Module 00 · Recap and bridge
This set assumes the seismic resolution modules, where impedance, the reflection coefficient, the wavelet and tuning are built from scratch. This module restates those four results in one place, names the assumption every one of them shared, and shows the measurement that assumption was hiding. It introduces nothing new about rocks. It is here so that module 01 can start from a specific question rather than from the beginning.
The interface, and the trace it makes at normal incidence — the chain from the resolution modules
Six controls — the first four drive steps 1 and 2
Three short steps. Nothing here needs a rock property that the resolution modules did not already use, until the last panel.
The resolution modules built a chain from a column of rock to a seismic wiggle. Four of its results are used constantly from here on, and they are restated below so that the settings used later have a starting point.
Impedance is velocity times density. One number per layer, and at normal incidence it is the only rock property a reflection responds to.
A reflection measures a contrast. The reflection coefficient is the difference in impedance across the boundary divided by the sum. Equal impedances give no reflection, whatever else is different about the two rocks.
The sign is the polarity. Going into a higher impedance gives one sign, into a lower impedance the other, and which one appears as a peak on a display is a convention rather than a fact about the rock.
The trace is a sum. Each boundary returns a copy of the wavelet, and what is interpreted is the total. When two boundaries are close together their wavelets overlap and the amplitude that gets measured belongs to neither of them alone.
1 Velocity × density, for both rocks and the contrast between them
2 The reflection, with the wavelet applied at normal incidence
Every trace in the resolution modules was built for a wave arriving perpendicular to the boundary. That case has a name: normal incidence. It is the simplest one, the arithmetic is a single fraction, and it is where the impedance result comes from.
A real survey does not record that case, or rather it records it only once. A source is fired at one point and a line of receivers stretches away from it, so most of the energy that returns took a slanted path down and a slanted path back. The angle at which the wave meets the boundary is the incidence angle, and across a single recording it takes a range of values rather than one.
The resolution modules state this exclusion rather than hide it. Their trace module says it is normal incidence only, with no offset, no AVO and no mode conversion. The wedge module lists offset among the things left out because each deserves separate treatment. This set is that separate treatment.
The two controls under where the angle comes from set the distance between the source and the receiver, which is called the offset, and the depth of the boundary. For a ray that travels in a straight line and reflects at the midpoint, the half-offset and the depth are the two short sides of a right triangle, so the angle is the arctangent of one divided by the other. Offset and angle are related but not the same number: the same offset gives a wide angle at a shallow boundary and a narrow one at a deep boundary.
One shot does not produce one ray. The source releases energy as a wave that spreads outward in all directions at once, so it meets the boundary everywhere beneath the spread, not at a single point. A line of receivers — geophones on land, often called nodes when each one records independently — is laid out along the ground, and each of them picks up energy that reflected at its own point and arrived at its own angle. The third panel draws the whole spread at once. One shot into that line yields a set of recordings covering a range of angles, and every one of them is a measurement of the same boundary.
How those recordings are organized, and what happens once velocity increases with depth and the rays stop traveling in straight lines, is the subject of module 04. What matters here is that the range of angles exists and that the resolution modules covered one end of it.
1 The case that has been covered zero offset, straight down and back
2 The offset you set drawn to the same scale
3 One shot, one line of receivers the wave spreads, and every node records a different angle
Once the angle is allowed to vary, the reflection coefficient varies with it. The left-hand panel shows that for two rocks: a shale over a sand filled with brine, and the same shale over the same sand filled with gas. Both curves are computed from the full reflection equations rather than from the impedance fraction.
The picture has two separate features. The curves start at different heights, which is the impedance contrast from step 1 and is already familiar. They also have different shapes, and that is new: the gas curve falls away from its starting value much faster than the brine curve does.
The right-hand panel plots the gap between the two curves. It widens with angle. A measurement made only at normal incidence sees the difference at the left-hand edge of that plot; a measurement that uses the whole range sees the difference grow. That is the observation the rest of this set examines.
