Effect of zonal E × B plasma drift on electron density in the low-latitude ionospheric F region at a solar activity maximum near vernal equinox

Details Effect of zonal E × B plasma drift on electron density in the low-latitude ionospheric F region at a solar activity maximum near vernal equinox Effect of zonal E × B plasma drift on electron density in the low-latitude ionospheric F region at a solar activity maximum near vernal equinox

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ge%26ae..47..621p&link_type=abstract

Geomagnetism and Aeronomy, Volume 47, Issue 5, pp.621-635

Computer Science

Sound

2

94.20.Ii, 94.20.Vv, Ionospheric Disturbances, Irregularities, And Storms

Scientific paper

The variations in the density of the ionospheric F2 layer maximum ( NmF2) under the action of the zonal plasma drift perpendicularly to the magnetic ( B) and electric ( E) fields in the direction geomagnetic west-geomagnetic east have been studied using the three-dimensional nonstationary theoretical model of electron and ion densities ( N e and N i ) and temperatures ( T e and T i ) in the low-latitude and midlatitude ionospheric F region and plasmasphere. The method of numerical calculations of N e , N i , T e , and T i , including the advantages of the Lagrangian and Eulerian methods, is used in the model. A dipole approximation of the geomagnetic field ( B), taking into account the non-coincidence of the geographic and geomagnetic poles and differences between the positions of the Earth’s and geomagnetic dipole centers, is accepted in the calculations. The calculated NmF2 and altitudes of the F2 layer maximum ( hmF2) have been compared with these quantities measured at 16 low-latitude ionospheric sounding stations during the geomagnetically quiet period October 11-12, 1958. This comparison made it possible to correct the input model parameters: the NRLMSISE-00 model [O], the meridional component of the neutral wind velocity according to the HWW90 model, and the meridional component of the equatorial plasma drift due to the electric field specified by the empirical model. It has been indicated that the effect of the zonal E × B plasma drift on NmF2 can be neglected under daytime conditions and changes in NmF2 and hmF2 under the action of this drift are insignificant under nighttime conditions north of 25° and south of -26° geomagnetic latitude. The effect of the zonal E × B plasma drift on NmF2 and hmF2 is most substantial in the nightside ionosphere approximately from -20° to 20° geomagnetic latitude, and the neglect of this drift results in an up to 2.4-fold underestimation of NmF2. The found dependence of the effect of the zonal E × B plasma drift on NmF2 and hmF2 on geomagnetic latitude is related to the longitudinal asymmetry of B, asymmetry of the neutral wind about the geomagnetic equator, and changes in the meridional E × B plasma drift at a change in geomagnetic longitude.

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