may exist simultaneously thus complicating the situation. In Refs this situation is analysed by applying the normal wave method to the M-profile approximated by a piece-wise linear profile. An alternative approach is described in Hybrid Representation in Action: Fock’s Contour Integral and the Attenuation Factor“Exploring Hybrid Representation for the Attenuation Factor”, where the contribution of evaporation duct is presented by trapped modes while the reflection from elevated M-inversion is analysed in terms of geometric optics.

The modal representation of the wave field for the case of elevated M-inversion is presented in this article. Hybrid Representation in Action: Fock’s Contour Integral and the Attenuation Factor“Exploring Hybrid Representation for the Attenuation Factor” introduces the hybrid, ray and modes, representation of the wave field in the problem of a two-channel system. Some results of the measurements versus prediction are discussed in Comparison of Experimental Results with the Deterministic Theory of Elevated Duct Propagation“Deterministic Theory and Results of Elevated Duct Propagation” and, finally, in Comparison of Experimental Results with the Deterministic Theory of Elevated Duct Propagation“Deterministic Theory and Results of Elevated Duct Propagation”, we introduce a method of estimating the excitation of the elevated duct due to scattering of the direct wave on the fluctuations in refractivity in the vicinity of the upper boundary of the atmospheric boundary layer.

Modal Representation of the Wave Field for the Case of Elevated M-inversion

Consider a piece-wise linear model of the M-profile as shown in Figure 1 and introduce the dimensionless coordinates ξ = mx/a, h = kz/m.

Dimensionless coordinates
Fig. 1 Piece-wise linear approximation of the M-profile with two M-inversions

The parameters of the M-profile can be expressed in terms of h-coordinates and the scaled potential U(h) = 2m210-6M(z):

  • Hk = kZk/m;
  • Hi = kZi/m;
  • Hs = kZs/m;
  • Uk = 2m210-6M(Zk);
  • Ui = 2m210-6M(Zi);
  • U0 = 2m210-6ΔM.

Let us also introduce the gradients of the M-profile in each of the layers between Zs, Zi and above Zk respectively:

  • G2 = dM/dz, with Zs < z < Zi;
  • G4 = dM/dz, with z > Zk.

The respective gradients of the dimensionless profile U(h) are given by:

μ13=U0/Hs,   μ23=a·106G2,    μ33=UiUk/HkHi,     μ43=a·106G4.

Following the approach described in Understanding Parabolic Approximation in Wave Propagation: Analytical Methods and Applications“Parabolic Approximation to the Wave Propagation”, we expand the attenuation factor W(ξ, h, h0) over the set of eigenfunctions of a continuum spectrum. Using the results of Green Function for a Parabolic Equation in a Stratified Medium“Parabolic Approximation to the Wave Propagation” and introducing the dimensionless “energyt = m2E/k2 we obtain:

Wξ, h, h0=ejπ4dtΨt, hΨ*t, h0ejξt            Eq. 1

where the eigenfunction Ψ(t, h) obeys the equation:

d2Ψdh2+UhtΨ=0            Eq. 2

and the boundary conditions:

Ψt, 0=0   and  Ψt, =0.            Eq. 3

As known from analogy with a quantum-mechanical problem, the solution to Eq. (2) is given by a superposition of the waves, outgoing (χ+) to infinity (h → ∞) and incoming (χ) from infinity:

Ψt, h=12πμ4χt, hStχ+t, h.            Eq. 4
It is also observed that χ(t, h) = (χ+(t, h))*, where the sign * indicates a complex conjugate. The factor
12πμ4
in Eq. (4) comes from a delta-function normalisation of the eigenfunction of the continuum spectrum, Understanding Parabolic Approximation in Wave Propagation: Analytical Methods and Applications“Green Function for a Parabolic Equation in a Stratified Medium”. From the boundary condition (3) we have:
St=χt, 0χ+t, 0.                Eq. 5

