@Article{MoroXDSRSSSCCLLWS:2022:BlSpLa,
author = "Moro, Juliano and Xu, J. and Denardini, Clezio Marcos and Stefani,
G. and Resende, Laysa Cristina Ara{\'u}jo and Santos, Angela
Machado dos and Silva, Regia Pereira and Silvia, Ligia Alves da
and Carmo, Carolina de Souza do and Carrasco, Alexander Jos{\'e}
and Li, H. and Liu, Z. and Wang, C. and Schuch, Nelson Jorge",
affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and {State Key
Laboratory of Space Weather} 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 {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} and
{Instituto Nacional de Pesquisas Espaciais (INPE)}",
title = "Blanketing Sporadic-E Layer Occurrences Over Santa Maria, a
Transition Station From Low to Middle Latitude in the South
American Magnetic Anomaly (SAMA)",
journal = "Journal of Geophysical Research: Space Physics",
year = "2022",
volume = "127",
number = "12",
pages = "e2022JA030900",
month = "Dec.",
keywords = "E-region, SAMA, sporadic E layers, Esb, digisonde, MIRE model.",
abstract = "Digisonde data obtained from July 2019 to June 2020 are used to
study the overall occurrences of the blanketing types (Es-f,Es-
Es-l, Es-h, Es-c) of the sporadic layers (Es-b) over Santa Maria,
a transition station from low to middle latitude in the South
American Magnetic Anomaly (SAMA). The results show that the
average occurrence of the Es-b layers is 54%, being maximum in
summer (66%), followed by spring (63%), autumn (55%), and winter
(40%). Except during the winter, the Es-f is the predominant type,
while the Es-c generally presents the lower occurrence. In
general, the top (ftEs) and the blanketing (fbEs) frequencies
range from 3 to 4 MHz between 100 and 110 km, with more pronounced
values during daytime compared to nighttime. A comparison between
the Es-b occurrences between Santa Maria and stations outside the
SAMA shows a great reduction in Santa Maria. It is caused by the
low intensity of the geomagnetic field, which affects the layer
formation process controlled by the ion dynamics. The performance
of the E-Region Ionospheric Model (MIRE), which use the tidal wind
components provided by the Global Scale Wave Model as input, is
analyzed in simulating the fbEs parameter and compared with
measurements. The discrepancies between the modeled and measured
fbEs are reduced when the meridional/zonal wind components are
adjusted by some factor. This comparison contributes to our
understanding of the role of the tidal winds over Santa Maria, a
transition station from low to middle latitude in Brazil.",
doi = "10.1029/2022JA030900",
url = "http://dx.doi.org/10.1029/2022JA030900",
issn = "2169-9402",
language = "en",
targetfile = "JGR Space Physics - 2022 - Moro - Blanketing Sporadic\‐E
Layer Occurrences Over Santa Maria a Transition Station From
Low.pdf",
urlaccessdate = "16 jun. 2024"
}