Open access peer-reviewed chapter

# Some Recent Advances in Nonlinear Inverse Scattering in 2D: Theory and Numerics

By Valery Serov, Markus Harju and Georgios Fotopoulos

Submitted: October 13th 2015Reviewed: January 12th 2016Published: July 6th 2016

DOI: 10.5772/62233

## Abstract

We survey our recently published results concerning scattering problems for the nonlinear Schrödinger equation

### Keywords

• Inverse scattering
• Schrödinger equation
• Born approximation
• numerical solution
• linear inverse problem

## 1. Introduction

We deal with the generalized nonlinear Schrödinger equation:

itExt=-Ext+hxEExt,E2000

where E denotes the electromagnetic field in two-dimensional case, ∆ is the two-dimensional Laplacian and h describes in a general form the nonlinear contribution to the index of refraction. Considering harmonic time dependence E(xt) = e− iωtu(x) with frequency ω > 0, we obtain the steady-state nonlinear equation with fixed energy:

-Δux+hxuux=k2ux,E1

where k2 = ω and fixed, and u denotes the complex amplitude of the field. Concerning the nonlinearity h(xs), we pose the basic assumptions.

1. hxscραx,αLσp2,0sρ,

2. hxs1-hxs2cρβxs1-s2,βLσp2,0s1,s2ρ,

where cρ and cρare constants and

σ>2-2/p,1<p.E2

Here, Lσp2denotes the weighted Lebesgue space with the norm.

fp,σ=21+|x|pσ|fx|pdx1/p,fp=fp,0.E5000

The main practical example (it can be considered as the motivation of this research) of such type equations (1) is the equation of the form:

-Δux+q1xux+q2xux21+rux2ux=k2ux,E3

with real number k, complex valued function q1(x) ∈ L2 and real-valued function q2(x) ∈ L2, and parameter r ≥ 0. A particular nonlinearity in (3) of cubic type (r = 0) can be met in the context of a Kerr-like nonlinear dielectric film, while the case when r > 0 corresponds to the saturation model (see [14]).

We consider the inverse scattering problems for (1). For these purposes, we are interested of the scattering solutions to (1), i.e. solutions of the form

uxkθ=u0xkθ+uscxkθ,E4

where θ𝕊1, the unit sphere in 2, u0(xkθ) = eik(x,θ) is the incident wave and usc(xkθ) is the scattered wave. The scattered wave must satisfy the Sommerfeld radiation condition at infinity:

limrruscxkθr-ikuscxkθ=0,r=x,E8000

for fixed k > 0 and uniformly in θ𝕊1. In that case, these solutions are the unique solutions of the Lippmann-Schwinger equation.

uxkθ=u0xkθ-2Gk+x-yhyuykθuykθdy,E5

where Gk+is the outgoing fundamental solution of the operator − ∆ − k2, i.e. the kernel of the integral operator (−∆ − k2 − i0)− 1. It is equal to

Gk+x=i4H01kx,E10000

where H01denotes the Hankel function of order zero and first kind.

The following main results concerning the direct scattering problem were proved in [5].

Under the basic assumptions and (2) for h, it is proved that for any ρ > 1 there is k0 > 0 such that for any k ≥ k0 in the ball Bρ=uL2:uρ,there is a unique scattering solution (or the solutions of the form in (4) to (5) which satisfies the condition:

|usc|0,kE6

uniformly in θ𝕊1. What is more, the solution is obtained as the limit

uxkθ=limjujxkθ,E12000

where

uj+1xkθ=u0xkθ-2Gk+x-yhyujykθujykθdy,E13000

for j = 0, 1, … with u0 as above. Let the function h have the same properties as above, but now with

