The Michell solution is a general solution to the elasticity equations in polar coordinates (                    r        ,        θ                        ). The solution is such that the stress components are in the form of a Fourier series in                     θ                        .
Michell showed that the general solution can be expressed in terms of an Airy stress function of the form
                                                                        φ                                                            =                                  A                                      0                                                                                     r                                      2                                                  +                                  B                                      0                                                                                     r                                      2                                                                   ln                                (                r                )                +                                  C                                      0                                                                   ln                                (                r                )                                                                                                  +                                  (                                      I                                          0                                                                                               r                                          2                                                        +                                      I                                          1                                                                                               r                                          2                                                                           ln                                    (                  r                  )                  +                                      I                                          2                                                                           ln                                    (                  r                  )                  +                                      I                                          3                                                                           )                                θ                                                                                                  +                                  (                                      A                                          1                                                                           r                  +                                      B                                          1                                                                                               r                                          −                      1                                                        +                                      B                                          1                                                                                                              ′                                                                                                 r                                     θ                  +                                      C                                          1                                                                                               r                                          3                                                        +                                      D                                          1                                                                           r                                     ln                                    (                  r                  )                  )                                cos                                θ                                                                                                  +                                  (                                      E                                          1                                                                           r                  +                                      F                                          1                                                                                               r                                          −                      1                                                        +                                      F                                          1                                                                                                              ′                                                                                                 r                                     θ                  +                                      G                                          1                                                                                               r                                          3                                                        +                                      H                                          1                                                                           r                                     ln                                    (                  r                  )                  )                                sin                                θ                                                                                                  +                                  ∑                                      n                    =                    2                                                        ∞                                                                    (                                      A                                          n                                                                                               r                                          n                                                        +                                      B                                          n                                                                                               r                                          −                      n                                                        +                                      C                                          n                                                                                               r                                          n                      +                      2                                                        +                                      D                                          n                                                                                               r                                          −                      n                      +                      2                                                        )                                cos                                (                n                θ                )                                                                                                  +                                  ∑                                      n                    =                    2                                                        ∞                                                                    (                                      E                                          n                                                                                               r                                          n                                                        +                                      F                                          n                                                                                               r                                          −                      n                                                        +                                      G                                          n                                                                                               r                                          n                      +                      2                                                        +                                      H                                          n                                                                                               r                                          −                      n                      +                      2                                                        )                                sin                                (                n                θ                )                                                            The terms                               A                      1                                   r                 cos                θ                         and                               E                      1                                   r                 sin                θ                         define a trivial null state of stress and are ignored.
The stress components can be obtained by substituting the Michell solution into the equations for stress in terms of the Airy stress function (in cylindrical coordinates). A table of stress components is shown below.
Displacements                     (                  u                      r                          ,                  u                      θ                          )                 can be obtained from the Michell solution by using the stress-strain and strain-displacement relations. A table of displacement components corresponding the terms in the Airy stress function for the Michell solution is given below. In this table
                    κ        =                              {                                                            3                  −                  4                                     ν                                                                                            f                      o                      r                                             p                      l                      a                      n                      e                                             s                      t                      r                      a                      i                      n                                                                                                                                                                                                                                                                                                                      3                            −                            ν                                                                                                                                                                                                                                                      1                            +                            ν                                                                                                                                                                                                          f                      o                      r                                             p                      l                      a                      n                      e                                             s                      t                      r                      e                      s                      s                                                                                                                              where                     ν                 is the Poisson's ratio, and                     μ                 is the shear modulus.
Note that a rigid body displacement can be superposed on the Michell solution of the form
                                                                                          u                                      r                                                                                              =                A                                 cos                                θ                +                B                                 sin                                θ                                                                                      u                                      θ                                                                                              =                −                A                                 sin                                θ                +                B                                 cos                                θ                +                C                                 r                                                            to obtain an admissible displacement field.