The present disclosure relates to methods for acquiring and separating contributions from two or more different simultaneously or near simultaneously emitting sources in a common set of measured signals representing a wavefield. In particular, the present disclosure relates to acquiring and separating contributions from two or more sources acquired at positions in a 2D lateral plane encoded by means of the simultaneous source methods such as, but not limited to, the method of signal apparition or methods using random dithering to encode sources. The inventions would apply equally to onshore and offshore seismic surveys, and for implosive, explosive or vibratory type sources.
Seismic data can be acquired in land, marine, seabed, transition zone and boreholes for instance. Depending on in what environment the seismic survey is taking place the survey equipment and acquisition practices will vary.
In towed marine seismic data acquisition a vessel tows streamers that contain seismic sensors (hydrophones and sometimes particle motion sensors). A seismic source usually but not necessarily towed by the same vessel excites acoustic energy in the water that reflects from the sub-surface and is recorded by the sensors in the streamers. The seismic source is typically an array of airguns customarily deployed as a set of sub-arrays, each of which includes a set of individual airguns. These are normally programmed to fire at the same instant, providing a close to instantaneous peak of energy followed by a longer, lower energy output as a result of oscillating air bubbles. A marine source can also be a marine vibrator for instance, which may be a single unit or a set of individual units composing an array. In either case, the intent is to provide a seismic source output which contains as far as possible a broad range of frequencies within the usable seismic frequency ranges, typically from 1-2 Hz up to around 500 Hz. In modern marine seismic operations many streamers are towed behind the vessel (3D seismic data acquisition). It is also common that several source and/or receiver vessels are involved in the same seismic survey in order to acquire data that is rich in offsets and azimuths between source and receiver locations.
In seabed seismic data acquisition, nodes or cables containing sensors (hydrophones and/or particle motion sensors) are deployed on the seafloor. These sensors can also record the waves on and below the seabottom and in particular shear waves which are not transmitted into the water. Similar sources are used as in towed marine seismic data acquisition. The sources are towed by one or several source vessels.
In land seismic data acquisition, the sensors on the ground are typically geophones and the sources are commonly vibroseis trucks. Vibroseis trucks are usually operated in arrays with two or more vibroseis trucks emitting energy close to each other roughly corresponding to the same shot location. In this invention we refer to such source configurations as groups of sources.
The general practice of marine and seabed seismic surveying is further described below in relation to
Prospecting for subsurface hydrocarbon deposits (701) in a marine environment (
Seismic sources typically employ a number of so-called airguns (709-711) which operate by repeatedly filling up a chamber in the gun with a volume of air using a compressor and releasing the compressed air at suitable chosen times (and depth) into the water column (712).
The sudden release of compressed air momentarily displaces the seawater, imparting its energy on it, setting up an impulsive pressure wave in the water column propagating away from the source at the speed of sound in water (with a typical value of around 1500 m/s) (713).
Upon incidence at the seafloor (or seabed) (714), the pressure wave is partially transmitted deeper into the subsurface as elastic waves of various types (715-717) and partially reflected upwards (718). The elastic wave energy propagating deeper into the subsurface partitions whenever discontinuities in subsurface material properties occur. The elastic waves in the subsurface are also subject to an elastic attenuation which reduces the amplitude of the waves depending on the number of cycles or wavelengths.
Some of the energy reflected upwards (720-721) is sensed and recorded by suitable receivers placed on the seabed (706-708), or towed behind one or more vessels. The receivers, depending on the type, sense and record a variety of quantities associated with the reflected energy, for example, one or more components of the particle displacement, velocity or acceleration vector (using geophones, mems [micro-electromechanical] or other devices, as is well known in the art), or the pressure variations (using hydrophones). The wave field recordings made by the receivers are stored locally in a memory device and/or transmitted over a network for storage and processing by one or more computers.
Waves emitted by the source in the upward direction also reflect downward from the sea surface (719), which acts as a nearly perfect mirror for acoustic waves.
One seismic source typically includes one or more airgun arrays (703-705): that is, multiple airgun elements (709-711) towed in, e.g., a linear configuration spaced apart several meters and at substantially the same depth, whose air is released (near-) simultaneously, typically to increase the amount of energy directed towards (and emitted into) the subsurface.
Seismic acquisition proceeds by the source vessel (702) sailing along many lines or trajectories (722) and releasing air from the airguns from one or more source arrays (also known as firing or shooting) once the vessel or arrays reach particular pre-determined positions along the line or trajectory (723-725), or, at fixed, pre-determined times or time intervals. In
Typically, subsurface reflected waves are recorded with the source vessel occupying and shooting hundreds of shots positions. A combination of many sail-lines (722) can form, for example, an areal grid of source positions with associated inline source spacings (726) and crossline source spacings. Receivers can be similarly laid out in one or more lines forming an areal configuration with associated inline receiver spacings (727) and crossline receiver spacings.
The general practice of land seismic surveying is further described below in relation to
Prospecting for subsurface hydrocarbon deposits (801) in a land environment (
Thus, one group of seismic sources could consist of the “array” of vibrators 802 and 803, while a second group of sources consists, e.g., of vibrators 804 and 805.
The elastic waves radiating away from the baseplate of the vibrators scatter, reflect (808) and refract (809) at locations or interfaces in the subsurface where the relevant material properties (e.g., mass density, bulk modulus, shear modulus) vary and are recorded at hundreds of thousand of individual/single sensors (810) or at thousands of sensor groups (811). Sensor signals from one or more sensors in a group can be combined or summed in the field before being sent sent to the recording truck (812) over cables or wirelessly.
