@Article{AbduBatMacSobMur:1996:PeChSp,
author = "Abdu, Mangalathayil Ali and Batista, Inez Staciarini and
Macdougall, J. and Sobral, Jose Humberto Andrade and
Muralikrishna, Polinaya",
affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)}",
title = "Permanent changes in sporadic E layers over Fortaleza, Brazil",
journal = "Journal of Geophysical Research",
year = "1996",
volume = "101",
number = "A12",
pages = "2629--2640",
keywords = "AERONOMIA.",
abstract = "We present an evaluation of global-scale equatorial and low
latitude ionospheric disturbances in response to the
weak-to-moderate disturbed conditions that marked the
SUNDL,kL/ATLAS 1 twelvc-day campaign of March 22 to April 2, 1992,
lonosonde data from South American and Indian-Asian longitudes are
analyzed to examine first the climatological (the average) pattern
of the critical F region parameters, (the layer peak density and
height) in comparison with the empirical International Reference
Ionospheric model, and then to characterize the day-to-day
variabilities aiming at identifying potential causal contributions
from either disturbance zonal and meridional winds or
magnetosphcric and disturbance dynamo electric fields. Included in
this analysis are data from South American midlatitude locations
which are used to determine meridional winds using an adaptation
of the servo analysis technique in the Field Line Integrated
Plasma (FLIP) model. We have made an assessment of the causal
mechanism of the day-to-day variabilities as arising from latitude
dependent disturbance meridional winds, and from electric fields
produced by disturbance zonal winds and disturbance dynamo. While
the contribution from disturbance meridional winds decreases from
middle to equatorial latitudes, that of the electric fields
maximizes around the equator. In particular, first-time evidence
based on ionosonde data is provided for a disturbance dynamo
electric field in the equatorial ionosphere. It is found that
there are two time intervals of maximum ionospheric variability
resulting from the weak to moderate magnetospheric disturbance
conditions that prevailed during the campaign: one near the
evcning/postsunset hours and the other in the postmidnight-sunrise
hours over low latitudes. At midlatitudes a broad maximum of the
response occurs from premidnight to morning hours. We provide a
comparison of results for the South American and Indian-Asian
longitudes and a discussion of the competing roles of the
disturbance zonal and meridional winds, and magnetospheric and
disturbance dynamo electric fields as a function of latitude.",
doi = "10.1016/S0273-1177(97)00610-8",
url = "http://dx.doi.org/10.1016/S0273-1177(97)00610-8",
issn = "0148-0227 and 2156-2202",
label = "8790",
language = "en",
targetfile = "abdu_permanent.pdf",
urlaccessdate = "20 maio 2024"
}