Brainscape_Module1_ElasticWaves Flashcards

(63 cards)

1
Q

What is stress (σ)?

A

Stress is the intensity of force acting on a body, measured as force per unit area (N/m²). It represents the internal forces within a material in response to external loads.

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2
Q

What is strain (ε)?

A

Strain is the deformation of a body caused by stress. It is dimensionless and represents relative change in length (ΔL/L) or volume (ΔV/V). It quantifies how much a material deforms under load.

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3
Q

What is linear elasticity (Hooke’s Law)?

A

For small deformations, strain is proportional to stress: σ_ij = c_ijkl ε_kl, where c_ijkl is the elastic stiffness tensor. This is the elastic region where deformations are fully recoverable when stress is removed.

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4
Q

What does ‘fully elastic’ mean?

A

Fully elastic means deformations disappear completely when stress is removed. In seismic exploration, stress and strain are well within the elastic regime, so Hooke’s Law applies.

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5
Q

How is Young’s modulus (E) measured?

A

Young’s modulus E = σ/ε = (F/A)/(ΔL/L) is measured using a uniaxial compression/tension test. Apply force F to a rod with cross-sectional area A and measure the length change ΔL relative to original length L.

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6
Q

What is Young’s modulus?

A

Young’s modulus E is the ratio of tensile stress to tensile strain in a uniaxial test. It measures material stiffness: how much a material resists stretching or compression along one axis.

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7
Q

How is Poisson’s ratio (ν) measured?

A

Poisson’s ratio ν = -ε_r/ε_l = -(Δw/w)/(ΔL/L) is measured in the same uniaxial test as Young’s modulus. Measure both longitudinal strain (ΔL/L) and transverse strain (Δw/w) when stretching a rod.

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8
Q

What is Poisson’s ratio?

A

Poisson’s ratio ν is the ratio of fractional transverse contraction to fractional longitudinal extension. It describes how much a material contracts laterally when stretched axially. Typical values: 0.1-0.35 for rocks.

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9
Q

How is bulk modulus (k) measured?

A

Bulk modulus k = -ΔP/(ΔV/V) is measured using a hydrostatic pressure test. Apply uniform pressure ΔP and measure volume change ΔV. Alternatively, calculate from k = E/[3(1-2ν)] using Young’s modulus and Poisson’s ratio.

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10
Q

What is bulk modulus (k)?

A

Bulk modulus k is the stress-strain ratio under hydrostatic pressure, also called incompressibility. It measures resistance to uniform compression: k = -ΔP/(ΔV/V). Higher k means more incompressible.

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11
Q

How is shear modulus (μ) measured?

A

Shear modulus μ = τ/tan(θ) is measured using a shear test. Apply tangential force (shear stress τ) and measure the angle of deformation θ. Alternatively, calculate from μ = E/[2(1+ν)] using Young’s modulus and Poisson’s ratio.

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12
Q

What is shear modulus (μ)?

A

Shear modulus μ (also called rigidity) is the ratio of shear stress to shear strain. It measures resistance to shape change without volume change. Fluids have μ = 0 (cannot support shear).

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13
Q

Write the generalized Hooke’s Law

A

σ_ij = c_ijkl ε_kl, where σ_ij is stress tensor, c_ijkl is elastic stiffness tensor, ε_kl is strain tensor. Inverse form: ε_ij = s_ijkl σ_kl, where s_ijkl is elastic compliance tensor.

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14
Q

How many independent elastic coefficients for a fully anisotropic material?

A

21 independent elastic coefficients. Starting from 81 components (3×3×3×3 tensor), symmetry of stress/strain tensors reduces to 36, and energy symmetry (c_ijkl = c_klij) reduces to 21.

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15
Q

How many elastic constants for isotropic material?

A

2 independent elastic constants. Commonly: λ and μ (Lamé parameters), or k and μ (bulk and shear modulus), or E and ν (Young’s modulus and Poisson’s ratio). All other moduli can be derived from any pair.

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16
Q

How many elastic constants for Transverse Isotropic (TI) material?

A

5 independent elastic constants. TI symmetry (cylindrical symmetry about one axis) reduces the 21 constants of fully anisotropic material to 5. TI is common in layered shales.

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17
Q

Why introduce material symmetries?

A

Material symmetry reduces the number of elastic constants needed: Fully anisotropic (21) → Transverse Isotropic/TI (5) → Isotropic (2). This simplifies modeling while capturing essential physics of layered rocks like shale.

