16
First-Order Acoustic Wave Equation Reverse Time Migration Based on the Dual-Sensor Seismic Acquisition System JIACHUN YOU, 1 XUEWEI LIU, 1 and RU-SHAN WU 2 Abstract—We analyze the mathematical requirements for conventional reverse time migration (RTM) and summarize their rationale. The known information provided by current acquisition system is inadequate for the second-order acoustic wave equations. Therefore, we introduce a dual-sensor seismic acquisition system into the coupled first-order acoustic wave equations. We propose a new dual-sensor reverse time migration called dual-sensor RTM, which includes two input variables, the pressure and vertical par- ticle velocity data. We focus on the performance of dual-sensor RTM in estimating reflection coefficients compared with conven- tional RTM. Synthetic examples are used for the study of estimating coefficients of reflectors with both dual-sensor RTM and conventional RTM. The results indicate that dual-sensor RTM with two inputs calculates amplitude information more accurately and images structural positions of complex substructures, such as the Marmousi model, more clearly than that of conventional RTM. This shows that the dual-sensor RTM has better accuracy in backpropagation and carries more information in the directivity because of particle velocity injection. Through a simple point- shape model, we demonstrate that dual-sensor RTM decreases the effect of multi-pathing of propagating waves, which is helpful for focusing the energy. In addition, compared to conventional RTM, dual-sensor RTM does not cause extra memory costs. Dual-sensor RTM is, therefore, promising for the computation of multi-com- ponent seismic data. Key words: Reverse time migration, dual-sensor acquisition system, amplitude-preserving migration, first-order acoustic wave equation. 1. Introduction In the development of seismic migration, geo- physicists seek to image discontinuities to its correct location in the subsurface as well as produce ‘true amplitudes’ that are representative of the reflection coefficients of subsurface interfaces. Therefore, true- amplitude migration remains a hot topic in migration research. True-amplitude prestack depth migration can be implemented as a form of integration scheme in terms of a weighted diffraction stack. Bleistein (1987) and Schleicher et al. (1993) pro- posed a similar weighted function in the Kirchhoff migration for recovering reflectivity. Tygel et al. (1993) discussed vector diffraction stack migration using three simple weights simultaneously. Beyond the assumption of isotropy, Vanelle and Gajewski (2013) tried to carry out true-amplitude Kirchhoff depth migration in media with arbitrary anisotropy by generating a new anisotropic migration weight func- tion. Gaussian beam migration as a type of ray-based migration technique began to be valued because of Hill’s contributions (Hill 1990, 2001). Gaussian beam migration has notable advantages over the classic asymptotic ray-based theory and is developing into an accurate and multifunctional migration technique. As a new ray-based migration method, the Gaussian beam migration would improve the subsurface illu- mination, especially beneath highly complex overburden, making this method comparable to Reverse Time Migration (RTM). Gray (2005) pro- posed two true-amplitude Gaussian beam migration procedures based on the deconvolution imaging condition and following some studies done by Zhang et al. (2005) and Hill (2001). On the other hand, one- way equation migration methods, from phase screen migration (Gazdag and Sguazzero 1984) to general- ized screen propagator migration (Wu 1994; de Hoop et al. 2000; Le Rousseau et al. 2001), are experi- encing a rapid development because they are less expensive, the accuracy of one-way propagators is 1 School of Geophysics and Information Technology, China University of Geosciences, Beijing 100083, China. E-mail: [email protected] 2 Earth and Planetary Science Department, University of California, Santa Cruz, CA 95064, USA. Pure Appl. Geophys. 174 (2017), 1345–1360 Ó 2017 Springer International Publishing DOI 10.1007/s00024-017-1468-3 Pure and Applied Geophysics

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Page 1: First-Order Acoustic Wave Equation Reverse Time Migration ...wrs/publication/journal/journal2016-2017... · solve the two-order acoustic wave equation in the depth domain accurately

First-Order Acoustic Wave Equation Reverse Time Migration Based on the Dual-Sensor

Seismic Acquisition System

JIACHUN YOU,1 XUEWEI LIU,1 and RU-SHAN WU2

Abstract—We analyze the mathematical requirements for

conventional reverse time migration (RTM) and summarize their

rationale. The known information provided by current acquisition

system is inadequate for the second-order acoustic wave equations.

