@InProceedings{RodriguesPaulMill:2018:RaImEq,
author = "Rodrigues, Fabiano S. and Paula, Eurico Rodrigues de and Milla, M.
A.",
affiliation = "{The University of Texas at Dallas} and {Instituto Nacional de
Pesquisas Espaciais (INPE)} and {Jicamarca Radio Observatory}",
title = "Radar imaging equatorial spread F events",
year = "2018",
organization = "Latin American Conference on Space Geophysics, 11. (COLAGE)",
abstract = "Equatorial spread F (ESF) is the name given to signatures of
ionospheric electron density irregularities observed by different
types of ground- and space-based sensors. ESF irregularities have
a wide spectrum of horizontal and vertical scale sizes, ranging
from hundreds of km down to cm. Large-scale ESF structures are
believed to be produced by the so-called ionospheric Generalized
Rayleigh-Taylor (GRT) instability. This instability finds
favorable conditions around sunset hours, near the magnetic
equator when large vertical density gradients and enhanced upward
plasma drifts are known to occur. Therefore, it explains the high
occurrence of ESF irregularities in the post-sunset hours, and
during periods when a pre-reversal enhancement of the upward ExB
plasma drifts occur. Most of the main features of ESF, including
its seasonal and longitudinal variability have been well studied
and reported. Recent efforts have focused on advancing our
understanding of the conditions leading to the short-term
(day-to-day) variability in ESF. We also seek a better
understanding, for instance, of unusual ESF events occurring
outside typical ESF periods. Those include quiet-time events
observed in the post-midnight sector, daytime, and during June
solstice. Advances in numerical modeling of ESF have allowed us to
better understand thermospheric and ionospheric conditions leading
to ESF development and suppression. To keep up with numerical
developments, new techniques and data sources need to be put in
place to confirm theories and projections. New radar measurements
and techniques can provide insights with that respect. In this
presentation, we will talk about two-dimensional views of ESF
events using observations made by relatively small radar systems.
In the first part of the talk, we will present results of
interferometric in-beam interferometric coherent scatter radar
observations made in the Brazilian sector using a small, low-power
radar system. In the second part of the talk, we will then present
new coherent scatter observations of ESF events using measurements
made by a 14-panel version of the AMISR system at the Jicamarca
Radio Observatory in Peru. While the interferometric measurements
provide high resolution observations of ESF scattering structures,
they are limited in field-of-view. We show that the limitation in
field-of-view can be overcome with AMISR-14 phased-array
observations at the expense of zonal resolution. We will present
and discuss results of both types of observations in light of
current ESF theories and modeling.",
conference-location = "Buenos Aires, Argentina",
conference-year = "16-20 abr.",
language = "en",
urlaccessdate = "28 abr. 2024"
}