@Article{MoraesRodrPerrPaul:2012:AnChLo,
author = "Moraes, Alison de Oliveira and Rodrigues, Fabiano da Silveira and
Perrella, Waldecir Joao and Paula, Eurico Rodrigues de",
affiliation = "Instituto Tecnol{\'o}gico de Aeron{\'a}utica (ITA), S{\~a}o
Jos{\'e} dos Campos, Brazil and Atmospheric \& Space Technology
Research Associates (ASTRA), Boulder, CO, USA and {} and
{Instituto Nacional de Pesquisas Espaciais (INPE)}",
title = "Analysis of the Characteristics of Low-Latitude GPS Amplitude
Scintillation Measured During Solar Maximum Conditions and
Implications for Receiver Performance",
journal = "Surveys in Geophysics",
year = "2012",
volume = "33",
number = "5",
pages = "1107--1131",
month = "Sept.",
keywords = "Fading (radio), Ionosphere, Ionospheric measurement,
Scintillation, Alternative approach - Amplitude scintillation -
Comprehensive studies - Cycle slips - Decorrelations - Electron
density irregularities, Equatorial anomaly, Fading duration,
GPS.",
abstract = "Ionospheric scintillations are fluctuations in the phase and/or
amplitude of trans-ionospheric radio signals caused by electron
density irregularities in the ionosphere. A better understanding
of the scintillation pattern is important to make a better
assessment of GPS receiver performance, for instance.
Additionally, scintillation can be used as a tool for remote
sensing of ionospheric irregularities. Therefore, the study of
ionospheric scintillation has both scientific as well as
technological implications. In the past few years, there has been
a significant advance in the methods for analysis of scintillation
and in our understanding of the impact of scintillation on GPS
receiver performance. In this work, we revisit some of the
existing methods of analysis of scintillation, propose an
alternative approach, and apply these techniques in a
comprehensive study of the characteristics of amplitude
scintillation. This comprehensive study made use of 32 days of
high-rate (50 Hz) measurements made by a GPS-based scintillation
monitor located in Sao JoseŽ dos Campos, Brazil (23.2S, 45.9W,
-17.5 dip latitude) near the Equatorial Anomaly during high solar
flux conditions. The variability of the decorrelation time (s0) of
scintillation patterns is presented as a function of scintillation
severity index (S4). We found that the values of s0 tend to
decrease with the increase of S4, confirming the results of
previous studies. In addition, we found that, at least for the
measurements made during this campaign, averaged values of s0 (for
fixed S4 index values) did not vary much as a function of local
time. Our results also indicate a significant impact of s0 in the
GPS carrier loop performance for S4 C 0.7. An alternative way to
compute the probability of cycle slip that.",
doi = "10.1007/s10712-011-9161-z",
url = "http://dx.doi.org/10.1007/s10712-011-9161-z",
issn = "0169-3298",
language = "en",
urlaccessdate = "16 jun. 2024"
}