@Article{ResendeZDMSACCMCPSWLL:2022:WoStSp,
author = "Resende, Laysa Cristina Ara{\'u}jo and Zhu, Y. and Denardini,
Clezio Marcos and Moro, Juliano and Silva, Ligia Alves da and
Arras, C. and Chagas, Ronan Arraes Jardim and Chen, Sony Su and
Marchezi, Jos{\'e} Paulo and Carmo, Carolina de Sousa do and
Pican{\c{c}}o, Giorgio Arlan da Silva and Silva, R{\'e}gia
Pereira da and Wang, C. and Li, H. and Liu, Z.",
affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and {State Key
Laboratory of Space Weathe} and {Instituto Nacional de Pesquisas
Espaciais (INPE)} and {Instituto Nacional de Pesquisas Espaciais
(INPE)} and {Instituto Nacional de Pesquisas Espaciais (INPE)} and
{German Research Centre for Geosciences (GFZ)} and {Instituto
Nacional de Pesquisas Espaciais (INPE)} and {Instituto Nacional de
Pesquisas Espaciais (INPE)} and {Instituto Nacional de Pesquisas
Espaciais (INPE)} and {Instituto Nacional de Pesquisas Espaciais
(INPE)} and {Instituto Nacional de Pesquisas Espaciais (INPE)} and
{Instituto Nacional de Pesquisas Espaciais (INPE)} and {State Key
Laboratory of Space Weather} and {State Key Laboratory of Space
Weather} and {State Key Laboratory of Space Weather}",
title = "Worldwide study of the Sporadic E (Es) layer development during a
space weather event",
journal = "Journal of Atmospheric and Solar-Terrestrial Physics",
year = "2022",
volume = "241",
pages = "e105966",
month = "Dec.",
keywords = "This work analyzes the worldwide development of Sporadic E (Es)
layers in different regions during a High-Speed Solar Wind Stream
(HSS) event on March 18, 2018. We used Digisonde data from
auroral, equatorial, and low-middle latitude stations as the
primary source for the analysis. We also examined a set of data
from selected geomagnetic quiet days to compare the Es layer
behavior in such regions. The preliminary results agreed with the
understanding that the wind shear mechanism is the principal agent
causing the Es layer behavior around the globe, except for the
auroral region. Magnetometer and Total Electron Content (TEC) data
showed that an undershielding electric field could also influence
the Es layer formation over equatorial regions. Further, we
observed auroral-type Es layer (Esa) occurrence in the South
American Magnetic Anomaly (SAMA). The particle precipitation
dynamics between the auroral site and SAMA region have different
ways of acting in the Esa layer formation. Finally, our analysis
provided a deep understanding of the Es layer behavior in
different latitudes during a specific space weather event.",
abstract = "Digisonde Data; Ionosphere; Space Weather; Sporacid E Layer.",
doi = "10.1016/j.jastp.2022.105966",
url = "http://dx.doi.org/10.1016/j.jastp.2022.105966",
issn = "1364-6826",
language = "en",
targetfile = "Worldwide study of the Sporadic E (Es) layer development during a
space weather event.pdf",
urlaccessdate = "26 abr. 2024"
}