Computer Science
Scientific paper
Jun 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986thdy.work..375r&link_type=abstract
In NASA. Goddard Space Flight Center Thermosphere Dynamics Workshop, Volume 2 p 375-377 (SEE N86-29301 20-42)
Computer Science
Earth Ionosphere, Geomagnetism, Magnetic Field Configurations, Paleomagnetism, Quadrupoles, Field Strength, Magnetohydrodynamic Flow, Space Plasmas
Scientific paper
The principal features that might exist in the terrestrial paleoionosphere, if the geomagnetic field were to assume a quadrupole form during a polarity reversal are discussed. Complicated phenomena would be expected to occur at magnetic equators and magnetospherically-driven plasma convection might occur at latitudes where the magnetic field is steeply inclined. The influence of magnetic field strength on ionospheric structure is considered in general terms.
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