Source positions may lie along straight lines (814) or various other trajectories or grids. Similarly, receiver positions may lay along lines oriented in a similar direction as the source lines, e.g., 820, and/or oriented perpendicularly to the source lines (821). Receivers may also be laid out along other trajectories or grids. The source spacing along the line (815) is the distance the source in a group move between consecutive shotpoints. The inter source spacing (816) is the distance between two sources in the same source group. Similarly, the receiver spacing is the spacing between individual receivers (e.g., 818) in case single sensors or between sensor groups (e.g., 817). The source line spacing (819) is some representative distance between substantially parallel source lines and similarly for the receiver line spacing. Waves may be affected by perturbations in the near surface (813) which obscure the deeper structure of interest (i.e., possible hydrocarbon bearing formations). In land seismic data acquisition, the sensors on the ground are typically geophones.
Explosive sources may also be used onshore, which may be one large charge or a series of smaller ones.
Impulsive marine sources are traditionally formed from a combination of individual energy emitting source elements, typically being of the airgun type, by which a volume of compressed air is released into the water column to produce energy in the preferred frequency spectrum. Each airgun element is typically deployed a few metres below the surface, arranged into arrays of similar units.
There are various brand names and designs of such units, including but not limited to Sleeve Guns, GI Guns and Bolt Airguns and donut guns. All such units work in a similar way and will be referred to herein as “airgun” for the sake of convenience.
Each individual airgun unit has a specific volume of air, which can be configured by the user. As each unit is initiated, the air volume is ejected almost instantaneously into the water column, and the resulting bubble rises towards the surface, oscillating with a given periodicity with decaying amplitude. This continues for up to a second or two. The periodicity is a function of the volume and pressure of the air.
Individual airgun elements are combined into sub-arrays in various configurations, consisting of airguns with a range of volumes such that the bubble periodicity is different for each airgun element. Airgun units are commonly combined together in such sub-arrays such that the overall output consists of a short, aligned initial output (referred to as the “peak”), followed by a period in which the various bubble periodicity times result in largely destructive interference, in order to make the overall radiating pressure wave, referred to as the sub-array signature, as close as possible to the idealized spike. Such a process is referred to as sub-array tuning, and the techniques involved in this are well established practice and beyond the scope of this description.
Following the firing of a shot, after a short period of time, since the source vessel is moving continuously, a subsequent shot is fired after a few seconds. This is generally between five and twenty seconds for mainstream seismic acquisition. The objective, quite apart from giving time for the source vessel to move, is also to allow the energy from each shot-point to decay before the next one is initiated. Some approaches use shorter shot intervals (two or more seconds), often but not universally combined with some element of timing change on sequential shots in order to limit the impact of the insufficient decay time on sequential shot records. These approaches are referred to as “simultaneous source” and are discussed below. These approaches enable more source points per unit area, albeit at some compromise in terms of interference or fold.
In the description below we focus on sources towed by a single vessel. However, the present invention also applies to sources towed by several vessels.
Traditionally seismic data have been acquired sequentially: an impulsive source, typically formed of two or more airgun sub-arrays or vibroseis units is excited and data are recorded until the energy that comes back has diminished to an acceptable level and all reflections of interest have been captured after which a new shot at a different shot location is excited. Being able to acquire data from several sources at the same time is clearly highly desirable. Not only would it allow to cut expensive acquisition time drastically but it could also better sample the wavefield on the source side which typically is much sparser sampled than the distribution of receiver positions. It would also allow for better illumination of the target from a wide range of azimuths as well as to better sample the wavefield in areas with surface obstructions. In addition, for some applications such as 3D VSP acquisition, or marine seismic surveying in environmentally sensitive areas, reducing the duration of the survey is critical to save costs external to the seismic acquisition itself (e.g., down-time of a producing well) or minimize the impact on marine life (e.g., avoiding mating or spawning seasons of fish species).
Simultaneously emitting sources, such that their signals overlap in the (seismic) record, is also known in the industry as “blending”. Conversely, separating signals from two or more simultaneously emitting sources is also known as “deblending” and the data from such acquisitions as “blended data”.
Simultaneous source acquisition has a long history in land seismic acquisition dating back at least to the early 1980's. Commonly used seismic sources in land acquisition are vibroseis sources which offer the possibility to design source signal sweeps such that it is possible to illuminate the sub-surface “sharing” the use of certain frequency bands to avoid simultaneous interference at a given time from different sources. By carefully choosing source sweep functions, activation times and locations of different vibroseis sources, it is to a large degree possible to mitigate interference between sources. Such approaches are often referred to as slip sweep acquisition techniques. In marine seismic data contexts the term overlapping shooting times is often used for related practices. Moreover, it is also possible to design sweeps that are mutually orthogonal to each other (in time) such that the response from different sources can be isolated after acquisition through simple cross-correlation procedures with sweep signals from individual sources. We refer to all of these methods and related methods to as “time encoded simultaneous source acquisition” methods and “time encoded simultaneous source separation” methods.
The use of simultaneous source acquisition in marine seismic applications is more recent as marine seismic sources (i.e., airgun sources) do not appear to yield the same benefits of providing orthogonal properties as land seismic vibroseis sources, at least not at a first glance. Western Geophysical was among the early proponents of simultaneous source marine seismic acquisition suggesting to carry out the separation as a pre-processing step by assuming that the reflections caused by the interfering sources have different characteristics. Beasley et al. (1998) exploited the fact that provided that the sub-surface structure is approximately layered, a simple simultaneous source separation scheme can be achieved for instance by having one source vessel behind the spread acquiring data simultaneously with the source towed by the streamer vessel in front of the spread. Simultaneous source data recorded in such a fashion is straightforward to separate after a frequency-wavenumber (wk) transform as the source in front of the spread generates data with positive wavenumbers only whereas the source behind the spread generates data with negative wavenumbers only.