Therefore, we introduce a dual-sensor seismic acquisition system

into the coupled first-order acoustic wave equations. We propose a

new dual-sensor reverse time migration called dual-sensor RTM,

which includes two input variables, the pressure and vertical par-

ticle velocity data. We focus on the performance of dual-sensor

RTM in estimating reflection coefficients compared with conven-

tional RTM. Synthetic examples are used for the study of

estimating coefficients of reflectors with both dual-sensor RTM and

conventional RTM. The results indicate that dual-sensor RTM with

two inputs calculates amplitude information more accurately and

images structural positions of complex substructures, such as the

Marmousi model, more clearly than that of conventional RTM.

This shows that the dual-sensor RTM has better accuracy in

backpropagation and carries more information in the directivity

because of particle velocity injection. Through a simple point-

shape model, we demonstrate that dual-sensor RTM decreases the

effect of multi-pathing of propagating waves, which is helpful for

focusing the energy. In addition, compared to conventional RTM,

dual-sensor RTM does not cause extra memory costs. Dual-sensor

RTM is, therefore, promising for the computation of multi-com-

ponent seismic data.

Key words: Reverse time migration, dual-sensor acquisition

system, amplitude-preserving migration, first-order acoustic wave

equation.

1. Introduction

In the development of seismic migration, geo-

physicists seek to image discontinuities to its correct

location in the subsurface as well as produce ‘true

amplitudes’ that are representative of the reflection

coefficients of subsurface interfaces. Therefore, true-

amplitude migration remains a hot topic in migration

research. True-amplitude prestack depth migration

can be implemented as a form of integration

scheme in terms of a weighted diffraction stack.

Bleistein (1987) and Schleicher et al. (1993) pro-

posed a similar weighted function in the Kirchhoff

migration for recovering reflectivity. Tygel et al.

(1993) discussed vector diffraction stack migration

using three simple weights simultaneously. Beyond

the assumption of isotropy, Vanelle and Gajewski

(2013) tried to carry out true-amplitude Kirchhoff

depth migration in media with arbitrary anisotropy by

generating a new anisotropic migration weight func-

tion. Gaussian beam migration as a type of ray-based

migration technique began to be valued because of

Hill’s contributions (Hill 1990, 2001). Gaussian beam

migration has notable advantages over the classic

asymptotic ray-based theory and is developing into an

accurate and multifunctional migration technique. As

a new ray-based migration method, the Gaussian

beam migration would improve the subsurface illu-

mination, especially beneath highly complex

overburden, making this method comparable to

Reverse Time Migration (RTM). Gray (2005) pro-

posed two true-amplitude Gaussian beam migration

procedures based on the deconvolution imaging

condition and following some studies done by Zhang

et al. (2005) and Hill (2001). On the other hand, one-

way equation migration methods, from phase screen

migration (Gazdag and Sguazzero 1984) to general-

ized screen propagator migration (Wu 1994; de Hoop

et al. 2000; Le Rousseau et al. 2001), are experi-

encing a rapid development because they are less

expensive, the accuracy of one-way propagators is

1 School of Geophysics and Information Technology, China

University of Geosciences, Beijing 100083, China. E-mail:

[email protected] Earth and Planetary Science Department, University of

California, Santa Cruz, CA 95064, USA.

Pure Appl. Geophys. 174 (2017), 1345–1360

� 2017 Springer International Publishing

DOI 10.1007/s00024-017-1468-3 Pure and Applied Geophysics

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increasing and they have an increasingly high imag-

ing quality for the medium with strong lateral

velocity variation. Conventional one-way wave

equation depth migration methods focus on imaging

structures instead of correct amplitude information.

Zhang et al. (2003) made a significant contribution in

one-way true-amplitude migration. Subsequently,

many other researchers showed their improvements,

including Vivas and Pestana (2010), Cao and Wu

(2010) and Amazonas et al. (2010). Because RTM is

based on the two-way wave equation, hence it can

solve problems that the conventional one-way equa-

tion and the Kirchhoff migration hard to deal with,

including imaging all types of waves, complex

structures and steeply dipping reflectors (Baysal et al.

1983; Chang and McMechan 1989). It is well known

that the weaknesses of RTM are the high memory

costs and the low-frequency artifacts. Many

researchers are working on addressing these prob-

lems. For example, Clapp (2009) proposed the

application of a random boundary to address the mass

memory problem and Youn and Zhou (2001) sug-

gested the usage of a Laplacian filter to remove low-

frequency artifacts. With respect to wave propaga-

tion, Deng and McMechan (2007, 2008) studied

viscoscalar and viscoelastic wave true-amplitude

RTM considering factors affecting the propagation of

waves, such as the intrinsic attenuation and trans-

mission losses. This paper attempts to study RTM

from a mathematical perspective by providing ade-

quate conditions to solve the wave equation in the

time domain.

