NivaarExam PrepOfficial exam papers ↗

18-Geol-A7 Applied Geophysics · May 2013

Question 5 of 8: Detecting a Thin Middle Layer — Three Methods, and the Equivalence Principle

Nivaar worked solution (AI-drafted; not reviewed by a licensed engineer)

Notes on this paper

National Exams — May 2013 — 04-Geol-A7 Applied Geophysics. Three-hour, open-book exam; any non-communicating calculator permitted. Part I (Questions 1–4) is compulsory; Part II states "answer any THREE of Questions 5–8," but all eight questions, and every lettered/numbered sub-part, are solved below. Two figures (the gravity profile of Q7 and the seismic time-distance graph of Q8) are read from the printed exam page; the reading tolerance is given in a check callout beside each.

Reference texts: Telford, Geldart & Sheriff, Applied Geophysics (2nd ed.) — the primary reference for every method in this paper (seismic refraction/reflection, gravity, magnetics, electrical/resistivity, EM, radiometrics); Kearey, Brooks & Hill, An Introduction to Geophysical Exploration (3rd ed.) — method-selection and field-procedure context; Blakely, Potential Theory in Gravity and Magnetic Applications — the horizontal-cylinder gravity formula and magnetic-anomaly shape analysis used in Q6–Q7.

Question 5: Detecting a Thin Middle Layer — Three Methods, and the Equivalence Principle (10 marks)

Question text not reproduced: the examination questions are © Engineers and Geoscientists BC. Open the official past paper (linked at the top of this page) to read the question, then follow the worked solution below.

Given. A 3-layer horizontal earth: layer 1 $v_1=800$ m/s, $\rho_1=100\ \Omega\cdot\text{m}$; layer 2 (the "thin" target) $v_2=1500$ m/s, $\rho_2=2\ \Omega\cdot\text{m}$; layer 3 (basement/half-space) $v_3=3000$ m/s, $\rho_3=50\ \Omega\cdot\text{m}$. Note layer 2 is both a low-velocity AND a low-resistivity layer sandwiched between higher-velocity, higher-resistivity layers — a "H-type" resistivity sequence ($\rho_1>\rho_2<\rho_3$) and a low-velocity seismic layer, which is the hardest case for every method below.

(a)(i) Vertical electrical sounding (VES). A conductive middle layer sandwiched between two more resistive layers produces an H-type sounding curve: apparent resistivity $\rho_a$ falls from $\rho_1$ toward $\rho_2$ as AB/2 increases past roughly the depth to layer 2, then rises back toward $\rho_3$ once AB/2 is large enough that current flow is dominated by the basement. As layer 2 becomes very THIN, the current has less and less "room" to be channelled through the low-resistivity layer before AB/2 also senses layer 3, so the dip toward $\rho_2$ becomes shallower and narrower and, for a sufficiently thin layer, may never reach anywhere near the true $\rho_2=2\ \Omega\cdot\text{m}$ at all — the curve can look almost like a simple 2-layer $\rho_1\to\rho_3$ curve, making the presence of layer 2 easy to miss entirely.

1101001000110100AB/2 (m) — logapparent ρₐ (Ω·m) — lognormal (h₂ = 20 m):clear mid-branch dipthin (h₂ = 2 m): dip shallows,nearly ρ₁→ρ₃ directVES sounding curve — 3-layer H-type(ρ₁=100 > ρ₂=2 ≪ ρ₃=50 Ω·m)
VES sounding curves (log-log $\rho_a$ vs. AB/2) for a normal-thickness vs. a very thin middle layer: the diagnostic H-type dip shallows and can disappear.

