@InProceedings{StekelEcScGuAnKeVi:2009:StSoFl,
author = "Stekel, Tardelli Ronan Coelho and Echer, Ezequiel and Schuch,
Nelson Jorge and Guarnieri, Luis Fernando and Antunes, Cassio
Espindola and Kemmerich, Nikolas and Vieira, Lucas Ramos",
affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto
Nacional de Pesquisas Espaciais (INPE)} and {Instituto Nacional de
Pesquisas Espaciais (INPE)} and Univap and {Instituto Nacional de
Pesquisas Espaciais (INPE)} and {Instituto Nacional de Pesquisas
Espaciais (INPE)} and {Instituto Nacional de Pesquisas Espaciais
(INPE)}",
title = "A study of solar flare electromagnetic effects on theionosphere of
southern Brazil during solar cycle 23",
year = "2009",
organization = "International Congress of the Brazilian Geophysical Society, 11.",
abstract = "The variation of solar x-ray radiation follows a behavior similar
to the solar cycle activity, which results in periodic
disturbances on the Earths atmosphere. Among the most intense
solar activity events are the solar flares: sudden, localized,
transient increases in brightness caused by active regions near
sunspots. The data analysis for investigation of this phenomenon
can provide important information about the Magnetosphere, the
Earth/Sun interaction, as well as events occurring in the
Ionosphere which can, for instance, generate disturbances in
telecommunications, small satellites or even in the Space Weather.
In this work we are studying the characteristics of high-intensity
flares (X class) and its effects on the Earth occurred during the
solar cycle 23 (1996 - 2007). For this purpose, we utilize data of
X-rays band (0.5 to 8 Å) from the GOES satellites (Geostationary
Operational Environmental Satellites), as well as the equipments
dedicated to study the Solar-Earth interactions at the Southern
Space Observatory (SSO/CRS/INPE MCT), (29°S, 53°W, 480 m a.s.l.),
S{\~a}o Martinho da Serra, RS, Brazil, such as riometer and
magnetometer. With these tools, we search for any correlation
between the solar activity and the ionospheric phenomenon, as the
Sudden Ionospheric Disturbance (SID) and magnetic crochet, causing
sudden changes in the ionospheric density and variations in the
components of the geomagnetic field that allow us to infer about
the disturbed currents in the ionosphere.",
conference-location = "Salvador, BA",
conference-year = "24 - 28 Aug.",
language = "en",
targetfile = "Resumo Exp_SBGf 2009 A study of solar flare electromagnetic
effects on ...Tardelli Ronan Coelho Stekel.doc",
urlaccessdate = "09 maio 2024"
}