ESS 314 · Week 6 · Lecture 11

Whole Earth Imaging

Lecture 11 · Week 6
ESS 314 Introduction to Geophysics

Marine Denolle · University of Washington

University of Washington · Denolle
ESS 314 · Week 6 · Lecture 11

By the end of this lecture, you will be able to:

  • [LO-11.1] Describe how global travel-time observations probe Earth's radial structure.
  • [LO-11.2] Read a global travel-time diagram and identify the major body-wave phases (P, S, PP, PcP, PKP, PKIKP, SKS).
  • [LO-11.3] Explain the shadow-zone reasoning behind the three canonical discoveries: fluid outer core (Oldham 1906), depth to CMB (Gutenberg 1914), and solid inner core (Lehmann 1936).

Prerequisites: Snell's law (Lec 3), ray-wavefront duality (Lec 4), forward/inverse problem framing (Module 2 intro).

University of Washington · Denolle
ESS 314 · Week 6 · Lecture 11

The motivating claim

No one has ever been more than 12.3 km below the surface.

That is roughly 1/500th of the way to the centre.

Yet seismologists report the radius of the core to within a kilometre,
the depth to the CMB to a few kilometres, and the speed of sound in the core
to three significant figures.

How?

Answer: by reading the times at which seismic waves arrive at stations around the globe.

University of Washington · Denolle
ESS 314 · Week 6 · Lecture 11

The reasoning arc for today

A seismic wave at has sampled the entire mantle.
A wave at has passed through the core twice and the inner core once.

Each travel time is a line integral of slowness along a path through the planet.

Collect enough — invert — and a 1-D Earth emerges.

University of Washington · Denolle
ESS 314 · Week 6 · Lecture 11

Physics: why rays curve

Snell's law at each infinitesimal interface bends the ray toward the slower side.
The shape of encodes the depth dependence of velocity.

University of Washington · Denolle
ESS 314 · Week 6 · Lecture 11

Both shadow zones start at 103° — for different reasons

alt:Two-panel Earth cross-section. Left: orange S-rays confined to mantle, vermilion shadow zone beyond 103 degrees. Right: blue P-rays in mantle, light-blue PKP rays arching through outer core emerging beyond 143 degrees, dashed-green PKIKP rays through inner core, vermilion P-shadow band from 103 to 143 degrees.

  • 103° is geometric — the epicentral distance at which a direct mantle ray just grazes the CMB
  • S shadow → antipode: fluid outer core, , shear cannot propagate
  • P shadow → 143°: P refracts into core ( km/s → km/s); PKP fills in beyond the caustic
University of Washington · Denolle
ESS 314 · Week 6 · Lecture 11

Discovery 1 · Oldham 1906

S-waves do not arrive at stations more than ~103° from the source.

Inference: the Earth has a fluid outer core, a zone where shear waves cannot propagate.

The reasoning required nothing more than absence-of-observation plus the physics of shear in fluids.

University of Washington · Denolle
ESS 314 · Week 6 · Lecture 11

Discovery 2 · Gutenberg 1914

A band of missing P arrivals exists between ~103° and ~143°.

Inference: a sharp velocity drop at the CMB refracts P-rays strongly.
Depth estimate: ~2900 km → within a few percent of modern PREM value (2891 km).

The reasoning required Snell's law applied at a single global interface.

University of Washington · Denolle
ESS 314 · Week 6 · Lecture 11

Discovery 3 · Lehmann 1936

Weak P-wave energy arrives inside the predicted P shadow, at ~150°–160°.

Inference: there must be a solid inner core with higher than the outer core, reflecting/refracting waves back into the shadow band.

The reasoning required reading anomalies in the P-shadow — a detail-driven result.

University of Washington · Denolle
ESS 314 · Week 6 · Lecture 11

Global travel-time curves — the AK135 inversion

Each curve is the forward prediction of a named phase. Every curve is also a teaching tool for phase identification.

University of Washington · Denolle
ESS 314 · Week 6 · Lecture 11

Phase nomenclature — the grammar

P/S = mantle K = outer core (P) I/J = inner core (P/S)
c = reflection at CMB i = reflection at ICB

University of Washington · Denolle
ESS 314 · Week 6 · Lecture 11

Worked example — CMB depth from

At (AK135):

  • min
  • min
  • s

With average mantle km/s:

→ CMB at ~2900 km. Modern value: 2891 km.

University of Washington · Denolle
ESS 314 · Week 6 · Lecture 11

The 1-D answer: PREM

Dziewonski & Anderson 1981.
Still the reference — 45 years on.
Note in the outer core.

University of Washington · Denolle
ESS 314 · Week 6 · Lecture 11

Key equation — travel time as integral of slowness

For a spherically symmetric Earth, depends only on ray parameter and the radial profile .

Inversion of many for → PREM.

University of Washington · Denolle
ESS 314 · Week 6 · Lecture 11

Cascadia anchor

Every teleseismic first arrival recorded at a PNSN station is compared to AK135.

The residual — positive or negative by a few seconds — is a direct measurement of 3-D mantle structure beneath our feet.

That residual is the data of Lecture 12.

University of Washington · Denolle
ESS 314 · Week 6 · Lecture 11

Research horizon

  • Inner-core rotation: Vidale et al. 2024 (Nature) — still debated.
  • Comparative planetology: Mars (InSight, Stähler et al. 2021), Moon (Apollo, Weber et al. 2011).
  • CMB texture: ULVZs, D″ phase transitions mapped with ScS precursors.
  • AI-assisted picking: PhaseNet/EQTransformer — 10× catalog completeness in 5 years.
University of Washington · Denolle
ESS 314 · Week 6 · Lecture 11

AI Literacy — Epistemics (LO-7)

Try this prompt: "List the seismic phases that pass through Earth's inner core and their typical travel times at ."

What to check

  1. Is each named phase valid under P/S/K/I/J/c/i?
  2. Has it been observationally confirmed? (PKJKP: contested.)
  3. Do the travel times match obspy.taup AK135 predictions?

The rule: never treat AI-generated scientific lists as primary sources. Cross-check.

University of Washington · Denolle
ESS 314 · Week 6 · Lecture 11

Concept checks

  1. If km/s everywhere, what is at ? Compare to PKIKP (~20 min). Sign of the difference?
  2. A seismogram at unknown shows P at 7 min, S at 13 min. Estimate from the curves. What phases come next?
  3. Why does the existence of PKIKP inside the P shadow require a solid inner core?
University of Washington · Denolle
ESS 314 · Week 6 · Lecture 11

Summary

  • Why: Travel times of body waves at global distances probe the deep Earth.
  • What: Three discoveries — fluid outer core, CMB depth, solid inner core — from shadow-zone reasoning alone.
  • How: Global curves inverted for the radial profile , , PREM.
  • Next: Residuals from PREM become the data for 3-D tomography. Lecture 12.
University of Washington · Denolle
ESS 314 · Week 6 · Lecture 11

Further reading

  • Kennett et al. 1995, GJI — AK135 model. (Open access.)
  • Stein & Wysession 2003, Ch. 3.3–3.5. (UW Libraries.)
  • IRIS/EarthScope Global Stacks: https://ds.iris.edu/spud/eventplot
  • Lowrie & Fichtner 2020, Ch. 3.5–3.6. (UW Libraries — primary text.)
  • obspy.taupTauPyModel(model="ak135") — reproduce every figure.
University of Washington · Denolle