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A numerical study of nighttime ionospheric variations in the American sector during 28–29 October 2003
Author(s) -
Chen Xuetao,
Lei Jiuhou,
Wang Wenbin,
Burns Alan G.,
Luan Xiaoli,
Dou Xiankang
Publication year - 2016
Publication title -
journal of geophysical research: space physics
Language(s) - English
Resource type - Journals
eISSN - 2169-9402
pISSN - 2169-9380
DOI - 10.1002/2016ja023091
Subject(s) - ionosphere , thermosphere , storm , atmospheric sciences , low latitude , northern hemisphere , geomagnetic storm , latitude , f region , geology , southern hemisphere , climatology , geophysics , physics , plasma , geodesy , solar wind , oceanography , quantum mechanics
Variations of nighttime F 2 peak height ( h m F 2 ) over the American sector during the 28–29 October 2003 storm period were investigated using the National Center for Atmospheric Research Thermosphere‐Ionosphere Electrodynamics Global Circulation Model. 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. These PPEFs greatly affect the low‐latitude ionosphere during storm time. On 28 October, even though the B z disturbance was weak with a short duration of southward B z , the TADs from the Southern Hemisphere can propagate to the Northern Hemisphere and result in the corresponding oscillations in the nightside h m F 2 .