σ>2-2/p,4/3p1/2,1<p<4/3.E7

Then for fixed k ≥ k0, the solution u(xkθ) admits the representation

uxkθ=eikxθ-1+i4πkxeikxAkθθ+ox-1/2,x.E15000

The function A(kθ′, θ) is called the scattering amplitude and it is defined as

Ak,θ,θ=2e-ikθyhyuykθuykθdy,E16000

where θ'=x|x|𝕊1is the direction of observation. This function A gives us the scattering data for inverse problem. More precisely, the inverse problem that is considered here is to extract some information about the function h by the knowledge of the scattering amplitude A for different sets of scattering data. There are four well-known inverse scattering data sets: (i) the full (scattering) data:

D=Akθθ:k>0,θ,θ𝕊1,E17000

(ii) the backscattering data:

DB=Akθθ:k>0,θ=-θ𝕊1,E17000

(iii) the fixed angle data:

DA=Akθθ:k>0,θ=θ0fixed,θ𝕊1E18000

and (iv) the fixed energy data:

DE=Akθθ:k=k0>0fixed,θ,θ𝕊1.E46000

We use the following notations for the direct and inverse Fourier transforms:

Ffξ=2eiξyfydyE8
F-1fx=12π22e-iξxfξdξ,E9

where (ξ, x) denotes the inner product in 2, i.e. (ξx) = ξ1x1 + ξ2x2. By C > 0, we denote a generic constant that may change from one step to another. By Ht2=W2t2,twe denote the standard L2 based Sobolev space. A weighted Sobolev space Wp,σ12is defined here by

Wp,σ12=fLσp2:fLσp2.E46000

The following notation for the characteristic function is used:

χAx=1,xA0,xA.E21000

## 2. Inverse scattering problems

The direct scattering theory described above can also be reversed. The inverse scattering theory treats the function h as unknown and attempts to recover it from the knowledge of the scattering amplitude A for different data. Usually, the model in (1) is probed with one or more incident plane waves u0 and the resulting scattered waves are measured at a distance. This gives rise to several different scattering data sets which can be used to recover the unknowns.

The inverse backscattering problem for (1) was treated in [6]. Also for (1), the recovery of unknown function h is possible from the full scattering data. In addition to the two-dimensional studies mentioned above, certain particular nonlinear cases of (1) have been investigated in other dimensions too. In one-space dimension, we refer to [7] and the references therein. In higher dimensions n ≥ 3 we are only aware of [8,9]. Similar problems with formally more general equation but with bounded h are considered in [10] and [11].

Our point of view is that the nonlinearity may contain local singularities in the space coordinate x, and therefore we work in the frame of weighted Lebesgue spaces. These local singularities can be recovered from the scattering amplitude using the method of Born approximation. As a unifying result, we obtain mathematically more general results that have far wider applicability in physical experiments.

Let us set

h0x=hx1.E22000

In the subsections that follow we consider the inverse problems of recovering information about h0 from the knowledge of full data D, backscattering data DB, fixed angle data DA and fixed energy data DE.

### 2.1. Full scattering data

The inverse problem with full data D was investigated in [5]. Here we summarize the main results without proofs.

Theorem 1 (Saito’s formula). Under the basic assumptions and (7) for the function h we have,

limkk𝕊1×𝕊1e-ikθ-θ,xAkθθdθdθ=4π2h0yx-ydy,x2,E23000

where the limit is valid in the sense of distributions for 4/3 < p ≤ 2 and pointwise (even uniformly) for 2 < p ≤ ∞.

Corollary 1 (Uniqueness). Let σ be as in (7). Consider the scattering problems for two sets of potentials h and h̃. If the scattering amplitudes coincide for some sequence kj → ∞ and for all θ′, θ𝕊1, then

h0x=h0̃xE24000

holds in the sense of distributions for 4/3 < p ≤ ∞.

Corollary 2 (Representation formula). Let σ be as in (7). Then the representation

h0x=limkk28π2𝕊1×𝕊1e-ikθ-θ,xAkθθ|θ-θ|dθdθE25000

holds in the sense of distributions for 4/3 < p ≤ ∞.

Remark 1. In addition to providing the above results, Saito’s formula might be applied numerically too. It can be written as a convolution equation:

4πh0*x-1=f,E26000

where the function f can be computed from the full scattering data in principle. A numerical inversion of this equation would yield a full recovery of h0 but this is an open problem as far as we know. What is more, unlike the representation formula above it holds pointwise in the important case of bounded (p = ∞) nonlinearities.