Another method for enabling or enhancing separability is to make the delay times between interfering sources incoherent (Lynn et al., 1987). Since the shot time is known for each source, they can be lined up coherently for a specific source in for instance a common receiver gather or a common offset gather. In such a gather all arrivals from all other simultaneously firing sources will appear incoherent. To a first approximation it may be sufficient to just process the data for such a shot gather to final image relying on the processing chain to attenuate the random interference from the simultaneous sources (aka. passive separation). However, it is of course possible to achieve better results for instance through random noise attenuation or more sophisticated methods to separate the coherent signal from the apparently incoherent signal (Stefani et al., 2007; Ikelle 2010; Kumar et al. 2015). In recent years, with elaborate acquisition schemes to for instance acquire wide azimuth data with multiple source and receiver vessels (Moldoveanu et al., 2008), several methods for simultaneous source separation of such data have been described, for example methods that separate “random dithered sources” through inversion exploiting the sparse nature of seismic data in the time-domain (i.e., seismic traces can be thought of as a subset of discrete reflections with “quiet periods” in between; e.g., Akerberg et al., 2008; Kumar et al. 2015). A recent state-of-the-art land example of simultaneous source separation applied to reservoir characterization is presented by Shipilova et al. (2016). Existing simultaneous source acquisition and separation methods based on similar principles include quasi random shooting times, and pseudo random shooting times. We refer to all of these methods and related methods to as “random dithered source acquisition” methods and “random dithered source separation” methods. “Random dithered source acquisition” methods and “random dithered source separation” methods are examples of “space encoded simultaneous source acquisition” methods and “space encoded simultaneous source separation” methods.
A different approach to simultaneous source separation has been to modify the source signature emitted by airgun sources. Airgun sources comprise multiple (typically three) sub-arrays each comprised of several individual airguns or clusters of smaller airguns. Whereas in contrast to land vibroseis sources, it is not possible to design arbitrary source signatures for marine airgun sources, one in principle has the ability to choose firing time (and amplitude i.e., volume) of individual airgun elements within the array. In such a fashion it is possible to choose source signatures that are dispersed as opposed to focused in a single peak. Such approaches have been proposed to reduce the environmental impact in the past (Ziolkowski, 1987) but also for simultaneous source shooting.
Abma et al. (2015) suggested to use a library of “popcorn” source sequences to encode multiple airgun sources such that the responses can be separated after simultaneous source acquisition by correlation with the corresponding source signatures following a practice that is similar to land simultaneous source acquisition. The principle is based on the fact that the cross-correlation between two (infinite) random sequences is zero whereas the autocorrelation is a spike. It is also possible to choose binary encoding sequences with better or optimal orthogonality properties such as Kasami sequences to encode marine airgun arrays (Robertsson et al., 2012). Mueller et al. (2015) propose to use a combination of random dithers from shot to shot with deterministically encoded source sequences at each shot point. Similar to the methods described above for land seismic acquisition we refer to all of these methods and related methods to as “time encoded simultaneous source acquisition” methods and “time encoded simultaneous source separation” methods.
Yet another approach is to fire a sequence of source arrays, one or more of which has a random time dither applied relative to the adjacent source points, but at a shorter time interval, for example, five seconds rather than the conventional ten. This has the advantage of keeping the shallow part of each shot free from interference, whilst mitigating the drop in fold. For example, conventional exploration seismic involves two identical source arrays, offset laterally from each other by, for example, 50 m (source centre to source centre). The firing cycle is Port—starboard—port—starboard, such that a source fires every ten seconds, into different sub-surface lines. This results in half-fold data relative to single source. Experiments with triple source using the same approach resulted in ⅓ fold data, considered insufficient. The partially overlapping approach in the above dual source example, would involve firing every 5 seconds, returning to full fold. Employing the same approach with three partially overlapping sources and a five second shot interval would result in limited fold drop and undisturbed shallow data. However, extrapolating this form three to four sources, for example (and temporarily ignoring the issues outlined above about overall sub-array capacity) would require, for example, a 2-3 second shot interval, resulting in limited undisturbed data lengths and loss of fold. Taking into consideration the practicalities, it has also been presented (for example, Hager, 2016), to arrange the firing sequence such that individual airgun sub-arrays may form part of more than one array, as noted above. However, the interference of adjacent shots (even mitigated by dither) and the loss of fold are unavoidable and their effects increase as attempts are made to increase the total number of arrays.
Recently there has been an interest in industry to explore the feasibility of marine vibrator sources as they would, for instance, appear to provide more degrees of freedom to optimize mutually orthogonal source functions beyond just binary orthogonal sequences that would allow for a step change in simultaneous source separation of marine seismic data. Halliday et al. (2014) suggest to shift energy in ωk-space using the well-known Fourier shift theorem in space to separate the response from multiple marine vibrator sources. Such an approach is not possible with most other seismic source technology (e.g., marine airgun sources) which lack the ability to carefully control the phase of the source signature (e.g., flip polarity).