A wave arriving perpendicular to a boundary moves the rock particles straight into it and straight back out. The rock is compressed and nothing slides, so the reflection depends only on resistance to compression, which impedance describes completely. A wave arriving at an angle moves the particles along a direction that is no longer perpendicular, so part of the motion is parallel to the boundary and the rock either side is also sheared. Resistance to shearing is a separate property with its own velocity — the shear velocity, Vs, alongside the Vp the earlier modules used. The wider the angle, the more of the motion is parallel and the more Vs matters, which is why one number becomes a curve.
The third panel shows what swapping the pore fluid does to each property of the sand, and the pattern in it is the reason the two curves have different shapes: Vp drops a long way, Vs barely moves, and Vp/Vs falls further than either. Where Vp and Vs come from, and why a fluid acts on one and not the other, is module 01.
1 Reflection coefficient against angle the same sand, two pore fluids
2 The gap between the two curves how much the fluid changes the reflection
3 What the fluid changes, property by property the same sand with brine, then with gas
Two measurements instead of one. A normal-incidence amplitude is a single number, and a single number cannot separate two unknowns. The variation with angle supplies a second number from the same recording, which is the basis of everything this set covers.
Fluid discrimination. The main practical use is distinguishing a sand filled with gas from the same sand filled with brine. The panels in step 3 show why that is possible in principle. How reliable it is in practice is what modules 05 through 08 examine.
What stacking costs. The image most interpreters work from is a stack, which averages the angle range into one trace. It is a cleaner picture and it discards the variation shown here. Both statements are true at once, and module 04 covers the trade.
The resolution limits still apply. Nothing in this set repeals tuning. An amplitude measured on a bed thinner than the resolution limit belongs to two merged reflections, and that is as true at 30° as at 0°.
Each answer is a number read off this page at the settings described.
Steps 1 and 2 use the four sliders directly. Impedance is velocity times density, the reflection coefficient is the impedance difference over the sum, and the trace places a 30 Hz Ricker wavelet at the reflection. Nothing there needs a shear velocity, which is why the sliders do not carry one.
Step 3 does not use the sliders, apart from porosity. Its two rocks are a shale from Castagna's mudrock line and a sand built from a Hertz-Mindlin dry frame with the pore fluid inserted by Gassmann's relation, at 23 MPa and 64 °C, with brine and then with gas. The curves are the exact Zoeppritz P-wave reflection coefficients for those two rock pairs. Using the slider values there instead would require inventing a shear velocity for them, and the usual way of doing that is a shale trend that does not apply to sands.
Deferred rather than simplified:
The porosity slider stops at 18%. The dry frame here is a soft-sand Hertz-Mindlin model, which describes a grain pack held together by contact stiffness and is not intended for well-cemented rock. Run below roughly 18% and it keeps returning numbers, but they describe a grain pack that no longer resembles the tight sand being asked about, and the difference between the two fluid cases at wide angle stops behaving monotonically for that reason rather than a physical one. A cemented-sand or constant-cement model would be the appropriate choice there.
The angle reaches 45° at the extremes of the sliders, at the shortest depth with the longest offset. On a marine gather at reservoir depth, 30° to 40° is a more usual practical limit: beyond that the reflection coefficient changes rapidly, the linear approximations most people use stop holding, and the processing that flattened the gather is less reliable. The curves here are exact Zoeppritz, so they remain correct across the whole range even where an approximation would not.
The shear velocities used in step 3 come out of the rock model rather than from a Vp-to-Vs trend. The shale takes its Vs from Castagna's mudrock line, which is a fit to shales. The sand takes its Vs from the shear modulus of the dry grain frame, which Gassmann's relation leaves unchanged when the pore fluid is swapped — the small rise in Vs from brine to gas is entirely the density drop, not a change in the frame.
Next up
Step 3 needed a property that impedance does not carry. Module 01 builds it: grains and pore space, where a rock's density comes from, and the two separate ways a rock resists being deformed.
Go to module 01 →