@InProceedings{ChingarandiBeckCandSant:2021:StLaVa,
author = "Chingarandi, Frank and Becker-Guedes, F{\'a}bio and Candido,
Cl{\'a}udia Maria Nicoli and Santos, S. M.",
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)}",
title = "A Study on the latitudinal variation of radio wave scintillation
over the brazilian sector during geomagnetic storms",
year = "2021",
organization = "Simp{\'o}sio Brasileiro de Geof{\'{\i}}sica Espacial e
Aeronomia, 8. (SBGEA)",
abstract = "The ionosphere is a medium which has significant effects on the
propagation of radio waves. Total Electron Content (TEC), is
defined as the integral of the free electrons along the path from
the satellite to the receiver. The magnitude of the TEC varies
with the time of the day, latitude, season of the year, solar
activity and geomagnetic activity. This is due to the exchange of
energy from the solar wind, interplanetary magnetic field and the
Earthas magnetosphere. TEC thus gives us a measure of the density
of the ionosphere electron density. Scintillation in GPS signals
is due to the presence of irregularities in the low latitude
ionosphere. This can have significant impact on Air Navigation
systems, Agriculture, Petroleum well as other industries which
depends on GPS for their operations. The intensity of the
scintillation is measured using the S4, ROT and ROTi indices. The
intensity depends on the background electron density as indicated
by the Total Electron Content. Thus these parameters can together
be used to study the behavior of the ionosphere at different
latitudes. This can be achieved by comparing the intensity of
scintillation at sites located near the magnetic equator with
sites located in the Equatorial Ionisation Anomaly region.",
conference-location = "Online",
conference-year = "22-26 mar.",
language = "en",
urlaccessdate = "20 maio 2024"
}