The recent development of “signal apparition” suggests an alternative approach to deterministic simultaneous source acquisition that belongs in the family of “space encoded simultaneous source acquisition” methods and “space encoded simultaneous source separation” methods. Robertsson et al. (2016) show that by using modulation functions from shot to shot (e.g., a short time delay or an amplitude variation from shot to shot), the recorded data on a common receiver gather or a common offset gather will be deterministically mapped onto known parts of for instance the ωk-space outside the conventional “signal cone” where conventional data is strictly located (
Consider a seismic experiment where a source is excited sequentially for multiple source locations along a line while recording the reflected wavefield on at least one receiver. The source may be characterized by its temporal signature. In the conventional way of acquiring signals representing a wavefield the source may be excited using the same signature from source location to source location, denoted by integer n. Next, consider the alternative way of acquiring such a line of data using a periodic sequence of source signatures: every second source may have a constant signature and every other second source may have a signature which can for example be a scaled or filtered function of the first source signature. Let this scaling or convolution filter be denoted by a(t), with frequency-domain transform A(ω). Analyzed in the frequency domain, using for example a receiver gather (one receiver station measuring the response from a sequence of sources) recorded in this way, can be constructed from the following modulating function m(n) applied to a conventionally sampled and recorded set of wavefield signals:
m(n)=½[1+(−1)n]+½A[1−(−1)n],
which can also be written as
m(n)=½[1+eiπn]+½A[1−eiπn]. (0.1)
By applying the function m in Eq. 0.1 as a modulating function to data ƒ(n) before taking a discrete Fourier transform in space (over n), F(k)=(ƒ(n)), the following result can be obtained:
which follows from a standard Fourier transform result (wavenumber shift) (Bracewell, 1999).
Eq. 0.2 shows that the recorded data ƒ will be scaled and replicated into two places in the spectral domain as illustrated in
Part of the data will remain at the signal cone centered around k=0 (denoted by H+ in
This process may be referred to as, “signal apparition” in the meaning of “the act of becoming visible”. In the spectral domain, the wavefield caused by the periodic source sequence is nearly “ghostly apparent” and isolated.
In practice the length of the source sequences is finite. While it is true that the Fourier series transform of any finite sequence will be periodic with a periodicity related to the length of the sequence, this type of periodicity is not what we refer to when describing periodic constraints in the current invention. Instead, in this invention we use the term periodic to denote a sequence that repeats itself at least once within the length of the sequence (i.e., the periodicity is less than half the sequence length).
A particular application of interest that can be solved by using the result in Eq. (0.2) is that of simultaneous source separation. Assume that a first source with constant signature is moved along an essentially straight line with uniform sampling of the source locations where it generates the wavefield g. Along another essentially straight line a second source is also moved with uniform sampling. Its signature is varied for every second source location according to the deterministic modulating sequence 700, generating the wavefield h. The summed, interfering data ƒ=g+h are recorded at a receiver location.
In the frequency-wavenumber domain, where the recorded data are denoted by F=G+H, the H-part is partitioned into two components H+ and H− with H=H++H− where the H−-component is nearly “ghostly apparent” and isolated around the Nyquist-wavenumber [
Although the above description has focused on acquisition along essentially straight lines, the methodology applies equally well to curved trajectories such as coil-shaped trajectories, circles, or other smoothly varying trajectories or sequences of source activations.
The concept may be extended to the simultaneous acquisition of more than two source lines by choosing different modulation functions for each source.
Acquiring a source line where the first two source locations have the same signature, followed by two again with the same signature but modified from the previous two by the function A(ω) and then repeating the pattern again until the full source line has been acquired, will generate additional signal cones centered around +kN/2.
For data acquired along a single line, the dimension of the lozenge-shaped regions is a function of the velocity of the recording medium c, the number of simultaneously emitting sources n and the distance between source firing locations along the direction of the source line Δx. The frequency at the top of the lozenge-shaped regions, ƒtop, is:
The frequency at the middle of the lozenge-shaped regions, ƒmid, below which the data are fully separated is:
Outside the lozenge-shaped region the response from the sources is not separated and overlap. Different methods for separating the wavefield contributions from the different sources in this region have been proposed, many of which rely on the exact or nearly exact separation of the wavefields within the lozenge-shaped regions (e.g., Andersson et al., 2016). Therefore, the larger the lozenge-shaped region is the larger area can first of all be exactly or nearly exactly reconstructed. However, in addition a larger lozenge-shaped region will also enhance the quality of separating wavefields in the overlapping region.
Instead of using the method of signal apparition, other methods for simultaneous source separation such as random dithering encoding can also be used to exactly or nearly exactly separate the response from different sources (Andersson et al., 2017). The region of exact or nearly exact separation will be smaller than the case of signal apparition. However, in a region in the frequency wavenumber space the number of unknowns is smaller than the number of equations under the assumption that the signal belongs in cones bounded by the velocity of the recording medium resulting in the ability to exactly or nearly exactly separate source contributions in a simultaneous source experiment below a certain frequency also in the case of randomly dithered sources.
Methods for increasing the frequency range for exact or nearly exact separation of individual contributions from sources recorded in a simultaneous source seismic experiment, including (but not necessarily) by means of the signal apparition approach mentioned above or a conventional method for simultaneous source separation such as methods based on random dithering substantially as shown in and/or described in connection with at least one of the figures, and as set forth more completely in the claims.
Advantages, aspects and novel features of the present invention, as well as details of an illustrated embodiment thereof, may be more fully understood from the following description and drawings.
In the following description reference is made to the attached figures, in which:
The following examples may be better understood using a theoretical overview as presented below.