(a)(ii) Seismic refraction. Refraction relies on layer 2 being a DISTINCT, DETECTABLE segment on the first-arrival time-distance graph. Layer 2's velocity (1500 m/s) is higher than $v_1$'s, so it CAN refract in principle, but as an intermediate layer its refracted branch only exists over the narrow offset range between its own crossover distance (where it first becomes the fastest path) and the larger offset at which the DEEPER, faster layer-3 refraction overtakes it. As layer 2 thins, that offset window shrinks and eventually the layer-2 branch is never the first arrival at any offset — it is completely "hidden" beneath the direct-to-layer-3 refraction, called a BLIND ZONE (or hidden layer problem), and the time-distance graph simply jumps from the $v_1$ direct-wave segment almost straight to the $v_3$ refracted segment, exactly as if layer 2 did not exist.

0204060801000.000.020.040.060.080.10offset x (m)first-arrival time T (s)normal — all 3 segments seenthin h₂ — v₂ segment shrinks toa blind zone (v₁ jumps ~direct to v₃)First-arrival time-distance curve
First-arrival time-distance curves for a normal vs. a thin middle layer: the v₂ segment shrinks to a blind zone and the graph jumps almost directly from v₁ to v₃.

(a)(iii) Seismic reflection. A synthetic seismogram at any one trace location shows a reflection wavelet from the top of layer 2 (positive reflection coefficient here, since $Z_2\lt Z_1$: low velocity into the layer) and a second wavelet from its base (comparable-magnitude, opposite-sign reflection coefficient, since $Z_3\gt Z_2$), separated in two-way time by $\Delta t=2h_2/v_2$. As layer 2 thins, $\Delta t$ shrinks; once it becomes smaller than roughly one quarter of the dominant seismic wavelet's period (the classic seismic "tuning thickness"), the two wavelets can no longer be resolved as separate events — they interfere (constructively or destructively depending on the exact phase), and the pair collapses into one composite, distorted wavelet whose amplitude no longer represents either interface's true reflection coefficient. Below tuning thickness, reflection seismic can still detect that SOMETHING changed at that time but can no longer resolve layer 2's actual thickness from the waveform alone.

0102030405060two-way time (ms)normal (h₂ large)thin h₂two well-separated events — top & base of layer 2 resolvedtwo well-separated events —top & base of layer 2 resolvedevents interfere / merge —layer below tuning thicknessSynthetic seismogram — reflections fromtop & base of layer 2
Synthetic seismogram traces: for a normal-thickness layer 2 the top- and base-reflections are two separate, resolvable events; for a thin layer 2 (below tuning thickness) they interfere and merge into one composite wavelet.

(b) Why VES resistivity of the middle layer is ambiguous even when it is thick enough to detect — the principle of equivalence. For a layer bounded by higher-resistivity layers above and below (an H-type sequence, exactly the case here), a VES sounding is sensitive mainly to the layer's transverse resistance $T=\rho_2 h_2$ (current flows predominantly ALONG the conductive layer, since it is the path of least resistance), not to $\rho_2$ and $h_2$ independently. Any combination of $\rho_2$ and $h_2$ that keeps the PRODUCT $\rho_2 h_2$ (and, more precisely, the two dimensionless ratios that control the sounding curve's shape) unchanged produces a curve that is indistinguishable, within normal field noise, from the true one — so the inversion is fundamentally non-unique: a thinner, more conductive layer and a thicker, less conductive layer with the same transverse resistance both fit the data equally well. This can only be resolved with independent information (a borehole log, or a seismic/other geophysical constraint on $h_2$), which is precisely the trade-off already illustrated numerically for the gravity cylinder in Question 7(c).

MethodDifficulty as layer 2 thins
(i) VES soundingH-type dip toward ρ₂ shallows/narrows — can vanish into an apparent 2-layer curve
(ii) Seismic refractionv₂ segment shrinks to a "blind zone" — layer never becomes a first arrival
(iii) Seismic reflectionTop/base reflections interfere below tuning thickness (Δt < ~T/4) — merge into one wavelet
(b) VES resistivity ambiguityPrinciple of equivalence: only ρ₂h₂ (transverse resistance) is resolved, not ρ₂ and h₂ separately