The above mentioned migration algorithms use a

single input data type, in general, the pressure or

displacement data, to image subsurface structures.

The full wave equation is a second-order partial

differential equation with respect to space coordi-

nates (Kosloff and Baysal 1983; Sandberg and

Beylkin 2009). But our present seismic acquisition

system records a wavefield at a given depth.

Therefore, there is a contradiction between the

solution of full wave equation and the initial con-

ditions provided by the current seismic acquisition

system, which in theory makes the two-way wave

equation unsolvable at the depth domain. Based on

this contradiction, You et al. (2016) proposed a

dual-sensor seismic acquisition system providing

two boundary conditions to completely solve the full

wave equation in the depth domain. This paper

attempts to determine the output of conventional

RTM when multiple input terms are involved.

Advances of past studies of vector acoustic (VA)

migration methods in multi-component seismic

acquisition, support our approach. Vasconcelos

(2013) proposed the VA theory for RTM based on

the reciprocity theorem using novel dual-source

multicomponent streamer and ocean-bottom acqui-

sition systems. El Yadari and Hou (2013) introduced

the vector-acoustic framework into Kirchhoff

migration, then El Yadari (2015) combined the

vector acoustic equation with the Gaussian beam

migration by Green’s function theory, forming a

novel migration scheme, which is feasible to any

type of migration methods, including finite differ-

ence or ray-based migration. Ravasi et al. (2015a, b)

studied RTM using Ocean Bottom Cable (OBC)

data, which has a higher imaging quality than the

conventional RTM. Solving the full wave equation

with full initial conditions helps to estimate more

accurate amplitude information of reflectors. It is

possible that wavefields in the time domain can be

more accurately computed when sufficient require-

ments are provided in the wavefield

backpropagation. Therefore, this study takes

advantage of amplitude-preserving migration in

RTM with enough initial conditions, which are

provided by our dual-sensor seismic acquisition

system. Several examples are given to verify dif-

ferences in estimating amplitudes of reflectors using

our proposed dual-sensor RTM and conventional

RTM for the whole imaging section.

2. Dual-Sensors Seismic Acquisition System

Sonneland et al. (1986) deployed two streamers

at different depths to reduce the weather noise and to

separate the upgoing and downgoing wavefields.

However, it was difficult to maintain the dual

streamer in the same vertical plane due to the

immature marine seismic acquisition technique.

Hence, this method failed to attract the attention of

1346 J. You et al. Pure Appl. Geophys.

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the seismic industry. With the development of

marine seismic acquisition techniques, it is now

possible to accurately hold the dual sensor in the

same vertical plane. In the previous research, the

marine over/under towed-streamer acquisition sys-

tem introduced by Schlumberger WesternGeco is

used to remove ghost waves and extend the seismic

bandwidth to both higher and lower frequencies

(Hill et al. 2006; Ozdemir et al. 2008). This tech-

nique has been deployed in many research fields and

attained a quality migration section by the conven-

tional Kirchhoff PSTM or PSDM (Moldoveanu et al.

2007; Bunting et al. 2011). However, previous

research works just exploited parts of advantages of

the dual-sensor seismic acquisition system, but we

want to make full use of this new system to obtain

better imaging results using the full initial condi-

tions in depth extrapolation and imaging in the time

domain.

The dual-sensor seismic acquisition system is

shown in Fig. 1. The marine acquisition system

consists of two streamers that are towed behind a

survey vessel. The two streamers are located at dif-

ferent depths below the sea surface. When a signal is

excited by a source towed behind the survey vessel

and propagates in the medium, the reflection waves

are received by the dual sensors in the streamer. A

similar land dual-sensor seismic acquisition system

was proposed by You et al. (2016) to achieve true-

amplitude migration in the depth domain.

3. Dual-Sensor Reverse Time Migration

It is well known that the conventional scalar-

acoustic wave equation is a second-order partial

derivative equation with respect to the space, which

needs two boundary conditions to deal with in the

depth domain. In our previous work, we carried out a

full wave equation true-amplitude depth migration

using our proposed dual-sensor seismic acquisition

system, in which the dual-sensor data are utilized to

solve the two-order acoustic wave equation in the

depth domain accurately and the spectral project

algorithm is introduced to remove evanescent waves

(You et al. 2016). Using conventional RTM as a

reference, we try to achieve a more reliable amplitude

estimate for the whole migration section based on an

update RTM equipped with the dual-sensor seismic

acquisition system. Next, we analyzed the first-order

partial differential wave equation system in theory

with two boundary conditions in the 2D media, which

is shown in Eq. 1.

