@Article{ResendeZDBSMCCSAMFCPWL:2021:NeFiSp,
author = "Resende, Laysa Cristina Ara{\'u}jo and Zhu, Y. and Denardini,
Clezio Marcos and Batista, Inez Staciarini and Shi, J. and Moro,
Juliano and Chen, Sony Su and Concei{\c{c}}{\~a}o Santos, F. and
Silva, Ligia Alves da and Andrioli, V{\^a}nia F{\'a}tima and
Muella, Marcio Tadeu de Assis Honorato and Fagundes, P. R. and
Carrasco, A. J. and Pillat, V. G. and Wang, C. and Liu, Z.",
affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and {State Key
Laboratory of Space Weather} and {Instituto Nacional de Pesquisas
Espaciais (INPE)} and {Instituto Nacional de Pesquisas Espaciais
(INPE)} and {State Key Laboratory of Space Weather} and {Instituto
Nacional de Pesquisas Espaciais (INPE)} and {Instituto Nacional de
Pesquisas Espaciais (INPE)} and {Universidade do Vale do
Para{\'{\i}}ba (UNIVAP)} and {Instituto Nacional de Pesquisas
Espaciais (INPE)} and {Instituto Nacional de Pesquisas Espaciais
(INPE)} and {Universidade do Vale do Para{\'{\i}}ba (UNIVAP)}
and {Universidade do Vale do Para{\'{\i}}ba (UNIVAP)} and
{Universidad de Los Andes} and {Universidade do Vale do
Para{\'{\i}}ba (UNIVAP)} and {State Key Laboratory of Space
Weather} and {State Key Laboratory of Space Weather}",
title = "New Findings of the Sporadic E (Es) Layer Development Around the
Magnetic Equator During a High-Speed Solar (HSS) Wind Stream
Event",
journal = "Journal of Geophysical Research: Space Physics",
year = "2021",
volume = "126",
number = "9",
pages = "e2021JA029416",
month = "Sept.",
keywords = "equatorial sporadic layers, gradient drift instability, sporadic
layers simulation.",
abstract = "The equatorial (Esq) and blanketing (Esb) sporadic (Es) layers
occur due to the Equatorial Electrojet Current (EEJ) plasma
instabilities and tidal wind components, respectively. Both Esq
and Esb layers can appear concurrently over some Brazilian
equatorial regions due to the peculiar geomagnetic field
configuration in this sector. Previous works indicate that the
inclination angle limit for the Esq occurrence in ionograms is 7°.
However, we found evidence that regions more distant can also
experience such equatorial dynamics during disturbed periods. In
this context, we deeply investigated this EEJ influence expansion
effect by analyzing the Esq layers in regions not so close to the
magnetic equator during a high-speed solar wind stream event that
occurred on May 05 and 06, 2018. To explain these atypical Esq
layer occurrences, we considered the Es layer parameters obtained
from digital ionosondes over the Brazilian regions, S{\~a}o
Lu{\'{\i}}s (dip: 9.5°), and Araguatins (dip: 10.5°). We use
magnetometer data and a model named MIRE (E Region Ionospheric
Model) to validate this mechanism. The results show that the
eastward electric field of the Gradient Drift instability in the
EEJ is effective during the magnetic storm main phase in the
boundary equatorial magnetic sites, creating the Esq layers. Thus,
the EEJ plasma irregularity superimposes the wind shear mechanism,
changing the Es layer dynamics during disturbed periods over the
magnetic equator boundary sites. Therefore, this work establishes
new findings of the EEJ influence expansion dynamics in the Es
layer formation over the Brazilian regions, which was considered
in MIRE for the first time.",
doi = "10.1029/2021JA029416",
url = "http://dx.doi.org/10.1029/2021JA029416",
issn = "2169-9402",
language = "en",
targetfile = "resende_new.pdf",
urlaccessdate = "16 jun. 2024"
}