@InProceedings{PaulaKantReze:2004:ChGPSi,
author = "Paula, Eurico Rodrigues de and Kantor, Ivan Jelinek and Rezende,
L. F. C. de",
affiliation = "{Divis{\~a}o de Aeronomia}",
title = "Characteristics of the GPS signal scintillation during ionospheric
irregulaties and their effects over the GPS system",
booktitle = "Anais...",
year = "2004",
organization = "Simp{\'o}sio Brasileiro de Engenharia Inercial (SBEIN), 4.",
abstract = "The ionospheric irregularities can give origin to amplitude and
phase scintillations in the GPS signal and can affect
telecommunication systems. In this work we present briefly the
physical mechanisms that give origin to the ionospheric
irregularities, and their dependence with season, local time,
solar activity and magnetic activity. Following we will describe
the potential effects of the scintillations on the GPS systems,
like the loss of lock, increase of the dilution of precision
(DOP), decrease on the available number of GPS satellites and
effects on the WAAS (Wide Area Augmentation System) navigation and
positioning system. This study was based on L1 (1.575 GHz) GPS
signal amplitude scintillations measured by an array of 11
Scintillation Monitors located over the Brazilian territory. The
GPS data were recorded at 50 samples/sec and the scintillation
index S4 was used to quantify the scintillation intensity. Over
the Brazilian territory the ionospheric irregularities incidence
is normally from September to March, however they can be triggered
at any month of the year during the incidence of a magnetic storm.
The ionospheric irregularities incidence and intensity increase
with the increase of the solar cycle. The irregularities are
generated at equatorial region after sunset due to plasma
instability processes and they occur in the pre-midnight time
sector and after midnight during some magnetic storms. The
ionospheric irregularity amplitudes are largely dependent of the
ionospheric background ionization and over the Brazilian territory
there are large ionization gradients from equator to low latitudes
due to the Equatorial Anomaly. Due to this anomaly the Total
Electron Content (TEC) presents 2 peaks at about 15o S and 15 o N
of magnetic latitude and a decrease at equatorial latitudes, and
as a consequence the ionospheric irregularities give origin to
larger amplitudes close to these crests. For instance stations
like S{\~a}o Jos{\'e} dos Campos and Cachoeira Paulista are
under the Equatorial Anomaly peaks. The ionospheric irregularities
can cause large fades on the GPS signal for stationary receivers
that can cause losses of lock (tracking) that can persist for tens
of seconds. As the ionospheric irregularity patterns (bubbles)
drift in the east-west direction with about 150 m/s, for moving
receivers like landing aircrafts, which have almost same velocity,
the fades can be potentially much longer causing even longer
tracking losses. In this work we show some statistics of loss of
lock occurrence during ionospheric irregularities. One consequence
of tracking loss is an increase in the dilution of precision due
to the GPS satellite loosing, what increases the navigation
errors. In severe conditions of irregularities incidence the
number of tracked satellites may fall below 4 that is the minimum
amount for calculating navigational solutions.",
conference-location = "S{\~a}o Jos{\'e} dos Campos",
conference-year = "17 - 19 nov.",
copyholder = "SID/SCD",
language = "pt",
organisation = "Instituto Nacional de Pesquisas Espaiciais",
targetfile = "De Paula et Rodrigues et Kantor.pdf",
urlaccessdate = "16 jun. 2024"
}