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18
Q

What is Transverse Isotropic (TI) media?

A

TI media have symmetry about one axis normal to a plane of isotropy (cylindrical symmetry). Properties are uniform in the plane but different perpendicular to it. Example: horizontally layered shale (VTI).

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19
Q

Why is TI important in seismic exploration?

A

Shale is often TI due to horizontal layering. Fractured carbonates with parallel fractures can be TI. TI is more realistic than isotropic assumptions but simpler than fully anisotropic. Affects velocity, AVO, time-depth conversion, and NMO correction.

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20
Q

What is anisotropy?

A

Anisotropy means physical properties vary with direction. In seismic: wave velocity depends on propagation direction. Causes: layering (shale), aligned fractures, stress-induced alignment. Isotropic: properties same in all directions (e.g., well-sorted sandstone).

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21
Q

What are the three main types of anisotropy?

A

1) VTI (Vertical Transverse Isotropy): horizontal layering, vertical symmetry axis (shale). 2) TTI (Tilted Transverse Isotropy): dipping layers, tilted symmetry axis. 3) HTI (Horizontal Transverse Isotropy): vertical fractures, horizontal symmetry axis.

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22
Q

What physical principles form the basis of the wave equation?

A

1) Newton’s 2nd law (F = ma), 2) Hooke’s law (σ = cε). Combining these gives the elastodynamic wave equation: ∂²u/∂t² = (c/ρ)(∂²u/∂x²) for 1D case.

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23
Q

Write the 1D wave equation

A

∂²u/∂t² = (c/ρ)(∂²u/∂x²), where u is particle displacement, t is time, c is elastic constant, ρ is density, x is position. Wave velocity V = √(c/ρ).

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24
Q

Write the P-wave velocity equation

A

V_p = √[(λ + 2μ)/ρ] = √[(k + 4μ/3)/ρ], where V_p is P-wave velocity, λ is Lamé’s first parameter, μ is shear modulus, k is bulk modulus, ρ is density.

