Skip to content
Brent$117.6Gas TTF$1,192USD453.87 ₸
MunaiHub

Equations: Geophysics and seismic surveying

The equations of the “Geophysics and seismic surveying” lessons in “Petroleum geoscience”, with their conditions and units, and what each symbol means in them.

Gravity anomaly above a sphere (a point mass)
Δg(x)=GMz(x2+z2)3/2,M=43πa3 Δρ\Delta g(x) = \frac{G M z}{(x^2 + z^2)^{3/2}}, \qquad M = \tfrac{4}{3}\pi a^3\,\Delta\rho

SI; 1 mGal =10−5= 10^{-5} m/s²

Holds when: The body is a uniform sphere or any spherically symmetric body: outside it, its field equals that of a point mass at the centre. The host rocks are uniform horizontally. The effect of everything else (deep sequences, basement relief) has already been subtracted as a regional background. Corrections for elevation and terrain have moved the observations to a horizontal surface (next section). We measure the vertical component; an ordinary gravimeter does not sense the horizontal components.

Geophysical exploration methods →
Half-width of the anomaly and the depth of the centre of the sphere
x1/2=z22/3−1≈0.7664 z,z≈1.305 x1/2x_{1/2} = z\sqrt{2^{2/3} - 1} \approx 0.7664\,z, \qquad z \approx 1.305\,x_{1/2}

any consistent units of length

Holds when: The body is a sphere (a point mass), and the anomaly is isolated: the regional background has been subtracted correctly. For other shapes the factor is different. For a long horizontal cylinder (a body elongated along strike), x1/2=zx_{1/2} = z. For a thin vertical column extending to a great depth, x1/2=3 zx_{1/2} = \sqrt3\,z, where zz is the depth of its top.

Geophysical exploration methods →
Normal gravity on the ellipsoid
gn(φ)=978,032.7 (1+0.0053024sin⁡2φ−0.0000058sin⁡22φ)g_\text{n}(\varphi) = 978{,}032.7\,\bigl(1 + 0.0053024\sin^2\varphi - 0.0000058\sin^2 2\varphi\bigr)

mGal

Holds when: An approximate form of the normal field for the ellipsoid (the smooth, slightly flattened model of the Earth's shape) of the Geodetic Reference System 1980 (GRS80) adopted in geodesy. We calculate the correction from the latitude of each station.

Geophysical exploration methods →
Bouguer anomaly
ΔgB=g−gn(φ)+0.3086 h−0.04194 ρ h+δgT\Delta g_\text{B} = g - g_\text{n}(\varphi) + 0.3086\,h - 0.04194\,\rho\,h + \delta g_\text{T}

mGal; hh in m, ρ\rho in g/cm³

Holds when: 0.3086 mGal/m is the mean normal vertical gradient: gravity decreases by this amount for every metre of rise. This is the free-air correction (also called the Faye correction). 0.04194 ρh0.04194\,\rho h is the attraction of an infinite flat slab of thickness hh, that is, 2πGρh2\pi G\rho h in milligals for a density in g/cm³. This is the correction for the intermediate layer (also called the Bouguer correction). The terrain correction accounts for how the ground around the station differs from a flat slab. On land it is positive both for hills above the station and for hollows below it. For a station below the reference level, hh is negative. At sea and in the air the corrections are different, and on a moving ship or aircraft we add the Eötvös correction for the motion.

Geophysical exploration methods →
Anomaly of a magnetic pole — the top of a long vertical body
ΔT(x)=C z(x2+z2)3/2,C=κ B0 A4π\Delta T(x) = \frac{C\,z}{(x^2 + z^2)^{3/2}}, \qquad C = \frac{\kappa\,B_0\,A}{4\pi}

xx, zz in m; AA in m²; B0B_0 and ΔT\Delta T in nT

Holds when: The body is a thin vertical column, magnetised along its axis, that extends far deeper than its top. The field of the lower end is negligible, so only the field of the upper “pole” remains. The magnetisation is induced and the field is vertical, or else the map has been reduced to the pole. The susceptibility is small (κ≪1\kappa \ll 1), and we do not take the demagnetisation of the body into account (the weakening of its magnetisation by its own field).

Geophysical exploration methods →
Depth from two-way time
z=∑i=1nVi ti2,t=∑i=1nti=∑i=1n2hiViz = \sum_{i=1}^{n} \frac{V_i\,t_i}{2}, \qquad t = \sum_{i=1}^{n} t_i = \sum_{i=1}^{n} \frac{2 h_i}{V_i}

SI: m, s, m/s

Holds when: The rays are vertical. After processing, the time section is reduced to the case where the source and the receiver are at the same point. The layers are horizontal, and the velocity in each layer is constant. The velocities are known: from check-shot surveys and vertical seismic profiling (VSP) in wells (measurements of wave travel time from the surface down the hole), from sonic logs (travel time from the sonic log) or, less accurately, from the seismic data themselves.