It is herein proposed to use acquisition patterns in a plane instead of just a line to reduce ambiguity in the overlapping region thereby causing the area of exact or nearly exact separation to be larger.
By a plane it is meant a portion of the (infinite) horizontal plane covering an area corresponding to the length of the shotlines and the length in the crossline direction occupied by adjacent shotlines. Note that the number of sampling locations in the inline and crossline directions will limit the resolution properties of the Fourier transform. In practice the number of points should be greater than or equal to 8 or more. Specifically, for a Bravais lattice (x1,x2)=(u1,1k1+u1,2k2,u2,1k1+u2,2k2) thus including rectangular sampling, staggered grid and hexagonal sampling, K1min≤k1<K1max, K2min≤k2<K2max, it should hold that K1max−K1min≥8 and K2max−K2min≥8.
Method for separating wavefields in the overlapping region includes utilizing the analytic part or the quaternion analytic part of the wavefields. In the following we describe the procedures in one spatial coordinate although it generalizes to two coordinates or more. We will use the notation
{circumflex over (ƒ)}(ξ)=∫−∞∞ƒ(x)e−2πixξdx
for the Fourier transform.
Let denote the cone ={(ω,ξ):|ω|>|ξ|}, and let denote the non-aliased (diamond shaped) set =\({(ω,ξ):|ω|>|ξ−½|}∪{(ω,ξ):|ω|>|ξ+½|}).
Suppose that
d(t,j)=ƒ1(t,j)+ƒ2(t−Δt(−1)j,j) (1)
is a known discrete sampling in x=j recorded at a first sampling interval. Note that due to this type of apparition sampling, the data d will always have aliasing effects present if the data is band unlimited in the temporal frequency direction.
If ƒ1 and ƒ2 represent seismic data recorded at a certain depth, it will hold that supp()⊂ and supp()⊂. We will assume that the source locations of ƒ1 and ƒ2 are relatively close to each other. Let
It is shown in Andersson et al. (2016) that
For each pair of values (ω,ξ)∈, most of the terms over k in (2) vanish (and similarly for D2), which implies that (ω,ξ) and (ω,ξ) can be recovered through
given that sin(2πΔtω)≠0.
By including an amplitude variation in (1), the last condition can be removed. For values of (ω,ξ)∉\ it is not possible to determine the values of (ω,ξ) and (ω,ξ) without imposing further conditions on the data.
Given a real valued function ƒ with zero average, let
ƒa(t)=2∫0∞ƒ∞−∞ƒ(t′)e2πi(t−′)ωdt′dω.
The quantity is often referred to as the analytic part of ƒ, a description that is natural when considering Fourier series expansions in the same fashion and comparing these to power series expansions of holomorphic functions. It is readily verified that Re(ƒa)=ƒ.
As an illustrative example, consider the case where
ƒ(t)=cos(2πt)
for which it holds that
ƒa(t)=e2πit.
Now, whereas |ƒ(t)| is oscillating, |ƒa(t)|=1, i.e., it has constant amplitude. In terms of aliasing, it can often be the case that a sampled version of ≡ƒa| exhibits no aliasing even if ƒ and |ƒ| do so.
Let us now turn our focus back to the problem of recovering (ω,ξ) and (ω,ξ) for (ω,ξ)∉. We note that due to linearity, it holds that
d
a(t,j)=ƒ1a(t,j)+ƒ2a(t−Δt(−1)j,j).
A natural condition to impose is that the local directionality is preserved through the frequency range. The simplest such case is when ƒ1 and ƒ2 are plane waves (with the same direction), i.e, when
ƒ1(t,x)=h1(t+bx), and ƒ2(t,x)=h2(t+bx).
Without loss of generality, we assume that b>0. We note that
A similar formula holds for .
Let us now assume that ω<½. Inspecting (2) we see that if, e.g., −½<ξ<0 then all but three terms disappear and therefore the blended data satisfies
Let wh, and wl be two filters (acting on the time variable) such that wh has unit L2 norm, and such that wh has a central frequency of ω0 and ωl has a central frequency of ω0/2. For the sake of transparency let wh=wl2. Suppose that we have knowledge of (ω,ξ) and (ω,ξ) for ω<ω0, and that the bandwidth of wl is smaller than ω0/2.
Let g1=ƒ1a*wl and g2=ƒ2a*wl. Note that, e.g.,
g
1(t,x)=h1a*wl(t+bx),
so that g1 is a plane wave with the same direction as ƒ1. Moreover, |g1| will typically be mildly oscillating even when ƒ1 and |ƒ1| are oscillating rapidly.
Let
be the phase function associated with g1, and define p2 in a likewise manner as phase function for g2. If wl is narrowbanded, g1 will essentially only contain oscillations of the form
i.e., |g1(t,x)| is more or less constant.
Under the narrowband assumption on wl (and the relation wh=wl2), we consider
d
h(t,x)=(da*wh)(t,x)≈
By multiplication by
d
h(t,x)=
In the Fourier domain, this amounts to two delta-functions; one centered at the origin and one centered at (0,−½). Here, we may identify the contribution that comes from ƒ2 by inspecting the coefficient in front of the delta-function centered at (0,−½). By the aid of the low-frequency reconstructions g1 and g2, it is thus possible to move the energy that originates from the two sources so that one part is moved to the center, and one part is moved to the Nyquist wavenumber. Note that it is critical to use the analytic part of the data to obtain this result. If the contributions from the two parts can be isolated from each other, it allows for a recovery of the two parts in the same fashion as in (3). Moreover, as the data in the isolated central centers is comparatively oversampled, a reconstruction can be obtained at a higher resolution than the original data. Afterwards, the effect of the phase factor can easily be reversed, and hence a reconstruction at a finer sampling, i.e. at a smaller sampling interval than the original can be obtained.