Given the linear approximation to the M-profile in each of the layers: Hs < h ≤ Hi Hs < h ≤ Hi, Hi < h ≤ Hk and h > Hki the solution for χ± can be presented via superposition of the Airy–Fock function. Taking into account the continuity of both the function v and its derivative at the boundaries of the layers with constant gradient of U(h), the outgoing wave can be written as follows:

1 With h > Hk:

χ+h=w1tUhμ42.                Eq. 6

2 with hk ≥ h > hi:

χ+h=Aw1tUhμ32+Rkw2tUhμ32                Eq. 7

where:

A=w2xk+w1xk+Rkw2xk,               Eq. 8
Rk=w2xk+Qkw2xkw1xk+Qkw1xk.               Eq. 9

Here:

xk+=tUkμ42,   xk=tUkμ32,   Rk

is a reflection coefficient of the wave incident to the boundary h = Hk from h < Hk, the parameter Qk is the surface impedance at the boundary h = Hk and is given by:

Qk=μ4μ3w1xk+w1xk.                Eq. 10

3 with Hi ≥ h > Hs:

χ+h=Bw1tUhμ22+Riw2tUhμ22                Eq. 11

where:

B=Aw2xi++Rkw1xi+w1xi+Riw2xi,                Eq. 12
Ri=w1xi+Qiw1xiw2xi+Qkw2xi,                Eq. 13
Qi=μ3μ2w1xi++Rkw1xi+w2xi+Rkw2xi,                Eq. 14

Here:

xi+=tUi/μ32,   xi=tUi/μ22,

the other parameters have the same meaning as above.

4 With h ≤ Hs:

χ+h=Cw2tUhμ12+Rsw1tUhμ12                Eq. 15

where:

C=Bw1xs++Riw2xs+w2xs+Rsw1xs,                Eq. 16
Rs=w2xs+Qsw2xsw1xs+Qsw1xs,                Eq. 17
Qi=μ2μ1w1xs++Riw1xs+w2xi+Rkw2xi.                Eq. 18
Here
xs+=τ/μ22, xs=τ/μ12,
, the other parameters have the same meaning as above.

The solution to W(ξ, h, h0) is obtained in principle and given by Eqs. (1)–(18). However, the direct calculation of Eq. (1) is not practical because of the problem of convergence. Therefore, a significant amount of research has been dedicated to finding effective methods of calculating the electromagnetic field in the presence of elevated M-inversion.

Here we consider a modal representation of the attenuation function W(ξ, h, h0) in a two-channel system when both elevated and surface-based M-inversion are present. In this approach, UHF Propagation in an Evaporation Ductthe integral is calculated as a sum of the residue at the poles of the S-matrix in the upper half-space of variable t. Taking into account Eqs. (5)–(18) we obtain the expression for the S-matrix in this particular problem:

S=RgA*w22xs·1Ri*Ts·1Ri*Ts+·1Ri*Rg*Aw12xs·1RiTs+·1RiTs·1RiRg             Eq. 19

where:

  • Rg = -w1(x0)/w2(x0) is the reflection coefficient of the ground;
  • x0=tU0/μ12,  Ts+=w2xs+/w1xs

    is the reflection coefficient of the wave incoming from the upper space from the boundary h = Hs with ideal boundary conditions on it;

  • Ts=w1xs/w2xs+

    is a similar coefficient of reflection from the boundary h = Hs,but for the wave incoming from the space below the boundary h = Hs.

The resonant terms in the denominator of the S-matrix determine the spectrum of the normal waves in a two-channel system. Apparently, the propagation constants of the normal waves are defined by the position of the poles of the S-matrix in the t-plane. The waves trapped in an evaporation duct (surface-based M-inversion) have propagation constants tn in the interval Re tn ∈ (0, U0). Waves localised in the elevated duct between Hs and Hk have propagation constants tn in the interval Re tn ∈ (0, Ui). And, finally, the normal waves localised in a channel formed by the ground surface h = 0 and the upper boundary of the elevated layer h = Hk are in the interval Re tn ∈ (Uk, 0).