Geophysical exploration methods →
Total anomalous mass from the integral of the anomaly
∬Δg  dA=2πGM\iint \Delta g\,\dd A = 2\pi G M

SI

Holds when: The integral is over the whole plane: the anomaly is measured far beyond the body and is completely separated from the regional background. The observation surface is flat, and all the anomalous masses lie below it.

Geophysical exploration methods →
Wavelength
λ=Vf\lambda = \frac{V}{f}

SI: m, m/s, Hz

Holds when: A wave of one frequency. A real wavelet has many frequencies, and we calculate the wavelength at a characteristic frequency. We must say which one (see the section on the wavelet). At a boundary the frequency stays the same, and the wavelength grows where the speed grows.

Seismic waves, acoustic impedance and reflections →
Acoustic impedance
Z=ρ VpZ = \rho\,V_p

SI: kg/(m²·s)

Holds when: The rock is uniform on the scale of the wavelength. A package of layers much thinner than the wavelength is “seen” by the wave through its averaged properties.

Seismic waves, acoustic impedance and reflections →
Reflection coefficient at normal incidence
R=Z2−Z1Z2+Z1R = \frac{Z_2 - Z_1}{Z_2 + Z_1}

dimensionless; impedances in any equal units

Holds when: Normal incidence of a plane P-wave. At oblique incidence, part of the energy goes into S-waves, and RR depends on the angle (see the section on AVO). The boundary is flat and extended, much wider than the zone from which the reflection comes. The rocks on both sides of the boundary are elastic and uniform.

Seismic waves, acoustic impedance and reflections →
Ricker wavelet
w(t)=(1−2π2fp2t2)e−π2fp2t2w(t) = \left(1 - 2\pi^2 f_p^2 t^2\right)e^{-\pi^2 f_p^2 t^2}

SI: s, Hz

Holds when: A model of a zero-phase wavelet. A real wavelet is found from seismic data near a well, and its shape differs from the Ricker shape. The shape of the wavelet does not change within the time interval under consideration.

Seismic waves, acoustic impedance and reflections →
Convolution model of a seismic trace
s(t)=∑kRk w(t−τk)+n(t)s(t) = \sum_k R_k\,w(t - \tau_k) + n(t)

time in s; amplitudes as fractions of the amplitude of the incident wavelet

Holds when: The layers are horizontal and the wave falls at normal incidence: a one-dimensional model. Only single reflections are included. Multiples (waves reflected many times between boundaries), transmission losses (energy lost on passing through boundaries) and spherical divergence (weakening as the wavefront spreads out) are left out, or compensated by processing. The wavelet is the same over the whole interval.

Seismic waves, acoustic impedance and reflections →
Tuning thickness for a Ricker wavelet
Δttun=62πfp≈0.39fp,htun=V Δttun2\Delta t_\text{tun} = \frac{\sqrt6}{2\pi f_p} \approx \frac{0.39}{f_p}, \qquad h_\text{tun} = \frac{V\,\Delta t_\text{tun}}{2}

SI: s, Hz, m, m/s

Holds when: A zero-phase Ricker wavelet. For other wavelets the factor is different. The reflections from the top and base are equal in size and opposite in sign, and the neighbouring reflections are far away.

Seismic waves, acoustic impedance and reflections →
Absorption at constant quality factor
AA0=e−πft/Q\frac{A}{A_0} = e^{-\pi f t/Q}

SI: Hz, s; QQ is dimensionless

Holds when: The quality factor does not depend on frequency in the seismic range and is the same along the whole path (otherwise we take its average along the path, weighted by time). Spherical divergence and boundary losses are accounted for separately.

Seismic waves, acoustic impedance and reflections →
Two-term approximation of the reflection coefficient (Shuey)
R(θ)≈A+Bsin⁡2θ,A=12 ⁣(ΔVpVp+Δρρ),B=12ΔVpVp−2Vs2Vp2 ⁣(Δρρ+2ΔVsVs)R(\theta) \approx A + B\sin^2\theta,\quad A = \tfrac12\!\left(\frac{\Delta V_p}{V_p} + \frac{\Delta\rho}{\rho}\right),\quad B = \tfrac12\frac{\Delta V_p}{V_p} - 2\frac{V_s^2}{V_p^2}\!\left(\frac{\Delta\rho}{\rho} + 2\frac{\Delta V_s}{V_s}\right)

dimensionless RR, AA, BB; speeds and densities in any consistent units

Holds when: Small relative contrasts of properties at the boundary. Angles of incidence less than about 30°. At larger angles a third term or the exact formulas are needed. A flat boundary between uniform isotropic rocks.