We assume that the function x ↦ h(xs) is real-valued and recall that

Ak,θ,θ=2e-ikθyhyuuykθdy,kk0.E27000

For reasons of purely technical nature we define the scattering solutions u(xkθ) for negative k as

uxkθ=ux,-k,θ¯,k<0.E28000

These are the unique solutions of the integral equation:

uxkθ=eikxθ-2Gk+x-y¯hyuuykθdy,E29000

provided that h is real-valued. This allows us to extend A to negative k ≤ − k0 by

Akθθ=A-k,θ,θ¯.E30000

We also put A(kθ′, θ) = 0 for |k| ≤ k0. Splitting

hyuu=h0xu0+hy,|u|u-h0xu0,E31000

we have that

Akθθ=2eikθ-θ,yh0ydy+2e-ikθyhyuuykθ-h0yu0dyE32000

or

Akθθ=Fh0kθ-θ+ARkθθ,E33000

where F denotes the Fourier transform (8). Using the basic assumptions for the function h and (6), we can easily obtain that

|AR(k,θ,θ)|2|h(y,|u|)u(y,k,θ)h0(y)u0| dyC2(α(y)+β(y))|usc(y)|dyC||usc||(||α||1+||β||1)0,|k|.E34000

We have used here the fact that the basic assumptions for the function h guarantee that the functions α and β both belong to L1(2).

Hence, for k large, we have approximately that

AkθθFh0kθ-θ.E10

These considerations and real valuedness of h suggest and justify the following definition:

We define the inverse Born approximation qB via the equality

Akθθ=FqBkθθ,E11

which is understood in the sense of tempered distributions. In order to recover main singularities of h0 from qB, we must study their difference and show that it is locally less singular than h0. To this end, we have the following main result from [5].

Theorem 2. Let σ be as in (7). Then

qB-h0Hloct2,E37000

where t < 3 − 4/p if 4/3 < p ≤ 3/2 and t < 1 − 1/p if 3/2 < p ≤ ∞.

Remark 2. Theorem 2 means that, for 4/3 < p < ∞, the main singularities of h0 can be recovered from the inverse scattering Born approximation qB with full data D. In the case of p = ∞, we have no singularities but may have finite jumps. Under such circumstances, we record the following special case.

Corollary 3. If a piecewise smooth compactly supported function h0 contains a jump over a smooth curve, then the curve and the height function of the jump are uniquely determined by the full scattering data. Especially, for the function h0 being the characteristic function of a smooth bounded domain, this domain is uniquely determined by the full scattering data.

Concluding, in this part of the work, the uniqueness of the direct problem for the nonlinearities h satisfying the appropriate properties was proved. These properties allow local singularities and do not require compact support, but rather some sufficient decay at infinity. Under similar properties, we were also able to establish the asymptotic behaviour of scattering solutions, which gives us the scattering data so we can investigate the inverse scattering problems. Note that both results were proved without assuming smallness of the norm of the nonlinearity as is necessary in dimensions three and higher.

What can we regard as the main result of this section is the Saito’s formula since it implies a uniqueness result and a representation formula for our unknown function h0. In addition, we managed to extract more information about the nonlinearity by applying the method of Born approximation. More precisely, the main singularities (or jumps over smooth curve) of h0 can be recovered from the Born approximation qB which corresponds to the full scattering data D.

### 2.2. Backscattering and fixed angle data

In this section, we consider backscattering data DB and fixed angle scattering data DA following [12]. Using (10) we introduce the inverse backscattering and inverse fixed angle scattering Born approximations qBband qBθ0as follows:

Ak,-θ,θ=FqBb2kθE12

and

Akθθ0=FqBθ0kθ-θ0,E13

where θ0 is fixed.