opot¼ �c2ðx; zÞqðx; zÞ omx

oxþ omz

oz

� �ðaÞ;

omx

ot¼ � 1

qðx;zÞopox

ðbÞ;omz

ot¼ � 1

qðx;zÞopoz

ðcÞ;pðx; z ¼ 0; tÞ ¼ dðx; 0; tÞ ðdÞ;pzðx; z ¼ 0; tÞ ¼ dðx;Dz;tÞ�dðx;0;tÞ

DzðeÞ ;

vxðx; z; t� tmaxÞ ¼ 0 ðfÞ;

8>>>>>>>>>>><>>>>>>>>>>>:

ð1Þ

Figure 1Marine dual-sensor seismic acquisition system

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where x and z are the horizontal and vertical coor-

dinates, respectively; p(x, z, t) is the pressure data at

time t; cðx; zÞ and qðx; zÞ are the velocity and density

of the media, respectively; and Dz is the grid space.

Recorded seismic data d(x, 0, t) and d(x, Dz, t), col-

lected by up/down dual sensors at z ¼ 0 and z ¼ Dz,

respectively, are used to compute the normal

derivative pz (x, z, t) at z ¼ 0, which makes the wave

equation solvable. The vectors vx (x, z, t) and vz (x, z,

t) are the horizontal and vertical particle velocity

vectors, respectively. tmax is the maximum of

recording time.

Equation 1 is a one-order equation system, which

needs three initial conditions to perform reverse time

extrapolation in the time domain for Eq. 1a–c. If we

want to use these two initial conditions to perform the

backpropagation of wavefields, the particle velocity

vector has to be evaluated at the receiver positions

using the normal derivative data pz (x, z, t). The

evaluation of the vertical particle velocity vector is

related to the spatial pressure gradient in the acoustic

media via the following equation:

pzðx; z;xÞ ¼ �jxqmzðx; z;xÞ; ð2Þ

where i is the imaginary unit and x is the circular

frequency.

In the conventional RTM, it is the conventional

approach to assume that the vz ðx; z; t� tmaxÞ ¼ 0,

hence the wavefield backpropagation is inaccurate,

resulting in imaging amplitude errors. However, in

our dual-sensor RTM, we reduce the strength of the

assumption mathematically and make the estimation

of imaging amplitudes for the whole section more

accredited.

The processing flow about dual-sensor RTM is

that: (1) we should estimate the quantity of particle

velocity using Eq. 2; (2) and then using the pressure

and estimated particle velocity to solve Eq. 1a–c to

perform the time reverse wave propagations. This

property may be one of the advantages of dual-sensor

RTM in terms of structural imaging. We will use the

simple point-shape model and Marmousi model to

discuss this later. In this study, we will discuss

another advantage of RTM, i.e., the estimation of

more accurate amplitudes for the reflection sections.

To compare the differences in estimating the

amplitudes, the conventional RTM and the dual-

sensor RTM are employed to migrate the recorded

data.

In general, the pressure-only data are used as the

injection to backpropagate the receiver wavefields in

the conventional RTM. The scheme can be written as

Conventional RTM : p ! Equation ð1aÞ; ð3Þ

where the ? symbol refers to the usage of data as the

initial condition to perform the backpropagation of

recorded data.

The operators of our dual-sensor RTM can be

written as

Dual-sensor RTM : p ! Equation ð1aÞ and

mEz ! Equation ð1cÞ; ð4Þ

where mEz refers to the evaluated vertical particle

velocity data from Eq. 2. Equation 4 shows that

pressure and evaluated vertical particle velocity data

are injected into Eq. 1a and c, respectively, as the

initial conditions to backpropagate the recorded data.

After finishing the wavefield extrapolation of the

receiver field, which is called backpropagation of the

receiver data, we also need to carry out the forward

propagation of the source field, which is named for-

ward modeling with a source. The operation of the

source wavefield is implemented in the conventional

and dual-sensor RTMs. The stratagem can be written

as:

Conventional and dual sensor RTMs: s

! Equation ð1aÞ; ð5Þ

where s represents the usage of the wavelet as a

excitement in the forward propagation of the wave-

field. In our work, we usually use a Ricker wavelet as

a source signal.

