A numerical study of nighttime ionospheric variations in the American sector during 28-29 October 2003

The model was generally able to reproduce the ionospheric variations on 28-29 October 2003 observed by the ionosondes. A series of controlled model simulations were subsequently undertaken to examine the effects of electric fields and neutral winds on the ionosphere.

The numerical experiments suggest that the dramatic nighttime increase of h(m)F(2) on the storm day 29 October is mainly caused by traveling atmospheric disturbances (TADs) from the high latitudes of the Northern Hemisphere. However, the electric field plays an important role in causing the elevation of h(m)F(2) in the equatorial region. The prompt penetration electric field (PPEF) associated with the southward component of the interplanetary magnetic field (B-z) is westward on the nightside, whereas when B-z reverses and becomes northward, the PPEF is westward in the premidnight and turns to eastward in the postmidnight.