@Article{CarrascoBatiAbdu:2014:COCa,
author = "Carrasco, A. J. and Batista, Inez Staciarini and Abdu,
Mangalathayil Ali",
affiliation = "{Universidad de Los Andes (ULA)} and {Instituto Nacional de
Pesquisas Espaciais (INPE)} and {Instituto Nacional de Pesquisas
Espaciais (INPE)}",
title = "Numerical simulation of equatorial plasma bubbles over Cachimbo:
COPEX campaign",
journal = "Advances in Space Research",
year = "2014",
volume = "54",
number = "3",
pages = "443--455",
keywords = "Codes (symbols), Computer simulation, Electric fields, F region,
Geophysics, Ionospheric measurement, Numerical models, Plasmas,
Conjugate points, Equatorial ionosphere, Equatorial plasma bubble,
Flux corrected transports, Ionospheric irregularities, Plasma
bubble, Predictor-corrector methods, Vertical electric fields,
Plasma diagnostics.",
abstract = "The problem of day-to-day variability in onset of equatorial
spread F (ESF) is addressed using data from the 2002 COPEX
observational campaign in Brazil and numerical modeling. The
observational results show that for values of virtual height of
the F layer base less than 355 km at around 18:35 LT, and for the
prereversal peak enhancement of the vertical plasma drift (Vp)
less than 30 m/s, the spread-F (ESF) was absent on four nights
over Cachimbo (9.5°S, 54.8°W, dip latitude = -2.1°). In this work
we analyze the geophysical conditions for the generation of the
irregularities by comparing the nights with and without the ESF.
In the comparison a numerical code is used to simulate plasma
irregularity development in an extended altitude range from the
bottom of the equatorial F layer. The code uses the flux corrected
transport method with Boris-Book's flux limiter for the spatial
integration and a predictor-corrector method for the direct time
integration of the continuity equation for O+ and the SOR
(Successive-Over-Relaxation) method for electric potential
equation. The code is tested with different evening eastward
electric fields (or vertical drifts Vp < 30 m/s and Vp > 30 m/s)
in order to study the influence of the prereversal enhancement in
the zonal electric field on plasma bubble formation and
development. The code also takes into account the zonal wind, the
vertical electric field and the collision frequency of ions with
neutrals and the amplitude of initial perturbation. The simulation
shows a good agreement with the observational results of the ESF.
The results of the code suggest that the instability can grow at
the F layer bottomside by the Rayleigh-Taylor mechanism only when
the Vp > 30 m/s. In the analyzed cases we have considered the
competition of other geophysical parameters in the generation of
plasma structures.",
doi = "10.1016/j.asr.2013.10.017",
url = "http://dx.doi.org/10.1016/j.asr.2013.10.017",
issn = "0273-1177 and 1879-1948",
label = "scopus 2014-11 CarrascoBatiAbdu:2014:COCa",
language = "en",
targetfile = "Carrasco_Numerical.pdf",
urlaccessdate = "15 jun. 2024"
}