In RTM, the cross-correlation imaging condition

is applied to compute the imaging amplitudes of

reflectors; the equation is shown below:

Iðz; xÞ ¼X

t

S�ðz; x; tÞRðz; x; tÞ; ð6Þ

where Sðz; x; tÞ and Rðz; x; tÞ are the forward- and

backpropagating wavefields, respectively, which are

computed by Eqs. (5) and (3) (or Eq. 4). The cross-

correlation imaging condition is proposed under-

standing the one-way migration in which the source

1348 J. You et al. Pure Appl. Geophys.

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and the receiver wavefields contain the downgoing

and upgoing wavefields, respectively. However,

RTM is a two-way migration method. Thus, both

source and receiver wavefields involve the downgo-

ing and upgoing waves. This results in the low-

frequency artifact in the migration section. This

artifact will affect the accuracy of the amplitude

estimates and needs to be removed. In this paper, a

simple derivative filter in the vertical dimension is

applied for this purpose.

In our work, the GPU (Graphics Processing Unit)

accelerating technique is used to speed up the

wavefield propagation, including the forward stimu-

lation and the backpropagation of waves.

4. Synthetic Examples

In this section, several synthetic examples are

given to compare between theoretical and estimated

reflection coefficients of reflectors obtained from

conventional RTM and dual-sensor RTM. A stag-

gered grid finite difference technique with perfectly

matched layer (PML) is used to solve the one-order

acoustic wave equation (Berenger 1994; Hastings

et al. 1996). Small differences in the imaging struc-

tures are also shown.

4.1. A Point-Shape Model

We set up a simple point-shape model to illustrate

differences in the directivity of wave propagation by

conventional RTM and our proposed dual-sensor

RTM. The model dimension is 200 m 9 200 m with

grid steps of 1 m 9 1 m. The background velocity of

model is 2000 m/s and the velocity of anomaly zone

is 3000 m/s, the velocity model is pictured in Fig. 2a.

200 receivers are put at z = 0 m and z = 1.0 m to

collect the dual-sensor data, respectively. In this

modeling, the type of source wavelet we utilized is

the Ricker wavelet with 60 Hz of the domain

frequency and the sampling interval is 0.0001 s.

The source excitement is located at x = 0 m and

z = 0 m. The acquisition system is shown in the

upper of Fig. 2a.

Figure 2b, c are snapshots of wave backward

propagation produced by conventional and dual-

sensor RTMs at t = 0.0707 s, respectively. To per-

form a fair comparison, wavefield snapshots are

compared in the term of the same numerical range

and migration sections are scaled to the same

numerical range as well. In theory, if the receiver

wavefield is propagated backward in time, the ideal

situation is that the exact wave field should be

recovered as the forward modeling with artifacts as

few as possible. Based on this principle and compar-

ing the snapshots in Fig. 2b, c, as the red arrows

pointed at, there are longer diffraction tails in

conventional RTM (Fig. 2b); while wavefield snap-

shot calculated by our proposed dual-sensor RTM

(Fig. 2c) presents a more convergent result and this

will bring less artifacts in imaging. Consequently,

observing the imaging results obtained by conven-

tional and dual-sensor RTMs (Fig. 2d, e), it shows

that dual-sensor RTM has a greater potential to reveal

the accurate reflector with less artificial noise than the

conventional RTM. These comparing results fully

proved the advantage of using pressure-particle

velocity data in the wave backpropagation, especially

in the near-field region. To make a comparison of the

dual-sensor RTM versus the sum of the conventional

RTM of two cables, we firstly implement the

conventional RTM using the different cables at

different depth separately and then add the results

together. The summation of the results of two cables

is shown in Fig. 2f. There is no apparent difference

between migration sections by one cable and the

summation of the of two cables. This demonstrates

that the dual-sensor migration is not equal to a simple

summation of the conventional RTM of each cables.

4.2. Two-Layer Model

This model consists of a 30� dipping layer and an

unconformity surface. The velocity model is shown in

Fig. 3a. The model dimension is 600 m 9 800 m with

grid steps of 1 m 9 1 m. The acquisition is comprised

of 114 shots spaced at 6.0 m, each having 120 receivers

with 1 m spacing. The minimum offset in the data is

0 m, the top-receiving line is at z = 0 mand the bottom-

receiving line is at z = 1.0 m. In thismodeling, the type

of source wavelet is Ricker wavelet with 60 Hz of the

domain frequency and the sampling interval is 0.0001 s.

The acquisition system is shown in the upper of Fig. 3a.

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1350 J. You et al. Pure Appl. Geophys.