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25
Write the S-wave velocity equation
V_s = √(μ/ρ), where V_s is S-wave velocity, μ is shear modulus, ρ is density. Note: S-wave velocity depends ONLY on shear modulus and density, not bulk modulus.
26
What are the key characteristics of P-waves?
P-waves are compressional/extensional waves. Particle motion is parallel to wave direction. They are curl-free (irrotational). They propagate through solids, liquids, and gases. Also called primary or longitudinal waves.
27
What are the key characteristics of S-waves?
S-waves are shear waves. Particle motion is perpendicular to wave direction. They are divergence-free (no volume change). They propagate ONLY through solids, NOT through fluids/gases (μ = 0 for fluids). Also called secondary or transverse waves.
28
Why don't S-waves propagate through fluids?
Fluids cannot support shear stress (μ = 0 for fluids). Since V_s = √(μ/ρ) and μ = 0, S-wave velocity V_s = 0 in fluids. This is why S-waves cannot travel through liquid outer core of Earth.
29
What is the relationship between V_p and V_s?
V_p/V_s = √[(λ + 2μ)/μ] = √[2(1-ν)/(1-2ν)], where ν is Poisson's ratio. Typical values: V_p/V_s ≈ 1.5-2.0 for consolidated rocks. For ν = 0.25: V_p/V_s ≈ 1.73. Always V_p > V_s.
30
Write Snell's Law
sin(θ₁)/V₁ = sin(θ₂)/V₂ = p, where θ₁, θ₂ are ray angles in media 1 and 2, V₁, V₂ are velocities, p is ray parameter (constant along raypath). Applies to both reflected and transmitted waves (P and S).
31
What is acoustic impedance (Z)?
Acoustic impedance Z = ρV is the product of density and wave velocity. It controls reflection/transmission at interfaces. Units: kg/(m²·s) or Rayl. Impedance contrast determines reflection strength.
32
Write the reflection coefficient equation (normal incidence)
R = (Z₂ - Z₁)/(Z₂ + Z₁), where R is reflection coefficient, Z₁ is acoustic impedance of medium 1, Z₂ is acoustic impedance of medium 2. R > 0: impedance increases (hard event). R < 0: impedance decreases (soft event).
33
Write the transmission coefficient equation (normal incidence)
T = 2Z₁/(Z₂ + Z₁), where T is transmission coefficient (for displacement amplitude), Z₁ is impedance of medium 1, Z₂ is impedance of medium 2. Note: energy is also conserved (R² + (Z₁/Z₂)T² = 1).
34
What are the Zoeppritz equations?
The Zoeppritz equations give exact reflection and transmission coefficients at an interface for P-P, P-S, S-P, and S-S waves as a function of incidence angle. They are complex, nonlinear equations. Basis for AVO analysis (amplitude variation with angle).
35
Why are Zoeppritz equations important?
Zoeppritz equations show that reflection amplitude varies with incidence angle, and this variation depends on contrasts in V_p, V_s, and ρ. This angle-dependence is the physical basis for AVO (Amplitude Versus Offset) analysis used in hydrocarbon detection.
36
What is the critical angle?
sin(θ_c) = V₁/V₂, where θ_c is critical angle, V₁ is velocity in upper medium, V₂ is velocity in lower medium (V₂ > V₁). At θ > θ_c, total reflection occurs. At θ = θ_c, refracted wave travels along interface (head wave).
37
What are head waves (refracted waves)?
Head waves are generated when the incidence angle equals the critical angle (θ = θ_c) and V₂ > V₁. The refracted wave propagates along the interface at velocity V₂, continuously radiating energy back into medium 1. Used in refraction seismology.
38
What is vertical resolution?
Vertical resolution Δz = λ/4 is the minimum layer thickness that can be distinguished. λ = V/f is wavelength, V is velocity, f is frequency. Example: V = 3000 m/s, f = 30 Hz → λ = 100 m → Δz = 25 m.
39
What is tuning?
Tuning occurs when layer thickness ≈ λ/4. Reflections from top and base of the layer interfere constructively or destructively. At tuning thickness, amplitude is maximum. Below tuning thickness, reflections cannot be separated (appear as single composite event).
40
What is horizontal resolution?
Horizontal resolution is the minimum lateral extent that can be observed. It equals the Fresnel zone radius: R_F = √(λz/2) = √(Vz/2f), where z is depth, V is velocity, f is frequency. Unmigrated data has large Fresnel zones; migration improves lateral resolution.
41
What is the Fresnel zone?
The Fresnel zone is the area on a reflector from which reflected energy arrives within half a wavelength of the first arrival. Radius: R_F = √(λz/2). All points within the Fresnel zone contribute to the recorded seismic signal. Larger Fresnel zone = poorer lateral resolution.
42
How does depth affect Fresnel zone size?
Fresnel zone radius R_F = √(Vz/2f) increases with depth z. Deeper targets → larger Fresnel zones → poorer horizontal resolution. This is why deep seismic imaging has worse lateral resolution than shallow imaging (for same frequency).
43
How does frequency affect resolution?
Higher frequency → shorter wavelength (λ = V/f) → better vertical resolution (Δz = λ/4) and horizontal resolution (R_F ∝ √λ). However, high frequencies attenuate faster (absorption), so deep reflections have lower frequency content and poorer resolution.
44
What is absorption/attenuation?
Absorption is the loss of seismic energy due to internal friction (conversion to heat) as waves propagate. Higher frequencies attenuate more than lower frequencies. Result: deep reflections have reduced frequency content and poorer resolution. Quantified by Q-factor.
45
What is the Q-factor?
Q-factor (quality factor) describes energy loss per cycle: Q = 2π × (stored energy)/(energy lost per cycle). Higher Q = lower attenuation. Typical rocks: Q = 20-100. Low Q means strong attenuation. High frequencies are more affected by attenuation.
46
What factors affect seismic resolution?
