@InProceedings{SurcoEspejoCosMorPauMon:2021:SiIoEe,
author = "Surco Espejo, T. M. and Costa, E. and Moraes, A. O. and Paula,
Eurico Rodrigues de and Monico, J. F. G.",
affiliation = "{Pontif{\'{\i}}cia Universidade Cat{\'o}lica do Rio de Janeiro
(PUC-Rio)} and {Pontif{\'{\i}}cia Universidade Cat{\'o}lica do
Rio de Janeiro (PUC-Rio)} and {Instituto de Aeron{\'a}utica e
Espa{\c{c}}o (IAE)} and {Instituto Nacional de Pesquisas
Espaciais (INPE)} and {Universidade Estadual Paulista (UNESP)}",
title = "Simulating ionospheric Eeffects on a ground based augmentation
system",
year = "2021",
organization = "Simp{\'o}sio Brasileiro de Geof{\'{\i}}sica Espacial e
Aeronomia, 8. (SBGEA)",
abstract = "The ionosphere affects the propagation of GPS signals in the
equatorial and low-latitude regions. Even auxiliary systems such
as the Ground Based Augmentation System (GBAS), are affected by
ionospheric effects, which are the focus of the present
contribution. For all active channels between GPS satellites and
receivers, models for the pseudorange, carrier phase, and received
power of the GPS L1 signal will be described, considering the
geometric range; receiver and satellite clock errors, ionospheric
and tropospheric delays; multipath; phase and amplitude
scintillation; and system parameters. To simulate ionospheric
delays, the vertical Total Electron Content is characterized
through a statistical analysis of dual-frequency GPS data from the
Rede Brasileira de Monitoramento Cont´\ınuo and their
residuals relative to those provided by the International
Reference Ionosphere (IRI 2016). This study considers different
combinations of five geophysical parameters. The \α
\− µ probability distribution model is used to represent
amplitude scintillation. To define the parameters of this
distribution, a random value for the S4 index (the standard
deviation of the received power, normalized by its average value)
and the associated value for \α and µ are selected,
according to data from the CIGALA/CALIBRA network. Successive
samples for the phase scintillation term are generated similarly,
according to empirical relationships between S4 and
\σ\φ (the standard deviation of phase fluctuations)
values, combined with zero-mean Gaussian probability
distributions. Next, the functions of a GBAS (Signal-in-Space
Receive and Decode; Signal Quality Receiver; Signal, Measurement,
and Data Quality Monitoring; Multiple Reference Consistency Check)
will be described. The functional blocks are integrated by the
Executive Monitor to test, smooth, correct, and average signals,
as well as to estimate protection levels and to generate
correction messages that will be transmitted to aircrafts via a
Very High Frequency Data Broadcast link. Finally, this
contribution will present and discuss results from the above
formulation for different combinations of geophysical parameters
and configurations of interest.",
conference-location = "Online",
conference-year = "22-26 mar.",
language = "en",
urlaccessdate = "20 maio 2024"
}