@InProceedings{Romero-HernandezDTGNPLNSRRJLBMMPA:2018:IoTEOv,
author = "Romero-Hernandez, E. and Denardin, Clezio Marcos and Takahashi,
Hisao and Gonzalez-Esparza, J. A. and Nogueira, P. A. B. and
P{\'a}dua, Marcelo Banik de and Lotte, Rodolfo Georjute and
Negreti, Patr{\'{\i}}cia Mara de Siqueira and Sergeeva, M. A.
and Resende, Laysa Cristina Ara{\'u}jo and Rodriguez-Martinez, M.
and Jonah, O. F. and Luz, V. and Barbosa Neto, Paulo Fran{\c{c}}a
and Monico, J. M. G. and Meneses J{\'u}nior, Francisco Carlos de
and Perez-Tijerina, E. and Aguilar-Rodriguez, E.",
affiliation = "FCFM/UANL and {Instituto Nacional de Pesquisas Espaciais (INPE)}
and {Instituto Nacional de Pesquisas Espaciais (INPE)} and
{Universidad Novo Mexico (UNAM)} and IFECTSP and {Instituto
Nacional de Pesquisas Espaciais (INPE)} and {Instituto Nacional de
Pesquisas Espaciais (INPE)} and {Instituto Nacional de Pesquisas
Espaciais (INPE)} and {Universidad Novo Mexico (UNAM)} and
{Instituto Nacional de Pesquisas Espaciais (INPE)} and
{Universidad Novo Mexico (UNAM)} and MIT and {Universidad Novo
Mexico (UNAM)} and {Instituto Nacional de Pesquisas Espaciais
(INPE)} and {Universidade Estadual Paulista (UNESP)} and
{Instituto Nacional de Pesquisas Espaciais (INPE)} and FCFM/UANL
and {Universidad Novo Mexico (UNAM)}",
title = "Ionospheric TECclimatology over the Latin America",
year = "2018",
organization = "Latin American Conference on Space Geophysics, 11. (COLAGE)",
abstract = "We present acomprehensive study of the ionospheric Total Electron
Content (TEC)climatology, based on data collected by four network
of ground-basedGlobal Navigation Satellite System (GNSS) sensor
networks thatcovered Latin America. This work provides a
qualitative andquantitative daytime and nighttime analysis of the
ionospheric TECclimatology, which encompasses: (a) the response of
TEC to the solar ux; (b) the seasonal variation of TEC in dierent
latitudinal andlongitudinal ranges; and (c) the North-South
electron densityasymmetry of TEC over Latin America. The response
to the solar uxis based on day-to-day TEC variations during two
periods of dierentsolar activity conditions: 2011 (ascending
phase) and 2014 (maximum).",
conference-location = "Buenos Aires, Argentina",
conference-year = "16-20 abr.",
language = "en",
urlaccessdate = "27 abr. 2024"
}