Furthermore, we assume in addition that the nonlinearity h possesses the Taylor expansion:

hx,1+s=hx1+shx1s+12s2hxs*s2,1<s*<1+sE40000

where

shx1η1x,|s2hx,s*|η2xE41000

uniformly in s ∈ (0, s0), s0 > 0 and with η1,η2LσpR2, where σ as in (7). From this we obtain the expansion:

hx,|u|u=h0xu0+g1xusc+g2xu02usc¯+ηxOusc2,E42000

where g2x=12shx1,g1x=h0x+g2xand ηLσp2with the same σ as above.

Again, the main result for the recovery of main singularities is formulated as the following theorem.

Theorem 3. Let σ be as in (7) with 2 < p ≤ ∞. Suppose in addition

h0̂,g2̂Ws12,1<s<2,E43000

and 2 < s′ < p ≤ ∞, where s′ is the Hölder conjugate of s. Then

qBθ0-h0,qBb-h0Hloct2E44000

for any t < 1 − 1/p if 1 < s ≤ 4/3 and for any t < min{1 − 1/p, 4/s − 2} if 4/3 < s < 2.

Let us sketch the main ideas in the proof of Theorem 3. Using the definition, we may expand the difference in several terms as

qBθ0-h0=q1θ0+qθ0+q2θ0+qRθ0.E111000

In straightforward manner one sees that qθ0C2and q2θ0,qRθ0Ht2with t < 3 − 4/p if 4/3 < p ≤ 3/2 and t < 1 − 1/p if 3/2 < p ≤ ∞. The first nonlinear term q1θ0cannot be analyzed directly from its definition. Instead, we first proved the representation

q1θ0x=-F4-1pvg1̂ξh0̂ηξ+η,θ0η2ξ+η-ξ+η2η,θ0xx-F4-1pvg2̂ξh0̂ηξ+η,θ0η2ξ+η+ξ+η2η,θ0xx,E45000

where F4-1denotes the four-dimensional inverse Fourier transform. This formula might have independent interest too, but primarily it allows us to prove the following regularity: the term q1θ0belongs to the space

1. C2L2if 1 < s < 4/3;

2. H12if s = 4/3;

3. Ht2,t<4/s-2if 4/3 < s < 2.

If we combine all these steps, we obtain Theorem 3 for fixed angle scattering.

The inverse backscattering Born approximation is treated similarly. Namely, we write

qBb-h0=q1b+qb+q2b+qRb.E46000

The latter four terms have exactly the same regularity results as their counterparts in fixed angle scattering. For the first nonlinear term, the representation is now

q1bx=4F4-1pvg1̂ξh0̂ηξηxx-4F4-1pvg2̂ξh0̂ηξ+2η,ηxx.E46000

The additional assumption h0WS1(2)in Theorem 3 implies that h0L1s2.This explains why we restrict s′ < p. By Sobolev embedding, we obtain

qBθ0-h0,qBb-h0Wpϵ2E47000

with some positive  < min{1/p, 1 − 2/p}. Hence, h0 is locally more singular than either of these differences. That’s why both Born approximations recover the main singularities of h0. On the other hand, we may perform the comparison also in the scale of Sobolev spaces. Indeed, if h0Hcompr2with some 0 < r < 1, then

qBθ0-h0,qBb-h0Hloct2E48000

for any t < 2r if 0 < r ≤ 1/3 and for any t < (1 + r)/2 if 1/3 < r < 1. In both cases this t can be made bigger than r. It means that we can reconstruct all singularities from Sobolev space Hr, 0 < r < 1 from data DB and DA by the method of Born approximation.

Corollary 4. If a piecewise smooth compactly supported function h0 contains a jump over a smooth curve, then the curve and the height function of the jump are uniquely determined by backscattering and fixed angle scattering data. Especially, for the function h0 being the characteristic function of a smooth bounded domain, this domain is uniquely determined by backscattering and fixed angle scattering data.

Concluding, in this section we proved that all singularities and jumps (in the absence of a uniqueness theorem) of the nonlinearity h can be recovered from the inverse scattering Born approximation corresponding to fixed angle scattering and backscattering data DA and DB, respectively. No assumptions about the smallness of the norm of nonlinearity h were used as it were in previous publications even in the linear case.

