@Article{SpogliACCFMRKC:2013:GPScTo,
author = "Spogli, L. and Alfonsi, L. and Cilliers, P. J. and Correia, Emilia
and De Franceschi, G. and Mitchell, C. N. and Romano, V. and
Kinrade, J. and Cabrera, M. A.",
affiliation = "Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma 2,
Rome, Italy and Istituto Nazionale di Geofisica e Vulcanologia,
Sezione Roma 2, Rome, Italy and South African National Space
Agency (SANSA), Space Science Directorate, Western Cape, South
Africa and {Instituto Nacional de Pesquisas Espaciais (INPE)} and
Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma 2,
Rome, Italy and University of Bath, Electronic and Electrical
Engineering, Bath, United Kingdom and Istituto Nazionale di
Geofisica e Vulcanologia, Sezione Roma 2, Rome, Italy and
University of Bath, Electronic and Electrical Engineering, Bath,
United Kingdom and Laboratorio de Telecomunicaciones, Universidad
Nacional de Tucum{\'a}n (UNT), Departamento de Electricidad,
Electr{\'o}nica y Computaci{\'o}n, Tucum{\'a}n, Argentina",
title = "GPS scintillations and total electron content climatology in the
southern low, middle and high latitude regions",
journal = "Annals of Geophysics",
year = "2013",
volume = "56",
number = "2",
pages = "R0220",
keywords = "climatology, GPS, ionosphere, midlatitude environment, plasma,
sampling, seasonal variation, spatiotemporal analysis, weather
forecasting, Antarctica, Latin America.",
abstract = "In recent years, several groups have installed high-frequency
sampling receivers in the southern middle and high latitude
regions, to monitor ionospheric scintillations and the total
electron content (TEC) changes. Taking advantage of the archive of
continuous and systematic observations of the ionosphere on L-band
by means of signals from the Global Positioning System (GPS), we
present the first attempt at ionospheric scintillation and TEC
mapping from Latin America to Antarctica. The climatology of the
area considered is derived through Ground-Based Scintillation
Climatology, a method that can identify ionospheric sectors in
which scintillations are more likely to occur. This study also
introduces the novel ionospheric scintillation 'hot-spot'
analysis. This analysis first identifies the crucial areas of the
ionosphere in terms of enhanced probability of scintillation
occurrence, and then it studies the seasonal variation of the main
scintillation and TEC-related parameters. The results produced by
this sophisticated analysis give significant indications of the
spatial/ temporal recurrences of plasma irregularities, which
contributes to the extending of current knowledge of the
mechanisms that cause scintillations, and consequently to the
development of efficient tools to forecast space-weather-related
ionospheric events. © 2013 by the Istituto Nazionale di Geofisica
e Vulcanologia. All rights reserved.",
doi = "10.4401/ag-6240",
url = "http://dx.doi.org/10.4401/ag-6240",
issn = "1593-5213",
label = "scopus 2013-11",
language = "en",
urlaccessdate = "11 maio 2024"
}