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The unconformity is designed to test whether the

migration method can image the lithological diver-

sity correctly, eliminating the effect of the upper

layer. The migration sections computed by conven-

tional RTM and dual-sensor RTM based on the shot

gathers are shown in Fig. 3b, c, thus, illustrating the

qualitative analyses of the imaging structures. Both

migration methods, dual-sensor RTM and conven-

tional RTM, provide the correct positions of

reflection interfaces. It is necessary to extract more

detailed information to test their differences. There-

fore, reflection coefficients along two interfaces are

selected from the migration sections. To have a fair

comparison, the whole migration section is scaled

with a constant factor to the same amplitude range

of the theoretical reflectivity to account for removal

of the impacts of unknown factors, such as the

amplitudes of the source. The estimated reflection

bFigure 2

a Velocity model; b the snapshot of wavefield backward propa-

gation at t = 0.0707 s using conventional RTM; c the snapshot of

wavefield backward propagation at t = 0.0707 s using dual-sensor

RTM; d the migration section calculated by conventional RTM;

e the migration section calculated by dual-sensor RTM; f the

migration section calculated by sum of conventional RTM of two

cables. The black-dashed lines and a star-shape icon illustrate the

acquisition seismic system with a total of 1 shot and its

corresponding streamers in which each streamer is composed of

200 receivers as presented by the solid black lines at different

depth. The left right arrow shown in black is the receiver interval

Figure 3a The original velocity model; b migration section after conventional RTM; c migration section after dual-sensor RTM. The black-dashed

lines and star-shape icons illustrate the acquisition seismic system with a total of 114 shots and its corresponding streamers in which each

streamer is composed of 120 receivers as presented by the solid black lines at different depth. The left right arrow shown in black is the

receiver interval and in red is the shot interval

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coefficients obtained from different migration meth-

ods and the theoretical coefficients of the two

interfaces in the model are shown in Fig. 4,

respectively. The relative errors of estimated and

theoretical reflection coefficients are calculated to

quantitatively differentiate the recovery perfor-

mances of the amplitudes of reflectors. The

analysis of Fig. 4a, which is the migration section

imaged by conventional RTM, shows that the

imaging energy of the whole section fits the

theoretical value with a vertical shift, more specif-

ically, the relative errors of the shallower reflector

deviate from the zero line by approximately 50%.

On the other hand, the estimated reflection coeffi-

cients of the two interfaces by the dual-sensor RTM

match well with the corresponding theoretical coef-

ficients and the relative error curves are almost zero.

The reason why the calculated coefficients are so

ringy is that we use the square grid to subdivide the

dipping interface result to the staircase shapes of the

interface. From this simple example, we see that the

dual-sensor RTM is capable of preserving ampli-

tudes in the wave propagation.

4.3. Multiple-Layer Model

In addition to the two interface example, we also

use a more complex model to test the performance of

our proposed dual-sensor RTM in recovering exact

amplitudes of reflectors. The velocity model is shown

in Fig. 5a. The model dimension is

1544 m 9 2400 m with grid steps of 4 m 9 4 m.

There are 120 shots spaced 16 m apart, in which each

streamer is composed of 120 receivers spaced at 4 m.

The minimum offset in the data is z = 0 m, the top-

receiving line is placed at z = 0 m and the bottom-

receiving line is put at z = 4.0 m. In this modeling,

the type of source wavelet is the Ricker wavelet with

60 Hz of the domain frequency and the sampling

interval is 0.0004 s. The acquisition system is shown

in the top of Fig. 5a. The results of conventional

RTM and dual-sensor RTM are shown in Fig. 5b, c.

Figure 4a Comparison of estimated reflection coefficients from conventional RTM and theoretical coefficients; b the relative errors of estimated

reflection coefficients from conventional RTM and theoretical coefficients; c comparison of estimated reflection coefficients from dual-sensor

RTM and theoretical coefficients; d the relative errors of estimated reflection coefficients from dual-sensor RTM and theoretical coefficients.

The solid blue line and the broken blue line in a and c present the estimated reflection coefficients of dipping interface and the unconformity

surface, respectively. The solid red line and the broken red line present the theoretical coefficients of the dipping interface and the

unconformity surface, respectively. The solid blue line and the solid red line in b and d are the relative errors for the dipping interface and the

unconformity surface, respectively

1352 J. You et al. Pure Appl. Geophys.

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The comparison between the migration sec-

tions generated by dual-sensor RTM and

conventional RTM demonstrates that there is no

structural imaging difference between them, but

we are more interested in the accurate amplitude

computational ability of these migration methods.

Therefore, three horizons are selected as carriers.

