The magnetic storm main phase modelling

Details The magnetic storm main phase modelling The magnetic storm main phase modelling

May 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989p%26ss...37..525w&link_type=abstract

Planetary and Space Science (ISSN 0032-0633), vol. 37, May 1989, p. 525-534.

Physics

10

Energy Distribution, Equatorial Atmosphere, Ionospheric Ion Density, Magnetic Storms, Ring Currents, Geomagnetism, Hydrogen Ions, Oxygen Ions

Scientific paper

Equatorial distributions of energy, current, and magnetic field disturbances, along with equatorial ion distributions, have been determined by solving the initial value problem for an ion drifting in a dipole magnetic field and convection electric field. Results are presented for hydrogen and oxygen ions. It is found that these two ring current carriers differ significantly in the growth time, amplitude, and sign of the disturbance created.

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