
NSSDC ID: SPMS-00740
Availability: At NSSDC, Ready for Offline Distribution (or Staging if Digital)
This is an analytical model of the Earth's magnetic field valid from the dayside subsolar magnetosphere to beyond lunar orbit in the nightside magnetotail. Only the quiet time magnetosphere is represented including the contributions from magnetopause, tail, and ring currents. The internal (core) field is represented by a fixed dipole. The field representation is given in Cartesian GMS coordinates using sixth-order expansions of power series and exponential terms. The 180 coefficients were determined by fitting to over 600 magnetometer measurements from OGO 3 and 5. Shortcomings of this model are the restriction to quiet conditions and the fact that the direction of the main dipole and the ring current is fixed (i.e., perpendicular to the Earth-Sun direction).
Questions or comments about this data collection can be directed to: Dr. Dieter K. Bilitza.
Olson, W. P., and K. A. Pfitzer, Quantitative model of the magnetospheric magnetic field, J. Geophys. Res., 79, No. 25, 3739-3748, Sept. 1974.
Olson, W. P., Quantative modeling of magnetospheric processes, Quantitative Modeling of Magnetospheric Processes, Geophys. Mono. 21, W.P. Olson, Amer. Geophys. Union, Wash., DC, 1979.