Geodynamics - Mohr's Circle for Strain

Lecture Notes 9 Mohr’s Circle for Strain Lecture 5 explained a simple and convenient way to find the stress on an arbitrary plane given the stress tensor σij. The technique involved writing equations for how the shear stress and normal stress on the xˆ1 plane vary when the coordinate system is rotated to xˆ i ' . These equations plotted as Mohr’s circle in stress space (σ,τ) and gave the tractions on plane x1' at angle θ to the most compressive principle stress. Since strain is a second-order tensor like stress, the same technique can be applied. Equations for the normal strain and shear strain on a plane at angle θ to the most compressive principle strain may be derived in the same way the equations for stress were derived. Consider the following transformation of coordinates: x2 x2' x1' � x1 Figure 9.1 The strain tensor ε in the xˆ i coordinate system is transformed to the strain tensor ε’in the xˆ i ' coordinate system by the equation ε ' = α εα T where the double underbars denote second-rank tensors, α represents the transformation matrix, and the superscript T denotes the transpose of matrix α. See Lecture 5 for the derivation of this equation. Since the coordinate system is rotated about the x̂3 axis, the transformation matrix is ⎡ cos θ ⎢ α = ⎢− sin θ ⎣⎢ 0 sin θ cos θ 0 0⎤ 0⎥⎥ 1⎥⎦ The equations for the normal strain and shear strain on the x1 ' plane in the new coordinate system are ε 11 ' = ε 11 + ε 22 ε 11 − ε 22 cos 2θ + ε 12 sin 2θ 2 2 ε +ε ε −ε ε 22 ' = 11 22 + 11 22 cos 2θ − ε 12 sin 2θ 2 2 − (ε 11 − ε 22 ) ε 12 ' = sin 2θ + ε 12 cos 2θ 2 + The derivation for these equations follows the derivation for the Mohr’s circle equations of stress in Lecture 5.