Seismic waves, acoustic impedance and reflections →
Weakening on passing a boundary down and back
T↓T↑=2Z2Z1+Z2⋅2Z1Z1+Z2=1−R2T_\downarrow T_\uparrow = \frac{2Z_2}{Z_1 + Z_2}\cdot\frac{2Z_1}{Z_1 + Z_2} = 1 - R^2

dimensionless

Holds when: Normal incidence, and thick layers, much thicker than the wavelength. In a package of thin layers, multiple reflections inside the layers partly return energy to the transmitted wave, and a simple product of factors overstates the losses.

Seismic waves, acoustic impedance and reflections →
Fold of a 2D line
n=N Δxrec2 Δxshotn = \frac{N\,\Delta x_\text{rec}}{2\,\Delta x_\text{shot}}

the intervals are in the same units of length

Holds when: A regular layout: all channels work, the shots follow one another at a constant interval, and the spread moves with them. The formula applies in the middle of the line. At the ends, the fold rises from one to its full value (figure below). The fold is counted for the nominal layout. Shots skipped because of obstacles, and rejected traces, reduce it.

Seismic acquisition and processing →
Fold of a 3D survey with an orthogonal layout
n=Nch Δxrec2 DSL⋅NRL2n = \frac{N_\text{ch}\,\Delta x_\text{rec}}{2\,D_\text{SL}}\cdot\frac{N_\text{RL}}{2}

lengths in the same units

Holds when: An orthogonal layout: each source point records a patch that is symmetric about it along and across the lines. Far from the edges of the survey. Near the edges the fold builds up from low values, as at the ends of a 2D line.

Seismic acquisition and processing →
Static correction of a station to the datum
tst=hLVZVLVZ+E−hLVZ−E0V0t_\text{st} = \frac{h_\text{LVZ}}{V_\text{LVZ}} + \frac{E - h_\text{LVZ} - E_0}{V_0}

SI: m, m/s, s

Holds when: Rays near the surface are vertical. In the slow LVZ the wave really is refracted to nearly vertical. The datum is below the base of the LVZ, and the LVZ is uniform beneath the station. The correction of a trace is the sum of the corrections of its source point and its receiver point (the corrections are surface-consistent: a point has the same correction for every trace). If the charge is fired below the LVZ, only the second term remains at the source point, and it is worked out from the depth of the charge.

Seismic acquisition and processing →
Traveltime curve of a reflection and the normal moveout correction
t(x)=t02+x2Vstack2,Δt(x)=t(x)−t0t(x) = \sqrt{t_0^2 + \frac{x^2}{V_\text{stack}^2}}, \qquad \Delta t(x) = t(x) - t_0

SI: s, m, m/s

Holds when: A horizontal boundary below a uniform layer. Then the formula is exact, and VstackV_\text{stack} equals the velocity of the layer. For a layered overburden, the hyperbola is an approximation at offsets that are not larger than the depth of the boundary, and VstackV_\text{stack} is close to the root-mean-square velocity (below). For a boundary that dips at an angle θ\theta in the plane of the line, Vstack=V/cos⁡θV_\text{stack} = V/\cos\theta, which is larger than the velocity of the layer.

Seismic acquisition and processing →
Root-mean-square velocity
Vrms2=∑iVi2 Δτi∑iΔτiV_\text{rms}^2 = \frac{\sum_i V_i^2\,\Delta\tau_i}{\sum_i \Delta\tau_i}

SI: m/s, s

Holds when: Horizontal, uniform layers. Offsets that are not larger than the depth of the boundary. At larger offsets the traveltime curve departs from a hyperbola, and the velocity that we pick depends on the range of offsets. Isotropic rocks. In shales the velocity depends on direction (anisotropy), and the stacking velocity usually comes out higher than the vertical velocity.

Seismic acquisition and processing →
Displacement of a reflection from a dipping boundary before migration
d=Vt02sin⁡θ,z=Vt02cos⁡θ,tan β=sin⁡θd = \frac{V t_0}{2}\sin\theta, \qquad z = \frac{V t_0}{2}\cos\theta, \qquad \mathrm{tan}\,\beta = \sin\theta

SI: m, s, m/s; angles in degrees

Holds when: A constant velocity above the boundary, and a plane boundary. The line runs in the dip direction of the boundary. On an oblique line, part of the displacement is across the line, and 2D migration will not fix it.

Seismic acquisition and processing →
Traveltime curve of a diffracted wave on a CMP section
t(x)=t02+4x2V2t(x) = \sqrt{t_0^2 + \frac{4x^2}{V^2}}

SI: s, m, m/s

Holds when: A constant velocity. A CMP section, with the source and receiver at one point. The scatterer lies in the plane of the line.