### 2.3. Fixed energy data

The two-dimensional fixed energy problemx1 was a long-standing open problem. In the case of linear Schrödinger operator, the first uniqueness and reconstruction algorithm was proved by Nachman [13] via ¯-methods for potentials of conductivity type. Sun and Uhlmann [14] proved uniqueness for potentials satisfying nearness conditions to each other. The question of global uniqueness for the linear Schrödinger equation with fixed energy was settled only in 2008 by Bukhgeim [15] for compactly supported potentials from Lp, p > 2. This result has recently been improved and extended to related inverse problems (see for example [16] and [17]). Note that Grinevich and Novikov [18] proved that in two dimensions there are nonzero real potentials of the Schwartz class with zero scattering amplitude at fixed positive energy. Thus, the compactness of the supports of the potentials is very natural condition in our considerations.

The results of this section are proved in [19] and they slightly generalize the linear case to a special type of nonlinearity. It turned out that (as we can see in this section) inverse fixed energy scattering problem is much more difficult than the others.

In fixed energy scattering problem, instead of the scattering solutions (4) we need the so-called complex geometrical optics solutions. Complex geometrical optics (CGO) solutions or exponentially growing solutions of the form:

uxz=eixz1+Rxz,z2,zz=0E14

with R decaying at infinity for |z| large for the homogeneous Schrödinger equation

-Δux+hx,|ux|ux=0E15

are obtained as follows. Substituting (14) into (15) yields

-ΔR-2izR+hxeixz1+R1+R=0.E51000

It means that using the Faddeev Green’s function

gzx=14π22e-ixξξ2+2zξdξE52000

as the fundamental solution of the differential operator

-Δ-2iz,E53000

we see that the function R solves the integral equation

Rxz=-2gzx-yhy,|eiyz1+Ryz|1+Ryzdy.E16

It remains to establish unique solvability of this equation. To this end we again use iterations in the sense of next theorem.

We assume that h is compactly supported in Ω2and

1. |h(xs)| ≤ α(x) with some α ∈ L2(Ω) and s ≥ 0

2. |h(x, |ei(x,z)(1 + R1)|) − h(x, |ei(x,z)(1 + R2)|)| ≤ β(x)|R1 − R2| with some β ∈ L2(Ω) and for any R1,R2L2such that ‖Rj < 1 − δ, j = 1, 2 for some fixed δ ∈ (0, 1) and for any z2

3. α2, ‖β2 > 0

Theorem 4. Under the above conditions for h, there exists a constant C0 > 0 such that for all |z| ≥ C0 the equation (16) has a unique solution in L2and this solution can be obtained as limjRjin L2, where

Rj+1xz=-2gzx-yhyeiyz1+Rjyz1+Rjyzdy,j=0,1,E55000

with R0 = 0. Moreover, the following estimates hold

|R|czγ,R-Rjcjzγj+1,j=0,1,.E56000

The proof of Theorem 4 is based on the fact that for any γ < 1 there is constant cγ > 0 such that

|gz*f|cγzγf2,z>1,E57000

for any f ∈ L2(Ω), see [20].

Turning now to the inverse fixed energy scattering problem, we define the scattering transform by

Thξ=2eixξhx,e01+Rxz1+Rxzdx,ξ2C0E58000

and Th(ξ) = 0 for ξ<2C0. Here z=12ξ-iJξ,

J=01-10E59000

and e0=eixz=e12x1ξ2-x2ξ1.What is more, we have the uniform limit Th(ξ)=limjTh,j(ξ), where

Th,jξ=2eixξhx,e01+Rjxz1+Rjxzdx.E60000

We point out that the scattering transform is somehow an auxiliary object (see DE in Introduction). But it is connected to the scattering amplitude as follows. It is well known that the scattering amplitude at fixed energy uniquely determines the Dirichlet-to-Neumann map Λh-k02which in turn uniquely determines the scattering transform (see the details, for example, in [19] and [20]). Recall that Λhf = ∂νu, where u satisfies the Dirichlet problem:

-Δu+hxuu=0,xΩux=fx,xΩ.E61000

Here, Ω is a domain with boundary ∂Ω and outward unit normal vector ν.