A similar argument will hold in the case when the filters wl and wh have broader bandwidth. By making the approximation that
p
1(t,x)≈eπiω
we get that
d
h(t,x)=
and since wh is a bandpass filter, (ω,ξ) will contain information around the same two energy centers, where the center around (0,−½) will contain only information about ƒ2. By suppressing such localized energy, we can therefore extract only the contribution from ƒ2 and likewise for ƒ1.
The above procedure can now be repeated with ω0 replaced by ω1=βω0 for some β>1. In this fashion we can gradually recover (dealias) more of the data by stepping up in frequency. We can also treat more general cases. As a first improvement, we replace the plane wave assumption by a locally plane wave assumption, i.e., let φα be a partition of unity (Σαφα2=1), and assume that
ƒ1(t,x)φα2(t,x)≈h1,α(t+bax)φα2(t,x).
In this case the phase functions will also be locally plane waves, and since they are applied multiplicatively on the space-time side, the effect of (4) will still be that energy will be injected in the frequency domain towards the two centers at the origin and the Nyquist wavenumber.
Now, in places where the locally plane wave assumption does not hold, the above procedure will not work. This is because as the phase function contains contributions from several directions at the same location, the effect of the multiplication in will no longer correspond to injecting the energy of D1 (and D2) towards the two centers around the origin and the Nyquist number. However, some of this directional ambiguity can still be resolved.
In fact, upon inspection of (2), it is clear that the energy contributions to a region with center (ω0,ξ0) must originate from regions with centers at (ω0,ξ0+k/2) for some k. Hence, the directional ambiguity is locally limited to contributions from certain directions. We will now construct a setup with filters that will make use of this fact.
Let us consider the problem where we would like to recover the information from a certain region (ω0,ξ0). Due to the assumption that ƒ1 and ƒ2 correspond to measurements that take place close to each other, we assume that ƒ1 and ƒ2 have similar local directionality structure. From (2) we know that energy centered at (ω0,ξ0) will be visible in measurements D1 at locations (ω0,ξ0+k/2). We therefor construct a (space-time) filter wh, that satisfies
We now want to follow a similar construction for the filter wl. Assuming that there is locally only a contribution from a direction associated with one of the terms over k above, we want the action of multiplying with the square of the local phase to correspond to a filtration using the part of wh that corresponds to that particular k.
This is accomplished by letting
where {circumflex over (Ψ)}={circumflex over (ψ)}*{circumflex over (ψ)}.
Under the assumption that ƒ1*wh and ƒ2*wj has a local plane wave structure, we may now follow the above procedure to recover these parts of ƒ1 and ƒ2 (by suppressing localized energy as described above). We may then completely recover ƒ1 and ƒ2 up to the temporal frequency ω0 by combining several such reconstructions, and hence we may proceed by making gradual reconstructions in the ω variable as before.
Let be the quaternion algebra (Hamilton, 1844). An element g∈ can be represented as q=q0+iq1+jq2+kq3, where the qj are real numbers and i2=j2=k2=ijk=1. We also recall Euler's formula, valid for i,j,k:
e
iθ=cos θ+i sin θ,ejθ=cos θ+j sin θ,ekθ=cos θ+k sin θ.
Note that although i,j,k commute with the reals, quaternions do not commute in general. For example, we generally have eiθejϕ≠ejϕeiθ which can easily be seen by using Euler's formula. Also recall that the conjugate of q=q0+iq1+jq2+kq3 is the element q*=q0−iq1−jq2−kq3. The norm of q is defined as ∥q∥=(qq*)1/2=(q02+q12+q22+q32)1/2.
Given a real valued function ƒ=ƒ(t,x), we define the quaternion Fourier transform (QFT) of ƒ by
ƒ(ω,ξ)=∫∞−∫∞−∞e−2πitωƒ(t,x)e−2πjxξdtdx.
Its inverse is given by
ƒ(t,x)=−1(ƒ)(t,x)=∫∞−∫∞−∞e−2πitωƒ(ω,ξ)e2πjxξdωdξ.
In a similar fashion, it is possible to extend the Fourier transform to other hypercomplex representations, e.g., octanions (van der Blij, 1961), sedenions (Smith, 1995) or other Cayley or Clifford algebras. A similar argument applies to other well-known transform domains (e.g., Radon, Gabor, curvelet, etc.).
Let
Using χ we define ƒq:2→ as
ƒq=−1χƒ.
We call ƒq the quaternion part of ƒ. This quantity can be seen as a generalization of the concept of analytic part. For the analytic part, half of the spectrum is redundant. For the case of quaternions, three quarters of the data is redundant.
In a similar fashion, it is possible to extend the analytic part to other hypercomplex representations, e.g., octanions (van der Blij, 1961), sedenions (Smith, 1995) or other Cayley or Clifford algebras.
The following results will prove to be important: Let ƒ(t,x)=cos u, where u=2π(at +bx)+c with a>0. If b>0 then
ƒq(t,x)=cos u+i sin u+j sin u−k cos u,
and if b<0 then
ƒq(t,x)=cos u+i sin u−j sin u+k cos u.
