@InProceedings{SantosReseMuelFagu:2018:StAbDo,
author = "Santos, F. C. and Resende, Laysa Cristina Ara{\'u}jo and Muella,
M. T. A. H. and Fagundes, P. R.",
affiliation = "{} and {Instituto Nacional de Pesquisas Espaciais (INPE)}",
title = "Study about the downward movement of sporadic E layers using a
theoretical model around the equatorial ionization anomaly",
year = "2018",
organization = "Latin American Conference on Space Geophysics, 11. (COLAGE)",
abstract = "Sporadic E layer (Es) refers to narrow ionization enhancements of
the ionospheric plasma with thickness less than 5 km occurring in
heights from 90 to 150 km. At equatorial and low latitude regions,
Es layers cause a scattering of radio waves at HF frequencies.
Thus, their detection and occurrence characteristics can be
analyzed from ionosonde observations. The Es layers are classied
in several types in relation to the formation mechanism according
to the region of the globe where they are detected. At low and
middle latitudes, the Es layer formation depends essentially on
the vertical wind shear associated with the tidal winds. In
several data for Brazilian region, it was observed the h type Es
with downward movement until lower altitudes. This behavior for
the low latitude is still not everything known. Therefore, in this
work, we used the Ionospheric Model of the E Region (MIRE) with
the purpose to identify the atmospheric physic dynamics of the Es
layer movement at latitudes around the Equatorial Ionization
Anomaly in the Brazilian sector. The new results about the
simulations and data will allow explaining the semidiurnal and
diurnal periodicity that characterizes the Es layer downward
motion.",
conference-location = "Buenos Aires, Argentina",
conference-year = "16-20 abr.",
language = "en",
urlaccessdate = "28 abr. 2024"
}