Next, we define the inverse fixed energy Born approximation by

qBfx=F-1Thξx.E17

In contrast to the preceding inverse problems, we now set the unknown function to be

h0x=F-1Th,0ξx.E18

In linear case h0 is the actual potential appearing in the Schrödinger equation, but otherwise the connection to physical scatterers is not known to us.

We assume that the nonlinearity h admits the Taylor expansion

hx,e01+s=hxe0+shx,e01+ss=0s+Oβ1xs2,E64000

where |∂sh(xe0(1 + s))|s = 0| ≤ β1(x) and O(β1(x)s2) with β1(x) ∈ L2(Ω) and with small s in the neighbourhood of zero and where O is uniform in x ∈ Ω and such s.

Suppose in addition that the nonlinearity h satisfies the asymptotic expansions

hxe0=j=0αjxξj,hx,e0|1+R1|=j=0αj̃xξjE65000

where |αj|,|αj̃|αx/2. Then we have the following main result concerning the recovery of singularities of h0(x) defined by (18).

Theorem 5. Under the foregoing conditions for the potential function h, it is true that

qBf-h0Ht2E66000

for any t < 1 modulo C2- functions.

Remark 3. The embedding theorem for Sobolev spaces says that the difference qBf-h0belongs to Lq(R2) for any q < ∞ modulo C(R2) functions. It means that all singularities from LlocpR2,p<of unknown function h0 can be obtained exactly by the Born approximation which corresponds to the inverse scattering problem with fixed positive energy.

We note that under fixed energy data we have some additional assumptions on h. This limits the applicability of the main result to, for example, saturation type nonlinearities. In particular, cubic nonlinearity is excluded from these considerations. Moreover, the unknown function h0 has no direct connection to original scatterers in nonlinear cases.

## 3. Numerical examples

Here we discuss the numerical computation of the Born approximation first proposed in [21] for backscattering and fixed angle data. We assume that the scatterer h0(x) is supported in the rectangle R0=-1,1×-1,12. We consider the following examples:

Example 1: h(x,|u|)=χΩ(x(linear)

Example 2: h(x,|u|)=χΩ(x)|u||u|21+|u|2(saturation)

Example 3: h(x,|u|)=0.75χΩ1(x)|u|+χΩ2(x)|u|21+|u|2(linear, saturation)

Example 4: h(x,|u|)=0.75χΩ2(x)|u|21+|u|2+ χΩ1(x(saturation, linear)

Here Ω, Ω1, Ω2 are the shifted ellipses rotated in angle Θ theta (counter-clockwise) detailed in Table 1 and shown in Figure 1.

Semi axisΘCentre
Ω1/2, 1/517π/18(−0.3, − 0.4)
Ω11/2, 1/4π/3(0.5, 0)
Ω21/3, 1/52π/3(−0.5, 0)

### Table 1.

Geometries of the ellipses Ω, Ω1 and Ω2

Consider the Born approximation for full data (11) in the form

2eikθ-θ,yfydy=Akθθ,f=qB.E19

To discretize the unknown function f we divide the rectangle R0 into N = n × n disjoint subrectangles rj of equal size, i.e.

R0=j=1Nrj.E68000

Then, we represent f on R0 in piecewise constant form:

fy=j=1Nfjχrjy,E69000

where fj’s are the unknown values on rj’s. Substitution into (19) yields

j=1Nfjrjeikθ-θ,ydy=Akθθ.E70000

Evaluating this at some points k=ks,θ=θtand θ = θp leads us to

j=1Nfjrjeiksθt-θp,ydy=Aksθtθp,s=1,,N1,t=1,,N2,p=1,,N3.E71000

If we denote M = N1N2N3, we may form one linearized index l = l(stp), l = 1, …, M and write the latter equation as

j=1NfjEjl=gl,l=1,,M,E20

where Ejl=rjeiksθt-θp,ydyare easily evaluated and gl=Aksθtθpneeds to be computed. The computation of gl is carried out using numerical integration, see [21] for details. In matrix form (20) is clearly Ef = g.