The three interfaces (H1, H2 and H3) are depicted

as the dashed red lines in Fig. 5a and the

calculated reflection coefficients are recorded

along the reflectors. The H1 horizon presents the

near surface of the model. The H2 horizon is

located in the middle of the model, which is used

to test the performance of the migration method in

recovering the amplitudes after the interference of

multiple reflectors, and the H3 horizon is a

unconformity in the depth of the model to test

whether our proposed dual-sensor RTM is able to

present the same behavior on better amplitude

recovery for multiple interfaces case. The similar

scaling method is employed for the same reason

mentioned in the secondary example. First of all,

we plot the estimated reflection coefficients of

three interfaces computed by dual-sensor RTM

and conventional RTM with its corresponding

theoretical coefficients; secondly, we plot statis-

tics on the relative errors of the estimated

reflection coefficients and the theoretical coeffi-

cients of three interfaces under two migration

methods to quantify this evaluation. The results of

conventional RTM and dual-sensor RTM are

shown in Figs. 6 and 7, respectively.

Figure 5a The original velocity model; b migration section after conventional RTM; c migration section after dual-sensor RTM. The black-dashed

lines and star-shape icons illustrate the acquisition seismic system with a total of 120 shots and its corresponding streamers in which each

streamer is composed of 120 receivers as presented by the solid black lines at different depth. The left right arrow shown in black is the

receiver interval and in red is the shot interval

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Figure 6 shows that the conventional RTM does

not provide accurate amplitude migration satisfac-

torily. The relative error for the deep horizon can

reach approximately 50%. Figure 7 indicates that

the estimated reflection coefficients of three inter-

faces using dual-sensor RTM fit its corresponding

theoretical coefficients for three horizons with less

errors. The relative errors of the H2 Horizon are

equal or less than 20% and the relative errors of the

H1 and H3 Horizons are under 10%. Comprehen-

sive analysis of Figs. 6 and 7 reveals that dual-

sensor RTM overcomes the energy losses of

conventional RTM in the wave propagation (Ravasi

et al. 2015a, b), which are advantages of our

proposed dual-sensor RTM over conventional

RTM. It needs to be mentioned that this benefits of

dual-sensor RTM can be achieved without

increasing much memory cost compared to con-

ventional RTM.

4.4. Marmousi Model

The more challenging task of this part is to use the

Marmousi data as input to perform conventional

RTM and dual-sensor RTM. This complex model is a

perfect platform to test the performance of estimating

coefficients of reflectors for complex structures. The

model dimension is 3500 m 9 7500 m with sam-

pling steps of 6.25 m 9 6.25 m. There are 240 shots

spaced 25 m apart, in which each streamer is

composed of 240 receivers spaced at 6.25 m. The

minimum offset in the data is z = 0 m, the up-

receiving line is at z = 0 m and the down-receiving

line is at z = 6.25 m. The original velocity model is

Figure 6a Comparison of the estimated reflection coefficients (solid blue line) along the H1 horizon using conventional RTM and the theoretical

coefficient (dashed red line); b the relative error of the estimated reflection coefficients and the theoretical coefficient for the H1 horizon;

c comparison of the estimated reflection coefficients (solid blue line) along the H2 horizon using conventional RTM and the theoretical

coefficient (dashed red line); d the relative error of the estimated reflection coefficients and the theoretical coefficient for the H2 horizon;

e comparison of the estimated reflection coefficients (solid blue line) along the H3 horizon using conventional RTM and the theoretical

coefficient (dashed red line); f the relative error of the estimated reflection coefficients and the theoretical coefficient for the H3 horizon

1354 J. You et al. Pure Appl. Geophys.

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displayed in Fig. 8a. In this modeling, the type of

source wavelet is the Ricker wavelet with 60 Hz of

the domain frequency and the sampling interval is

0.0005 s. The acquisition system is shown in the

upper of Fig. 8a. The imaging results using conven-

tional RTM and dual-sensor RTM are shown in

Fig. 8b, c. As mentioned previously, it is apparent

that conventional RTM and dual-sensor RTM give

similar imaging result in the case of a simple model,

while there are differences at the detailed levels for

more complicated models such as the Marmousi

model. Hence, local features of the migration sections

(dashed black zone in Fig. 8a) are extracted and

zoomed in Fig. 9. The images in Fig. 9 indicate that

dual-sensor RTM gives better imaging amplitudes in

the complicated zone of the model and images the

weak reflectors clearer than conventional RTM.