Now we consider the resonant terms of the S-matrix in more detail and assume that Uk > 0. The resonant term
1RiTs+
determines the spectrum of the normal waves for the elevated channel with boundaries h = Hs and h = Hk. With U0 ≠ 0 localisation of the modes in the surface-based channel is possible, in principle, and the spectrum of these modes is defined by the equation 1 – RsRg = 0. In the case where UkU0, both series of propagation constants are clearly separated in the wave-number space. More detailed analysis of this case is provided in Hybrid Representation in Action: Fock’s Contour Integral and the Attenuation Factor“Exploring Hybrid Representation for the Attenuation Factor”. Now we concentrate on the modes of the elevated channel (duct). The characteristic equation for the spectrum of propagation constants is given by:
1RiTs+=0.                Eq. 20
With
τ/μ221
we can estimate:
Ts+=1+Oe43tn3/2/μ22

and Eq. (20) can then be reduced to 1+Ri = 0. Assume that the propagation constants of interests are such that:

Re tnUk/μ221.

These normal waves experience complete reflection from the boundary h = Hk, in fact the respective rays turn back long before reaching the boundary Hk. The reflection coefficient can then be estimated as Rk ≈ -1. Taking into account Eq. (12) for Ri we can obtain instead of Eq. (20) the following characteristic equation for the waves trapped in an elevated duct:

vxi+qivxi=0             Eq. 21

where:

qiμ3/μ2 vxi+/vxi+, vx=1/2jw1xw2x.

Equation (21) can be further simplified using the asymptotic formulas for the Airy function v. The result is given by:

sin ςi++ςi+π2=0,           Eq. 22

where:

ςi+=23μ33Uit3/2,     ςi=23μ23Uit3/2.

The solution to Eq. (22) provides a spectrum of the propagation constants tn of the elevated duct:

tn=Ui32μ2μ33μ23+μ33πn122/3.            Eq. 23

As observed, Eq. (23) is obtained by neglecting the leaking of the modes into the space outside the duct. The number N1 of trapped modes is limited by the condition tn > Uk, therefore:

N1=entier 23μ23+μ33μ2μ3UiUk3/2+12.           Eq. 24
Counting the next terms of the asymptotic for both
Ts+
and Rk we can obtain from Eq. (20) some correction terms to the propagation constants tn (23). These correction terms provide an estimate for a phase shift and attenuation factor for the modes due to the limited thickness of the potential barrier. Omitting the simple but cumbersome calculations we provide the final result for the imaginary part of the propagation constants:
γn=Im tn=14μ23+μ33μ2μ33 exp 43μ33+μ43μ3μ43tnUk3/2.           Eq. 25

Let us consider another situation and assume now that Uk < 0. We pay attention to the modes of the channels formed by the earth’s surface h = 0 and the upper boundary of the M-inversion, h = Hk. As discussed above, the propagation constants of these modes lie in the interval Re tn ∈ (Uk, 0). The spectrum of the propagation constant is determined by the characteristic equation 1 – RsRg = 0. Using asymptotic expressions for Airy functions we obtain:

RsRiDejδ,           Eq. 26
Rgexp jπ2+j43μ13U0t3/2

where:

δ=π+43μ23+μ33μ23μ33t, D=12RiTs+,
Ts+exp jπ2j43μ23t3/2.

Let us expand the term D into a series:

D=m=01m 1RiTs+m.         Eq. 27

The series (27) takes into account the multiple effect of secondary reflection of the waves in the channel Hs ≤ h ≤ Hk due to a leakage of the energy of the normal waves localised in the channel 0 < h ≤ Hk due to partial reflection from the boundary h = Hs. In the first and rough approximation this effect of mutual coupling of two channels can be neglected, at least this approximation will be good enough for |Re tn| ≫ 1. Under this condition we can retain only the first term in series (27). As a result we obtain:

1RsRg1RiRgejδ=0.         Eq. 28

The last equation can be further simplified to the form:

23μ23+μ33μ23μ33Uitn3/2+23μ13U0tn3/223μ23+μ13μ23μ13tn3/2=πn14.         Eq. 29

The limiting case when surface M-inversion is absent is accounted for by Eq. (29) if we assume that U0 = 0. We can also observe that the number n satisfying Eq. (29) starts from n = N1 + N2 + 1, where N2 is the number of modes trapped in a surface-based channel, 0 < h ≤ Hs.

