This is the trace of the strain tensor. In general the trace of the strain tensor gives area change in 2-D and volume change in 3-D The principal axes.

Slides:



Advertisements
Similar presentations
Mohr Circle for stress In 2D space (e.g., on the s1s2 , s1s3, or s2s3 plane), the normal stress (sn) and the shear stress (ss), could be given by equations.
Advertisements

Stress and Deformation: Part I (D&R, ; ) The goal for today is to explore the stress conditions under which rocks fail (e.g., fracture),
Anderson’s theory of faulting
Kinetics (I) Review of Kinetics of Planar Mechanisms
Chapter Outline Shigley’s Mechanical Engineering Design.
Lecture 7 Mechanical Properties of Rocks §Rock properties: mass density, porosity, and permeability §Stress §Mohr's circle §Strain §Elasticity of rocks.
III. Strain and Stress Basics of continuum mechanics, Strain Basics of continuum mechanics, Stress Reading Suppe, Chapter 3 Twiss&Moores, chapter 15 Additional.
Chapter 3 Rock Mechanics Stress
Geology 3120 Powerpoint notes available online at:
Stress: Force per unit area across an arbitrary plane.
Principle and Maximum Shearing Stresses ( )
The stresses that cause deformation
Analysis of Stress and Strain
Mechanics of Materials – MAE 243 (Section 002) Spring 2008 Dr. Konstantinos A. Sierros.
Analysis of Stress and Strain Review: - Axially loaded Bar - Torsional shaft Questions: (1) Is there any general method to determine stresses on any arbitrary.
Announcements This week's lab: 1-3 PM with Andrew McCarthy. Please come prepared with specific questions. There will be no lecture this Wednesday! Please.
1 MAE 5130: VISCOUS FLOWS Momentum Equation: The Navier-Stokes Equations, Part 1 September 7, 2010 Mechanical and Aerospace Engineering Department Florida.
Announcements Next week lab: 1-3 PM Mon. and Tues. with Andrew McCarthy. Please start on lab before class and come prepared with specific questions Cottonwood.
Joints and Shear Fractures
Forces Acting on a Control Volume Body forces: Act through the entire body of the control volume: gravity, electric, and magnetic forces. Surface forces:
Stress, Strain, and Viscosity San Andreas Fault Palmdale.
The Mechanics of the crust
16 July 2015GLG510 Advanced Structural Geology Force, Traction, and Stress.
Stress II Cauchy formula Consider a small cubic element of rock extracted from the earth, and imagine a plane boundary with an outward normal, n, and an.
IV. Basics of continuum mechanics, Stress Reading Suppe, Chapter 3 Twiss&Moores, chapter 15 Additional References : Jean Salençon, Handbook of continuum.
Theories of Stress and Strain
CHAPTER 4 DEFORMATION AND STRAIN. Deformation describes the complete transformation from the initial to the final geometry (shape, position and orientation)
Content Stress Transformation A Mini Quiz Strain Transformation
STRAIN RATE, ROTATION RATE AND ISOTROPY
Stress II. Stress as a Vector - Traction Force has variable magnitudes in different directions (i.e., it’s a vector) Area has constant magnitude with.
Transformations of Stress and Strain
APPLICATIONS/ MOHR’S CIRCLE
Force and Stress Earth Structure (2 nd Edition), 2004 W.W. Norton & Co, New York Slide show by Ben van der Pluijm © WW Norton, unless noted otherwise.
Integrating geologic maps with fault mechanics John Singleton, George Mason University NSF Cutting Edge Workshop 2012.
FLUID STATICS HYDROSTATIC FORCES AND BUOYANCY
This week: PS #1 assigned (due next Tuesday) Lab #1 due tomorrow at 11:00 Lectures: ch. 3- Force and Stress Lab #2: Field trip to Mt Baldy- Will collect.
If A and B are on the same side of the origin (i. e
Lecture 7 Mechanical Properties of Rocks
1 Principal stresses/Invariants. 2 In many real situations, some of the components of the stress tensor (Eqn. 4-1) are zero. E.g., Tensile test For most.
Introduction to Seismology
Elasticity I Ali K. Abdel-Fattah. Elasticity In physics, elasticity is a physical property of materials which return to their original shape after they.
EXPLORATION GEOPHYSICS THE EXPLORATION TASK PLAN EXPLORATION APPROACH FOR A MATURE TREND GATHER DATA FOR A MATURE TREND DEVELOP PLAY PROSPECT FRAMEWORK.
Chapter 3 Force and Stress. In geology, the force and stress have very specific meaning. Force (F): the mass times acceleration (ma) (Newton’s second.
NB: Uniaxial strain is a type a non-rotational transformation Uniaxial strain.
CHAPTER OBJECTIVES To show how to transform the stress components that are associated with a particular coordinate system into components associated with.
BFC (Mechanics of Materials) Chapter 1: Stress & Strain Shahrul Niza Mokhatar
Geology Failure Models
The stresses that cause deformation
Outline Force, vectors Units Normal, shear components Pressure
Strain I. Recall: Pressure and Volume Change The 3D stresses are equal in magnitude in all directions (as radii of a sphere) The magnitude is equal to.
ME16A: CHAPTER FOUR ANALYSIS OF STRESSES IN TWO DIMENSIONS.
1 Structural Geology Force and Stress - Mohr Diagrams, Mean and Deviatoric Stress, and the Stress Tensor Lecture 6 – Spring 2016.
1 Structural Geology Deformation and Strain – Mohr Circle for Strain, Special Strain States, and Representation of Strain – Lecture 8 – Spring 2016.
Structural Geology Deformation and Strain – Homogeneous Strain, Strain Ellipsoid, Strain Path, Coaxial and Noncoaxial Strain Lecture 7 – Spring 2016 Deformation.
Force and Stress – Normal and Shear Stress Lecture 5 – Spring 2016
Mohr-Coulomb failure Goal: To understand relationship between stress, brittle failure, and frictional faulting and to use this relationship to predict.
Objectives  Introduce the concept of pressure;  Prove it has a unique value at any particular elevation;  Show how it varies with depth according.
6. Strain Assoc.Prof.Dr. Ahmet Zafer Şenalp Mechanical Engineering Department Gebze Technical University.
Transformation methods - Examples
Two-Dimensional Rotational Dynamics 8.01 W09D2
EAG 345 – GEOTECHNICAL ANALYSIS
Chapter 15 (1) Slope Stability
Mohr Circle In 2D space (e.g., on the s1s2 , s1s3, or s2s3 plane), the normal stress (sn) and the shear stress (ss), could be given by equations (1) and.
Stress = Force/Area Force is measured in units of mass*acceleration 1 N (Newton) = 1 kg * m * s-2 another common unit for force is the pound.
BDA30303 Solid Mechanics II.
Chapter 3 Force and Stress
In-class problem For maximum and minimum stresses of 600 and 200 mega-pascals (MPa) oriented as a vertical vector and a horizontal, E-W striking vector.
Review from LAB #3.
The Traction Vector and Stress Tensor
Presentation transcript:

This is the trace of the strain tensor. In general the trace of the strain tensor gives area change in 2-D and volume change in 3-D The principal axes are directions along which the starting vector and ending vector are parallel Pure shear = principal axes do not rotate with time

Principal Axes = maximum stretch direction Intermediate stretch direction Minimum stretch direction (or most contractional) The principal axes are all mutually orthogonal to one another

(10,0)becomes (11,1) (10,-10) remains fixed, as does (-10, 10) (0, 10) becomes (1,11) (10,10) becomes (12,12) etc...

In principal axis coordinate system this tensor can be written:

Simple Shear In Simple shear the principal axes rotate with increasing shear Simple shear applies only to finite strain

Marker This part of marker not disformed Rotational strain

Stress = Force/Area Force is measured in units of mass*acceleration 1 N (Newton) = 1kg * m * s -2 another common unit for force is the pound

Pressure is a number. It corresponds to a special kind of stress. Stress is a tensor, but it has the same units as pressure (Pa) 1000 Pa = 1 kPa 1,000,000 Pa = 1 MPa (about 10 bars)

Traction is a Vector Tractions are vectors = force/area Traction can be resolved into two components Normal component to plane = normal stress Tangential component = shear stress

The stress tensor The stress tensor is symmetric The stress tensor has 3 principal axes The principal axes are mutually orthogonal principal axis = direction in which the traction vector is parallel to normal to plane => no shear stress resolved on that plane

= maximum compressive principal stress = intermediate compressive principal stress = minimum compressive principal stress

Normal Stress and Shear Stress = Normal Stress resolved on plane = shear stress resolved on plane

Anderson Faulting Theory If  1 is vertical then a new fault will be a normal fault (extensional) If  1 is horizontal and  3 is vertical then reverse (thrust) fault (contractional faulting) If  1 and  3 are both horizontal then strike- slip (transcurrent) fault

Fault Angles and Principal Stresses  2 in the plane of the fault  1 20°-40° from the plane of the fault  3 50°-70° from the plane of the fault

 n = (  1 +  3 )/2 - [(  1 -  3 )/2] cos 2   = [(  1 -  3 )/2] sin 2  THESE ARE ALSO THE EQUATIONS FOR A CIRCLE WITH A RADIUS OF (  1 -  3 )/2 AND A CENTER (  1 +  3 )/2 TO THE RIGHT OF WHERE THE AXES CROSS!!!!

Let’s Look at internal friction angles, coefficients of friction, and theta If  =10° (so  =tan  =0.18), then 2  =80°, so  =40° and  1 axis is 40° from the fault plane. If  =20° (so  =tan  =0.36), then 2  =70°, so  =35° and  1 axis is 35° from the fault plane.

If  =30° (so  =tan  =0.58), then 2  =60°, so  =30° and  1 axis is 30° from the fault plane. If  =40° (so  =tan  =0.84), then 2  =50°, so  =25° and  1 axis is 25° from the fault plane.

Cohesion Cohesion = shear strength that remains even when normal tractions are zero Byerlee’s law with cohesion The cohesion represents the intercept value

Pre-existing faults If there are pre-existing faults, then figure in previous slide predicts a range of orientations of faults, with respect to maximum principal stress direction that can slip If there are no pre-existing faults, then only one orientation is possible

Role of Fluid Pressure or Pore Pressure Hydrostatic Pressure: P hydrostatic =  water g z Lithostatic pressure is when entire weight of the overlying rock (density  rock ) is being supported P lithostatic =  rock g z

Fluid Pressures and Tractions Fluid Pressures can support normal tractions but not shear tractions! Elevated fluid pressures make the Mohr circle move to the left

Effective Stress Effective Stress = total stress minus the fluid Pressure  1 ' =  1 - P f  2 ' =  2 - P f  3 ' =  3 - P f Shear Tractions are not affected!

Joints The