For backscattering data and fixed angle data the system (20) is modified accordingly. We note that the system Ef = g does not depend on the scatterer but only on data type and measurement setup.

The fixed energy case differs from the first three data sets. In fixed energy inversion we approximate the scattering transform as

ThξTh,1ξ.E73000

We choose M = m × m points ξ uniformly from the rectangle [−ss] × [−ss]. The function Th,1(ξ) is evaluated by numerical integration, see [19,21] for details. Then the inverse Born approximation (17) is computed similarly to (19).

We use the following parameter values:

ks=s,θp=θp=cosp2πN2-1N2,sinp2πN2-1N2E74000

We use N = 2500 and N1 = 12 for each data set. For full data we use N2 = N3 = 6. For backscattering and fixed angle data, we use N2 = 24. For fixed energy scattering we use m = 40 and s = 6.

In all four cases we obtain the linear system Ef = g whose coefficient matrix E is of size M × N. The data g is corrupted with zero mean Gaussian noise with standard deviation σ = 0.01 max |g|.

The size M as well as the ranks r(E) and (approximate) condition numbers log10κ(E) measuring the ill-posedness of the linear system EF = g are shown in Table 2.

DataMr(E)log10κ(E)
Full172836063
Backscattering28828115
Fixed angle28824117
Fixed energy160026815

### Table 2.

Matrix sizes, ranks and condition numbers

As the linear system is rank-deficient and ill-posed, we use regularization method to solve it. More precisely, we apply the total variation method (TV) which is defined as

f=argminzEz-g22+δLz1,E75000

where the matrix L implements the differences between neighbouring elements in horizontal and vertical directions (for details, see [21]). As in [21] we formulate this minimization problem as a quadratic problem in standard form for more efficient solution. As the regularization parameter we use δ = 2 ⋅ 10− 3 for DE and δ = 10− 3 otherwise.

All computations are carried out in a UNIX system with 512 GB of memory and 40 logical CPU cores, each running at 2.8 GHz. The software platform is MATLAB R2015b. We have used 12 workers in parallel in computing the right-hand side g. We note that a desktop PC with 8 logical cores running at 3.4 GHz and 16 GB of memory is also capable of our computations, but with 7 workers it is considerably slower in computing g.

The computational times to both form and solve the linear system are shown in Table 3. We point out that the right-hand side g contains synthetic data and actual physical measurements may take longer or shorter time.

Example 1Example 3
DataEgTVgTV
Full1.3s47s70s3m20s63s
Backscattering0.4s9s59s37s45s
Fixed angle0.3s9s66s33s58s
Fixed energy0.1s4m11s78s--

### Table 3.

Computational times

The contour plots of scatterers h0(x) and their TV reconstructions via Born approximation from full data, backscattering data and fixed angle data (with θ0 = (1, 0)) are shown in Figures 25 for all examples. For fixed energy scattering we only consider the linear Example 1, since otherwise we do not have direct comparison to a scatterer. The TV reconstruction is shown in Figure 6. In each figure solid white line indicates the true geometry of the scatterer.

We see that the location of the scatterer is located quite nicely in all cases. The shape of the scatterer is best seen from full data and backscattering data. By computing the Born approximation from full angle data, we close an open problem from [5].

## Acknowledgments

This work was supported by the Academy of Finland (application number 250215, Finnish Programme for Centres of Excellence in Research 2012–2017).

## How to cite and reference

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Valery Serov, Markus Harju and Georgios Fotopoulos (July 6th 2016). Some Recent Advances in Nonlinear Inverse Scattering in 2D: Theory and Numerics, Applied Linear Algebra in Action, Vasilios N. Katsikis, IntechOpen, DOI: 10.5772/62233. Available from:

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