To conclude, we may state that the characteristic equations (20) and (29) determine the limited, yet large, (for high frequencies and strong inversions of temperature) set of trapped modes in a two-channel system. While in the general case the two modal series in the evaporation and the elevated duct are coupled, for modes localised deep in respective channels the mutual coupling can be neglected in the first approximation. In this way, the trapped modes of the evaporation duct can be estimated as the modes formed by a surface-based inversion only, Fig. 2, and the analysis is similar to that provided in UHF Propagation in an Evaporation Duct“Exploring UHF Propagation in Evaporation Ducts”.

Surface-based inversion
Fig. 2 Isolated surface-based M-inversion

Let us obtain a residue of the integrand in Eq. (1) in the pole of the S-matrix. Utilising the asymptotic expression for Airy functions incorporated into Ψ(t, h) and Ψ*(t, h0), the residue with Re tn > Uk is truncated to:

Re s Ψt, hΨ*t, h0 t=tn=2j Im tnχ+tn, hχ+tn, h0         Eq. 30

Next we obtain an asymptotic expression for the height-gain functions χ+(tn, h). First, define the coefficients (8) and (12) for Re tn > Uk:

Atnjμ4μ3exp 2         Eq. 31

where:

=43μ33+μ43μ33μ43tnUk3/2

and, for Re tn > 0:

BtnAμ3μ21cos nπ            Eq. 32

For 0 > Re tn > Uk:

Btn2jμ3μ2 sin 32μ23Uitn3/2+π4 1exp j43μ23Uitn3/2+jπ2 · exp j23μ23Uitn3/2jπ4.          Eq. 33

While obtaining Eq. (32) we take into consideration that Ri(tn) = -1 at the pole. Assume that there is no evaporation duct present, i. e. Hs = 0, U0 = 0, and consider a height-gain function χ(tn, h) with h → 0 for 0 > Re tn > Uk. As follows from Eq. (11):

χ+tn, h=0=2B cos S1δ exp jδ          Eq. 34

where:

S1=23μ23tn3/2+π4, δ=23μ23+μ33μ23μ33Uitn3/2.

Taking into account that at the pole, as follows from Eq. (22) with U0 = 0, the arguments of the cosine in the term S1 – δ = -nπ + π/2, we obtain the boundary condition of interest, χ+(h = 0) = 0. With U0 ≠ 0 and Re tn < 0, from Eq. (15) it follows that:

χ+tn, 0cos 23μ13U0tn3/223μ13+μ23μ13μ23tn3/2π4.               Eq. 35

The equation for the poles takes the form RsRg = 1 in this case. The relationship between Rs and Rg is given by Eq. (26) from which we obtain that the argument of the cosine in Eq. (35) has the value nπ + π/2 at the pole and, therefore χ+(tn, 0) = 0.

In the case of positive Re tn > 0, |tn| ≫ 1, the behavior of the height-gain function χ+(tn, h) with h → 0 is governed by the exponent factor:

χ+tn, h h0exp23μ23tn3/20

and the boundary condition at h = 0 is satisfied asymptotically.

