The magnetic field measured by a magnetometer on the Earth's surface has basic two parts:
The constant main field caused by internal currents in the Earth and the variable
external field dominated by currents in the
ionosphere. Based upon this model magnetometer analysis can be reduced to three basic steps:
 Remove the background magnetic field. To do this, find a day close to the interval
of interest when the magnetic field is very steady. This is known as the quiettime field. Subtract
the quiettime field from the magnetic field measured on the day of interest to yield the external
magnetic perturbations caused by ionospheric currents.
Note that the quiet time field comprises not only the constant main field but also the external field due
to everpresent ionospheric current, ring current, and
magnetopause current. We assume that the ionospheric currents of interest
(i.e., those driven by processes out in Space) are inherently timevarying.
 Calculate the equivalent current. Take the horizontal magnetic field perturbation
vector and rotate 90^{o} clockwise to yield the equivalent ionospheric current.
 Examine the vertical component. If d_{Z} = 0 then the current is overhead or spatially uniform.
If d_{Z} does not equal 0 then use the line current model to infer where the current is concentrated relative
to the magnetometer.