The result is straightforward to derive using the quaternion counterpart of Euler's formula. Note that whereas |ƒ(t,x)| is oscillating, ∥ƒq∥=√{square root over (2)}, i.e., it has constant amplitude. In terms of aliasing, it can often be the case that a sampled version of ∥ƒq∥ exhibits no aliasing even if ƒ and |ƒ| do so.
Assume that ƒ(t,x)=cos(u), and that g(t,x)=cos(ν), where u=2π(a1t+b1x)+e1 and ν=2π(a2t+b2x)+e2 with a1,a2≥0. It then holds that
with similar expressions if b1<0.
Let us describe how to recover (ω,ξ) and (ω,ξ) us the quaternion part. We will follow the same procedure as before, and hence it suffices to consider the case where ƒ1=h1(t+bx), ƒ2=h2(t+bx), with b>0, and ω<½. Let wh and wl be two (real-valued) narrowband filters with central frequencies of ω0 and ω0/2, respectively, as before. From (2), it now follows that
d*w
h(t,x)≈c1 cos(2πω0(t+bx)+e1)+c2 cos(2πω0(t+{tilde over (b)}x)+e2),
for some coefficients c1,c2, and phases e1,e2, and with b<0.
Since ƒ1 and ƒ2 are known for ω=ω0/2, we let
g
1(t,x)=ƒ1*wl(t,x)≈c3 cos(πω0(t+bx)+e3).
We compute the quaternion part g1q of g1, and construct the phase function associated with it as
and define p2 in a likewise manner as the phase function for g2.
Let dq be the quaternion part of d*wh. It then holds that after a left and right multiplication of conjugate of the phase factors p1 and p2
This result is remarkable, since the unaliased part of d is moved to the center, while the aliased part remains intact. Hence, it allows for a distinct separation between the two contributing parts.
It is herein proposed to increase the maximum frequency for fully recovering the contributions in recorded a wavefield from individual sources in a simultaneous source survey. More precisely, this is achieved by considering sampling the same wavefield along a plurality of parallel sail-lines to unambiguously delineate regions of overlap in a Fourier-wavenumber plane of at least two spatial dimensions.
Let us begin by introducing notation and recapitulating the theory for regular seismic apparition. We will use the notation
{circumflex over (ƒ)}(ξ)=∫∞−∞ƒ(x)e−2πixξdx
for the Fourier transform in one variable, and consequently {circumflex over (ƒ)}(ω,ξ1,ξ2) for the Fourier transform of two dimensional function ƒ(t,x1,x2) with a time (t) and spatial (x1,x2) dependence. When referring to Fourier transforms with respect to only part of the variables we will use the {circumflex over ( )} notation and use the variable names to implicitly specify with regards to which dimensions the transform is applied.
Suppose that ƒ(t,x1,x2) is a function with frequency support in two cones of the form
The constraint comes from assuming that the function ƒ represent the recording of a wavefield at time t at a fixed receiver coordinate, source coordinates (x1,x2), and fixed depth, where the recorded wave field at this depth is a solution to the homogeneous wave equation with a velocity c. The wavefields are generated at discrete values of (x1,x2) which we assume to be equally spaced with sampling distances Δx
We now consider the case where several sources are used simultaneously. In this presentation we assume that the M sources are aligned sequentially, although the theory can easily be adjusted to cover more general sampling formations. Moreover, in this presentation, we will assume that the different sources are fired with a small internal time delays, that vary with period M. This variation can be of more general form, for instance varying with a delay pattern that includes a heteroscale variation (several superimposed or products of periodic or non-periodic functions), random or quasi-random time delay patterns or variations in source amplitude for instance. Let us denote the periodic delay pattern by Δm
The Poisson sum formula
Σk=−∞∞ƒ(k)=Σk=−∞∞ƒ(k)
can be modified (by using the Fourier modulation rule) as
By the standard properties of the Fourier transform it is straightforward to show that
hold for the spatial sampling parameter Δx and some fixed spatial shift x0.
Let us now consider Fourier representation of the data. We can assume that the sampling in time is fine enough to use the continuous Fourier transform for the temporal part. For the spatial parts, we will expand the data by means of Fourier series representation, thus obtained a representation that is periodic with respect to the continuous frequency-wavenumber parameters ξ1 and ξ2.
The transform thus takes the shape
By taking a one-dimensional Fourier transform with respect to the time variable it holds that
Let us now focus on the part
Σk
By using the version of the Poisson sum formula above, we can rewrite the expression above as
Using a similar argument for the sum over k2 we obtain
It is now important to note that the periodicity of ĥ with respect to ξ2 is (1/M) and not 1 as it is for the periodicity with respect to ξ1. To see this, note that for any integer k2′ it holds that
It now follows that
will have period 1 in the ξ1-direction and period 1/M in the ξ2-direction. It is now possible to choose the time delays Δm
Let us now consider what happens for fixed values of ω. Since the support of {circumflex over (ƒ)} lies inside a cone whose width is determined by the spatial sampling parameters and the propagation medium velocity, it follows that the footprint of {circumflex over (ƒ)}(ω,ξ1,ξ2) will be a disk in the (ξ1,ξ2)-plane.
One such scenario would be a vessel travelling along a sail-line, where it is possible to collect information along that line fairly densely. To collect information not only along single lines, the vessel will have to travel along several sail lines. To obtain a dense sampling, these sail lines would therefore have to be laid out close to each other, and this results in that the total measurement scenario takes a long time.