Finally, we can present an explicit expression for the attenuation function W(ξ, h, h0) over the sum of the normal waves that can be used for computer calculation:

Wξ, h, h0=ejπ/4ξπ14μ4μ23μ33μ23+μ33 n=1N ejξtnγnξ χnh χnh0.           Eq. 36

The number of trapped modes N is determined by the number of real roots of Eqs. (22) and (29). The eigenfunction χn(h) is given by the following equations:

1 with h > Hk:

χnh=w1tnUhμ42 exp 2.           Eq. 37

2 with Hk > h ≥ 0:

χnh=2μ4μ3vtnUhμ32.           Eq. 38

3 with Hi > h, tn > 0:

χnh=2jBtnvtnUhμ22.           Eq. 39

and for Hi > h ≥ Hs, tn < 0:

χnh=Btnw1tnUhμ22+Ritnw2tnUhμ22.           Eq. 40

The factor B(tn) is defined by Eqs. (32) and (33).

4 with Hs > h, tn < 0:

χnh=μ1ςn1/4 vμ1hςn,           Eq. 41

where:

ςn=μ1Hstn/μ12.
The representation (36) is valid in a “geometric shadow” region, i. e. at a distance exceeding the maximum length of the cycle of the trapped modes
Λmax~22aZi.
. In the opposite case, at distances less than Λmax, the “leak” modes of a higher order provide a substantial contribution to the sum of the normal waves.
Graph: M-profile
Fig. 3 M-profile

These modes, though attenuating with distance, are not localised in the elevated duct, their amplitude grows exponentially with the order of the mode. The sum of leaked modes converges slowly as a result of interference of these modes. This leads to a need for precise determination of the relative phases of the modes and, in turn, to a sophisticated calculation of the complex propagation constants. An alternative method to calculate the field at the “line-of-sight” distance x < Λmax is to use the method of stationary phase applied directly to integral (1).

Read also: Excitation of Waves in a Continuous Spectrum and Evaporation Duct with Two Trapped Modes

In a transition region at distances close to Λmax, the most practical approach is to use interpolation over values of the attenuation function obtained in either region. While the asymptotic expression can be obtained for the transition region it is very cumbersome and practically does not provide significant advantage over a simple interpolation.

To illustrate the modal representation described in this section, we apply the above formulas to the case of radio wave propagation at wavelength λ = 9,1 cm in a surface based tropospheric duct created by M-profile, shown in Figure 3. Figure 4 shows the range dependence of the received signal strength at two elevations: 100 and 500 m.

Graph: range dependence
Fig. 4 Range dependence of the received field at the wavelength 9,1 cm inside the duct (1) and above the duct (2)

The calculated signal strength clearly illustrates the multimode character of the field inside the duct at the height 100 m and the contribution of a few modes only for the receiving antenna above the duct (at 500 m). Figure 5 shows the impact on the radar coverage diagram at 10 GHz in case of the above tropospheric duct. It is observed that strong ducting mechanism allows for a target detection at the distances of several hundred miles.

Signal coverage
Fig. 5 Coverage diagram for 10 GHz source at 30,5 m for the surface-based duct formed by M-profile in Figure 3. The return path loss is 220 dB
Author
Author photo - Olga Nesvetailova
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Literature
  1. Jensen, N.O., Lenshow, D.H. An observational investigation on penetrative convection. J.Atmos.Sci., 1978, 35(10), 1924–1933.;
  2. Monin, A.S., Yaglom, A.M. Statistical Fluid Mechanics, Vol.1, MIT Press, Cambridge, MA, 1971, p. 769.;
  3. Gossard, E.E. Clear weather meteorological effects on propagations at frequencies above 1 GHz, Radio Sci., 1981,16(5), 589–608.;
  4. Tatarskii, V.I. The Effects of Turbulent Atmo- sphere on Wave Propagation, IPST, Jerusalem, 1971.;
  5. Gavrilov, A.S., Ponomareva, S.M. Turbulence Structure in the Ground Level Layer of the Atmosphere. Collected Data, Meteorology Series, No.1, Research Institute for Meteorological Information, Obninsk (in Russian), 1984.;
  6. Kukushkin, A.V., Freilikher, V.D. and Fuks, I.M. Over-the-horizon propagation of UHF radio waves above the sea , Radiophys. Quantum Electron. (translated from Russian), Consultant Bureau, New York , RPQEAC 30 (7), 1987, 597–620.;
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