For axial symmetry, in this study we report on analytical solutions of
the magnetohydrodynamics (MHD) equilibrium of a plasma within the mag
netic environment of a point dipole. Inside the plasma domain, the mag
netic flux function is calculated for a given shape of the pressure pr
ofile. Another magnetic flux function is derived outside the plasma do
main, where the pressure vanishes. Both functions and their normal der
ivatives are continuous through the boundary between the two domains;
together they constitute the solution of our problem. A pressure profi
le that is a quadratic function of the magnetic flux function is used.
It leads to an exact solution which is a simple function of the spher
ical coordinates. It is shown that, in this situation, the plasma ener
gy is distributed over the entire plasma domain. This solution is well
suited as a magnetospheric model. The magnetic flux function determin
ed outside the plasma domain is expressed by a very general formula th
at is valid for wide classes of both the pressure profiles and the sha
pe of a plasma exterior boundary. Far away from this boundary, as near
the coordinate center, the magnetic field tends to be dipolar. (C) 19
98 American Institute of Physics. [S1070-664X(98)02808-0].