Seismic acquisition and processing →
Radius of the first Fresnel zone
rF=V2t0f≈zλ2r_\text{F} = \frac{V}{2}\sqrt{\frac{t_0}{f}} \approx \sqrt{\frac{z\lambda}{2}}

SI: m, m/s, s, Hz

Holds when: A constant (average) velocity, zero offset, a horizontal boundary, and a depth much larger than the wavelength. If the velocity grows with depth, the rays bend, and the zone is a little wider.

Seismic acquisition and processing →
The largest bin without spatial aliasing
b≤Vint4fmaxsin⁡θb \le \frac{V_\text{int}}{4 f_{max}\sin\theta}

SI: m, m/s, Hz

Holds when: A CMP section (zero offsets). The velocity above the target is constant. The estimate is made for the highest frequency that we still want to keep.

Seismic acquisition and processing →
The Dix formula
Vint2=Vn2 tn−Vn−12 tn−1tn−tn−1V_\text{int}^2 = \frac{V_n^2\,t_n - V_{n-1}^2\,t_{n-1}}{t_n - t_{n-1}}

SI: m/s, s

Holds when: Horizontal uniform layers, and the stacking velocity equals the root-mean-square velocity. Both reflections are on one vertical line, and the stacking velocities are picked without errors. In practice their errors grow many times over when they are subtracted.

Seismic interpretation →
Converting time to depth with an average velocity, and layer by layer
z=Vavg t2,z=V1t12+V2 (t−t1)2z = \frac{V_\text{avg}\,t}{2}, \qquad z = \frac{V_1 t_1}{2} + \frac{V_2\,(t - t_1)}{2}

SI: m, s, m/s

Holds when: Rays are vertical: the time is reduced to the vertical, and dips are moderate. The average velocity works while the thickness and velocity of the layers above the horizon change little sideways. The layer-by-layer method needs followed intermediate horizons and the interval velocity of each layer (from wells or by the Dix formula). For more layers the layer-by-layer formula continues as a sum (depth from two-way time).

Seismic interpretation →
Depth when velocity grows linearly with depth
z=V0k(ekt/2−1)z = \frac{V_0}{k}\left(e^{k t/2} - 1\right)

SI: m, m/s, s⁻¹, s

Holds when: Velocity grows with depth linearly (a compacting unit of uniform composition), and the instantaneous velocity does not change sideways. Vertical rays. For several units, each is described by its own V0V_0 and kk.

Seismic interpretation →

Symbols

SymbolMeaning and context
Δg\Delta g
 dA\dd A
Δg(x)\Delta g(x)
  • anomaly at a distance xx from the point above the centre of the sphere; the value in m/s² multiplied by 10510^5 gives milligals, m/s²Geophysical exploration methods
ΔT(x)\Delta T(x)
Δt(x)\Delta t(x)
aa
AA
A/A0A/A_0
bb
ΔgB\Delta g_\text{B}
BB
B0B_0
CC
dd
DSLD_\text{SL}
EE
E0E_0
ff
fmaxf_{max}
fpf_p
gg
GG
gng_\text{n}
gn(φ)g_\text{n}(\varphi)
hh
hih_i
hLVZh_\text{LVZ}
htunh_\text{tun}
kk
MM
nn
NN
NchN_\text{ch}
NRLN_\text{RL}
n(t)n(t)
ΔVp, ΔVs, Δρ\Delta V_p,\ \Delta V_s,\ \Delta\rho
QQ
RR
rFr_\text{F}
RkR_k
Δxrec\Delta x_\text{rec}
s(t)s(t)
Δxshot\Delta x_\text{shot}
tt
δgT\delta g_\text{T}
T↓, T↑T_\downarrow,\ T_\uparrow
t0t_0
t1t_1
tit_i
tn, tn−1t_n,\ t_{n-1}
tstt_\text{st}
t(x)t(x)
Δttun\Delta t_\text{tun}
VV
V0V_0
V1, V2V_1,\ V_2
VavgV_\text{avg}
  • average velocity down to the horizon: 2z/t2z/t at wells, and from a map between them, m/sSeismic interpretation
ViV_i
VintV_\text{int}
VLVZV_\text{LVZ}
Vn, Vn−1V_n,\ V_{n-1}
  • root-mean-square velocities (in practice, stacking velocities) down to the lower and the upper reflection, m/sSeismic interpretation
VpV_p
Vp, Vs, ρV_p,\ V_s,\ \rho
VrmsV_\text{rms}
VstackV_\text{stack}
w(t)w(t)
xx
x1/2x_{1/2}
  • half-width of the anomaly: the distance from the extremum (the highest or lowest value) to the point where the anomaly is half as large, mGeophysical exploration methods
zz
ZZ
Z1Z_1
Z2Z_2
z, λz,\ \lambda
β\beta
Δρ\Delta\rho
Δτi\Delta\tau_i
θ\theta
κ\kappa
λ\lambda
ρ\rho
τk\tau_k
φ\varphi