@Article{PincheiraAbduBatiRich:2002:InIoRe,
author = "Pincheira, X. T. and Abdu, Mangalathayil Ali and Batista, Inez
Staciarini and Richards, P. G.",
affiliation = "{Universidade de Bio Bio} and {Instituto Nacional de Pesquisas
Espaciais (INPE)} and {Instituto Nacional de Pesquisas Espaciais
(INPE)} and {University of Alabama in Huntsville}",
title = "An investigation of ionospheric responses, and disturbance
thermospheric winds, during magnetic storms over South American
sector",
journal = "Journal of Geophysical Research",
year = "2002",
volume = "107",
number = "A11",
pages = "art. no. 1379",
month = "Nov.",
keywords = "equatorial f-region, meridional winds, geomagnetic storms,
electric-fields, neutral winds, plasma drifts.",
abstract = "This paper presents the results of a study of the ionospheric and
thermospheric response to magnetic storm disturbances for four
stations covering a wide range of latitude in the South American
region. The study is based on the F layer critical frequency
(f(o)F(2)) and the peak height (h(m)F(2)) from Fortaleza (FZ),
which is equatorial, Cachoeira Paulista (CP), which is low
latitude, Concepcion (CON), a midlatitude site, and King George
Island (KGI), a middle to high latitude site. Equivalent neutral
winds are extracted from the measured h(m)F(2) by employing the
Field Line Interhemispheric Plasma (FLIP) model. The Equatorial
Ionization Anomaly (EIA) can undergo enhancement due to
magnetospheric disturbance electric field that penetrates to low
latitudes during the growth phase of a storm/substorm, whereas EIA
inhibition occurs more often under disturbance dynamo (DD)
electric field. Season-dependent meridional/transequatorial winds
can significantly alter the EIA response to disturbance electric
fields. Large amplitudes of DD electric field is observed during
evening and morning hours in equinoctial, but not in winter,
months. Over the Brazilian low latitude of large westward magnetic
declination angle, large equatorward meridional wind surges seem
to be helped by the presence of disturbance zonal (westward)
winds. The low latitude disturbance can, in some cases, be traced
to specific disturbance fronts originating promptly from auroral
activity enhancements. This study confirms earlier studies that
show that the quiet time meridional wind increases with increase
of latitude and that over midlatitude it shows decreases with
increase of solar flux due to the effect of the ion drag force.
This study further shows that the disturbance meridional wind and
the intensity of DD electric field increase with increasing
intensity of high latitude energy input. The negative ionospheric
storm phase over middle latitude, observed in equinox and not in
winter, is also intensified with the increasing intensity of high
latitude energy input.",
copyholder = "SID/SCD",
doi = "10.1029/2001JA000263",
url = "http://dx.doi.org/10.1029/2001JA000263",
issn = "0148-0227 and 2156-2202",
language = "en",
targetfile = "jgra16193.pdf",
urlaccessdate = "20 maio 2024"
}