1) Frequency: higher f → better resolution but more attenuation. 2) Depth: deeper → larger Fresnel zone, more attenuation. 3) Velocity: affects wavelength λ = V/f. 4) Absorption (Q-factor): reduces high frequencies. 5) Migration: improves lateral resolution by collapsing Fresnel zone.
47
What is wavelength (λ)?
Wavelength λ = V/f is the spatial distance between successive wave peaks (or troughs), where V is wave velocity and f is frequency. Controls resolution: shorter λ → better resolution. Typical seismic: f = 30 Hz, V = 3000 m/s → λ = 100 m.
48
What are surface waves?
Surface waves propagate along a free surface (e.g., Earth's surface). Two main types: Rayleigh waves (elliptical retrograde particle motion) and Love waves (horizontal transverse motion). They decay exponentially with depth. Slower than body waves (P and S). Often coherent noise in seismic data.
49
What are Rayleigh waves?
Rayleigh waves are surface waves with elliptical retrograde particle motion (both vertical and horizontal components). Velocity: V_R ≈ 0.9V_S. Amplitude decays exponentially with depth. Dominant surface wave on free surface. Ground roll in seismic data is often Rayleigh waves.
50
What are Love waves?
Love waves are surface waves with horizontal transverse motion (perpendicular to propagation direction, parallel to surface). They require layering (faster layer over slower layer). Velocity: V_S1 < V_Love < V_S2. Amplitude decays with depth. No vertical motion.
51
Why are surface waves considered noise in seismic exploration?
Surface waves (ground roll) are coherent noise because they: 1) Have high amplitude, 2) Are slow (low velocity), 3) Have low frequency, 4) Obscure reflected body waves (P and S). Removed using frequency-wavenumber (f-k) filtering or velocity filtering.
52
What is dispersion?
Dispersion occurs when wave velocity depends on frequency. Different frequency components travel at different speeds, causing wavelet shape to change with distance. Surface waves are dispersive (velocity depends on frequency). Body waves (P, S) in elastic media are non-dispersive.
53
What is geometric spreading?
Geometric spreading is the decrease in amplitude as wavefront expands spherically from a point source. Amplitude decreases as 1/r for 3D spreading (spherical wavefront) or 1/√r for 2D spreading (cylindrical wavefront), where r is distance. Causes amplitude loss but not frequency change.
54
What is the difference between absorption and geometric spreading?
Geometric spreading: amplitude loss due to wavefront expansion (1/r decay), frequency-independent, energy conserved. Absorption: amplitude loss due to internal friction (converted to heat), frequency-dependent (high frequencies attenuate more), energy lost. Both cause amplitude decrease with distance.
55
What is mode conversion?
Mode conversion occurs when a wave encounters an interface at oblique incidence. A P-wave can generate both reflected/transmitted P-waves AND converted S-waves (and vice versa). Governed by Zoeppritz equations. Important for multi-component seismic and PS-wave imaging.
56
What is the ray parameter (p)?
Ray parameter p = sin(θ)/V is constant along an entire raypath (Snell's law). It characterizes the ray geometry. Horizontal slowness: p = dt/dx. Units: s/m. Useful for ray tracing and moveout calculations.
57
What is the difference between phase velocity and group velocity?
Phase velocity: velocity of individual wave crests (V_phase = ω/k). Group velocity: velocity of wave packet (energy transport): V_group = dω/dk. In non-dispersive media: V_phase = V_group. In dispersive media (e.g., surface waves): V_phase ≠ V_group.
58
What is particle velocity vs wave velocity?
Particle velocity: velocity of individual particles oscillating as wave passes (typically mm/s to cm/s in seismics). Wave velocity: velocity of wavefront propagation through medium (km/s). Particle velocity << wave velocity. Particle displacement amplitude is typically μm to mm.
59
What is a plane wave?
A plane wave has constant phase on infinite parallel planes perpendicular to propagation direction. Mathematical form: u = A exp[i(k·x - ωt)], where k is wavevector, ω is angular frequency. Approximation valid far from source (far-field). Used in theoretical analysis (Zoeppritz, AVO).
60
What is a spherical wave?
A spherical wave expands radially from a point source with amplitude decreasing as 1/r. Mathematical form: u = (A/r) exp[i(kr - ωt)]. Realistic near-field representation of seismic sources. At large distances, locally approximates plane wave.
61
What are Lamé parameters (λ, μ)?
Lamé parameters λ and μ are elastic constants for isotropic materials. μ is shear modulus (rigidity). λ is related to compressibility: k = λ + 2μ/3. P-wave velocity: V_p = √[(λ+2μ)/ρ]. S-wave velocity: V_s = √(μ/ρ). Any two elastic moduli determine all others for isotropic media.
62
What is the period (T) of a wave?
Period T = 1/f is the time for one complete wave cycle. Units: seconds. Related to wavelength by λ = VT, where V is wave velocity. Example: f = 30 Hz → T = 0.033 s (33 ms). Period is the temporal equivalent of wavelength (spatial). Lower frequency → longer period → longer wavelength.
63
What are diffracted waves?
Diffracted waves occur when waves encounter edges, corners, fault planes, or small objects (size comparable to wavelength). Energy bends around obstacles following Huygens' principle. Characteristics: 1) Hyperbolic moveout in seismic data, 2) Diagnostic for discontinuities (faults, pinchouts), 3) Important for imaging steep flanks and salt bodies. Migration collapses diffraction hyperbolae to their true spatial position. Used in diffraction imaging for subsalt and fault detection.