@InProceedings{Balan:2016:ReDeUn,
author = "Balan, Nalan",
affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)}",
title = "Recent developments in the understanding of the mechanisms of EIA
under quiet and active conditions",
year = "2016",
organization = "Annual Meeting Asia Oceania Geosciences Society, 13. (AOGS)",
abstract = "The equatorial ionization anomaly (EIA), the largest ionospheric
feature that covers over half the global area in 24 hours, was
discovered by Namba and Maida in 1939 and Appleton in 1946. It has
an ionization trough around the equator, crests at ~±15° magnetic
latitudes and a crest-to-trough ratio of approximately 1.6 during
quiet daytime. Though several mechanisms were suggested, the
equatorial plasma fountain mechanism involving the upward ExB
drift due to eastward electric field and downward field aligned
plasma diffusion due to gravity and plasma pressure gradient
forces was found to be able to model and explain the EIA [Moffett
and Hanson, 1965]. However, the easy-to-understand
misinterpretations of the involved physics of the plasma fountain
and formation of EIA created misunderstandings in the literature,
which has lead to wrong explanations for the strong EIA observed
during major daytime space weather events. In this talk we review
the recent understanding of the mechanisms of the plasma fountain
and formation of EIA and try to clear the misunderstandings
through basic principles, observations and modeling under both
quiet and active conditions.",
conference-location = "Beijing",
conference-year = "31 July - 05 Aug.",
language = "en",
urlaccessdate = "27 abr. 2024"
}