Structural analysis shows that the amplitude

information is a powerful tool to make a

comparison. To quantitatively evaluate the perfor-

mance of estimating the amplitudes of the

Marmousi model, three vertical logs are plotted

in Fig. 8a, namely, logs A, B and C, located at

x = 1875 m, x = 3125 m and x = 5000 m, respec-

tively. Log B is located in the center of the model,

passes though the three faults and several anticlines

of the model and carries abundant information. The

degree of complexity in geological structures in

logs A and C is relatively weak. For the sake of a

reasonable comparison, a band-limited theoretical

amplitude is calculated for comparison. The pro-

cess flow is as follows: First, the theoretical

coefficient needs to be converted from the depth

domain into the time domain as time series;

second, the reflection amplitude can be produced

by convolving the theoretical coefficient with the

wavelet in the time domain; and finally, the

synthetic reflection amplitude in the time domain

Figure 7Same as Fig. 6 but using dual-sensor RTM

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needs to be transformed back into the depth

domain (Kiyashchenko et al. 2007). The estimated

reflection amplitudes can be recorded at the posi-

tions of the logs in the imaged sections. Thus, we

obtain the estimated reflection amplitudes at logs

A, B and C in the imaged sections produced by

conventional RTM and dual-sensor RTM, which

are displayed with corresponding theoretical ampli-

tudes in Figs. 10, 11 and 12, respectively.

The comparison of Figs. 10, 11 and 12 demon-

strates that the reconstructed amplitudes obtained by

conventional RTM for the whole section show

relatively strong bias from the theoretical values,

which has an impact on the accurate amplitude

preservation; while the reflection amplitudes esti-

mated by dual-sensor RTM are more reliable.

Furthermore, to show more accurately the differences

between these two migration methods, the correlation

coefficients between computing reflection amplitudes

based on different migration methods and theoretical

reflection amplitudes at A, B and C positions,

respectively, are tabularized in Table 1. Table 1

shows that our proposed dual-sensor RTM can

achieve better correlation coefficients than conven-

tional RTM with slightly increasing memory costs,

even for a complex structure.

5. Discussion

In practice, it is almost impossible to collect the

dual-sensor data without any noise contamination.

Figure 8a The original velocity model; b migration section using conventional RTM; c migration section using dual-sensor RTM. The black-dashed

lines and star-shape icons illustrate the acquisition seismic system with a total of 240 shots and its corresponding streamers in which each

streamer is composed of 240 receivers as presented by the solid black lines at different depth. The left right arrow shown in black is the

receiver interval and in red is the shot interval

1356 J. You et al. Pure Appl. Geophys.

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Additionally, a key factor, the velocity model, also

has an influence on the imaging result using our

proposed dual-sensor migration methods. Hence, to

study about the impact of these sensitivity factors on

our migration results, we will hold a deeper discus-

sion on this issue.

6. Conclusions

We input one more item in the conventional

RTM based on a newly dual-sensor seismic

acquisition system under the theoretical framework

of the one-order acoustic wave equations. With two

inputs, we present a processing idea with respect to

RTM and to provide a mathematical analysis of the

potential of dual-sensor RTM. To verify the per-

formance of dual-sensor RTM and conventional

RTM in recovering the amplitudes of reflectors,

several examples are given to illuminate the

advantages of dual-sensor RTM over conventional

RTM for more accurate amplitude estimations and

complex structure imaging. We believe that the

dual-sensor acquisition system provides require-

ments for one-order acoustic wave equations to

make waves propagate in the correct direction and

compensates for the imaging energy losses of the

deep structures, requiring no additional memory

Figure 9a Migrated image obtained by conventional RTM; b migrated image obtained by dual-sensor RTM; c the true reflectivity

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Figure 10a Comparison of the estimated reflection amplitudes (solid blue line) computed by conventional RTM and the theoretical amplitudes (solid

red line) at the position A; b comparison of the estimated reflection amplitudes (solid blue line) computed by dual-sensor RTM and the

theoretical amplitudes (solid red line) at the position A

Figure 11Same as Fig. 10 but at the position B

1358 J. You et al. Pure Appl. Geophys.

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costs. This characteristic means that this method-

ology is of importance for multi-measurement

exploration, which is a focus of ongoing research.

Acknowledgements

We appreciate the valuable comments and sugges-

tions from the reviewer Matteo Ravasi and Nizare El

Yadari in improving the quality of this manuscript.

We also thanks Xiao-Bi Xie for helpful discussions.

This research is financial supported by The

Fundamental Scientific Research for The Central

Universities (Grant No. 2652016169).

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(Received June 15, 2016, revised December 6, 2016, accepted January 4, 2017, Published online January 20, 2017)

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