@Article{TakahashiWDPPCOSGIS:2016:IoTEWe,
author = "Takahashi, Hisao and Wrasse, Cristiano Max and Denardini, Clezio
Marcos and P{\'a}dua, Marcelo Banik de and Paula, Eurico
Rodrigues de and Costa, S. M. A. and Otsuka, Y. and Shiokawa, K.
and Galera Monico, J. F. and Ivo, Andr{\'e} Aparecido de Souza
and Sant'Anna, Nilson",
affiliation = "{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 Brasileiro de Geografia e
Estat{\'{\i}}stica (IBGE)} and {Nagoya University} and {Nagoya
University} and {Universidade Estadual Paulista (UNESP)} and
{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto
Nacional de Pesquisas Espaciais (INPE)}",
title = "Ionospheric TEC weather map over South America",
journal = "Space Weather",
year = "2016",
volume = "14",
number = "9",
pages = "2016SW001474",
note = "{Setores de Atividade: Pesquisa e desenvolvimento
cient{\'{\i}}fico.}",
keywords = "Total Electron Content, Space Weather, GNSS Data, Aeronomy.",
abstract = "Ionospheric weather maps using the total electron content (TEC)
monitored by ground-based Global Navigation Satellite Systems
(GNSS) receivers over South American continent, TECMAP, have been
operationally produced by Instituto Nacional de Pesquisas
Espaciaiss Space Weather Study and Monitoring Program (Estudo e
Monitoramento Brasileiro de Clima Especial) since 2013. In order
to cover the whole continent, four GNSS receiver networks, (Rede
Brasileiro de Monitoramento Cont{\'{\i}}nuo) RBMC/Brazilian
Institute for Geography and Statistics, Low-latitude Ionospheric
Sensor Network, International GNSS Service, and Red Argentina de
Monitoreo Satelital Continuo, in total ~140 sites, have been used.
TECMAPs with a time resolution of 10 min are produced in 12 h time
delay. Spatial resolution of the map is rather low, varying
between 50 and 500 km depending on the density of the observation
points. Large day-to-day variabilities of the equatorial
ionization anomaly have been observed. Spatial gradient of TEC
from the anomaly trough (total electron content unit, 1 TECU =
1016 el m2 (TECU) <10) to the crest region (TECU > 80) causes a
large ionospheric range delay in the GNSS positioning system.
Ionospheric plasma bubbles, their seeding and development, could
be monitored. This plasma density (spatial and temporal)
variability causes not only the GNSS-based positioning error but
also radio wave scintillations. Monitoring of these phenomena by
TEC mapping becomes an important issue for space weather concern
for high-technology positioning system and telecommunication.",
doi = "10.1002/2016SW001474",
url = "http://dx.doi.org/10.1002/2016SW001474",
issn = "1542-7390",
label = "lattes: 8030262077949409 3 TakahashiWNPPCOSMIS:2016:IoTEWe",
language = "en",
targetfile = "takahashi_ionospheric.pdf",
urlaccessdate = "27 abr. 2024"
}