Instead, the vessel could carry sources spread out in the direction perpendicular to the sail line. By using the properties described above it is possible to obtain a sampling that provides full resolution up to a certain frequency ω0 where the overlapping of disk does not prohibit perfect recovery, at an (more) equally spaced sampling lattice than what is obtained by acquiring data along individual sail lines.
An important consideration for the acquisition of data that is rich in low frequencies is related to how we choose to encode the simultaneous sources relative other in for instance choosing the magnitude of the time shifts used for encoding and where the sources are located relative to each other in space.
In the following for simplicity we will discuss the case of two simultaneous sources. However, the same arguments generalizes in a straight forward way to a larger number of sources, for instance with time delays smaller than the time delay considered between the two sources in the following and/or spaced at distances within the two sources considered below.
The combined output of two sources at a certain frequency is A=eiωt+eiω(t+Δt), where Δt is the time shift between the activation time of the two sources and ω is the (angular) frequency of the emitted amplitude spectrum.
The interference manifests itself in an amplitude effect and a phase effect. Both are unraveled during the decoding. However, the level of the interference of the two sources is relevant when considering the signal-to-noise ratio in the acquired data.
For simplicity we consider an average time delay in activation time between the two sources of 50 ms. The simple equation for the combined output shows that frequencies below 6.7 Hz benefit from constructive interference between the two sources.
The spatial separation of the two sources is also important to achieve constructive interference. The phase shift between two sources that are separated by a small distance relative to the distance of propagation can be computed in a straight forward manner using Pythagoras theorem. If we simply consider a case where the distance of propagation is 5000 m in a medium with propagation velocity 1500 m/s (water), the phase shift between two sources spaced 750 m apart in a direction perpendicular to the plane of propagation is 37 ms. In such a case we will obtain constructive interference below 10 Hz. However, in the broadside direction the limit for constructive interference is lower as the phase shift becomes greater. Below 4 Hz we can expect constructive interference for all azimuths and emergence angles smaller than 15 degrees relative to the vertical which will enable the acquisition for instance of refracted arrivals for tomography and full waveform inversion propagating in the deeper part of the subsurface of interest.
A synthetic example was created using an acoustic 3D finite-difference synthetic data set mimicking a seabed seismic acquisition geometry over a complex sub surface model.
In the example a 25 m by 25 m shot grid was generated over a single seabed node receiver. The source had a spectrum up to 30 Hz.
In
In the description of the embodiments of the invention it is clear that acquisition lines or source lines do not necessarily need to be straight lines but can correspond to curved trajectories in the acquisition plane. It is also clear that in such a case, the term spatial directions is used to denote the path describing these trajectories.
The methods described herein may be understood as a series of logical steps and (or grouped with) corresponding numerical calculations acting on suitable digital representations of the acquired seismic recordings, and hence can be implemented as computer programs or software comprising sequences of machine-readable instructions and compiled code, which, when executed on the computer produce the intended output in a suitable digital representation. More specifically, a computer program can comprise machine-readable instructions to perform the following tasks:
(1) Reading all or part of a suitable digital representation of the obtained wave field quantities into memory from a (local) storage medium (e.g., disk/tape), or from a (remote) network location;
(2) Repeatedly operating on the all or part of the digital representation of the obtained wave field quantities read into memory using a central processing unit (CPU), a (general purpose) graphical processing unit (GPU), or other suitable processor. As already mentioned, such operations may be of a logical nature or of an arithmetic (i.e., computational) nature. Typically the results of many intermediate operations are temporarily held in memory or, in case of memory intensive computations, stored on disk and used for subsequent operations; and
(3) Outputting all or part of a suitable digital representation of the results produced when there no further instructions to execute by transferring the results from memory to a (local) storage medium (e.g., disk/tape) or a (remote) network location.
Computer programs may run with or without user interaction, which takes place using input and output devices such as keyboards or a mouse and display. Users can influence the program execution based on intermediate results shown on the display or by entering suitable values for parameters that are required for the program execution. For example, in one embodiment, the user could be prompted to enter information about e.g., the average inline shot point interval or source spacing. Alternatively, such information could be extracted or computed from metadata that are routinely stored with the seismic data, including for example data stored in the so-called headers of each seismic trace.
Next, a hardware description of a computer or computers used to perform the functionality of the above-described exemplary embodiments is described with reference to
Further, the claimed advancements may be provided as a utility application, background daemon, or component of an operating system, or combination thereof, executing in conjunction with CPU 1000 and an operating system such as Microsoft Windows 10, UNIX, Solaris, LINUX, Apple MAC-OS and other systems known to those skilled in the art.
The hardware elements in order to achieve the computer can be realized by various circuitry elements, known to those skilled in the art. For example, CPU 1000 can be a Xenon or Core processor from Intel of America or an Opteron processor from AMD of America, or may be other processor types that would be recognized by one of ordinary skill in the art (for example so-called GPUs or GPGPUs). Alternatively, the CPU 1000 can be implemented on an FPGA, ASIC, PLD or using discrete logic circuits, as one of ordinary skill in the art would recognize. Further, CPU 1000 may be implemented as multiple processors cooperatively working in parallel to perform the instructions of the inventive processes described above.
Number | Date | Country | Kind |
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1803535.2 | Mar 2018 | GB | national |
This application is a continuation of PCT Application No. PCT/IB2019/051440, filed Feb. 21, 2019, which claims priority to Great Britain Application No. 1803535.2, filed Mar. 5, 2018. The entire contents of the above-identified applications are incorporated herein by reference.
Number | Date | Country | |
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Parent | PCT/IB2019/051440 | Feb 2019 | US |
Child | 17011315 | US |