@InProceedings{MarcheziGuScTrSiCoAn:2011:LoPe1.,
author = "Marchezi, Jos{\'e} Paulo and Guimar{\~a}es Dutra, Severino Luiz
and Schuch, Nelson Jorge and Trivedi, Nalin Babulal and Silva,
Andirlei Claudir da and Coelho Stekel, Tardelli Roman and Antunes,
Cassio Espindula",
affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto
Nacional de Pesquisas Espaciais (INPE)} and {Instituto Nacional de
Pesquisas Espaciais (INPE)} and {} and {Instituto Nacional de
Pesquisas Espaciais (INPE)} and {Instituto Nacional de Pesquisas
Espaciais (INPE)} and {Instituto Nacional de Pesquisas Espaciais
(INPE)}",
title = "Long Periods (1.0 – 10 mhz) Geomagnetic Pulsations with Solar
Cycle in the South Atlantic Magnetic Anomaly Region",
year = "2011",
organization = "Magnet Brazil, 1. Simp{\'o}sio de Geomagnetismo do Brasil, 1.",
keywords = "campo magn{\'e}tico.",
abstract = "The geomagnetic field is essential to the existence of life on the
planet. The geomagnetic field acts as a barrier that protects the
Earth from the high energy particles coming from the solar wind
and outer space. The Earths magnetic Field undergoes changes on
time scales of long or short periods, from seconds to several
years (secular variations). The variations of about less than five
years are of external origin, arising from the Sun-Earth
interactions. The secular variations are associated with the
processes within the Earth. The project is a study of the
continuous pulsations Pc5 (150-600 seconds and frequency 2-7
millihertz), and its relation to solar cycle and the South
Atlantic Magnetic Anomaly (SAMA). Region where the Earths magnetic
field undergoes continuous slow decrease of its total field
strength, caused by the westward drift of the SAMA center and the
geomagnetic axis away from the anomaly region. The lower intensity
of the geomagnetic field permits easier precipitation of charged
particles in the atmosphere over the SAMA region. The SAMA center
is located in the vicinity of the Southern Space Observatory
SSO/CRS/CCR/INPE-MCT, in S{\~a}o Martinho da Serra, RS, Brazil
(29.42° S, 53.82° W, elevation 488m). The geomagnetic pulsations
are the result of the interactions between solar wind charged
particles and the magnetospheric plasma in the terrestrial
ionosphere. These variations are detected by fluxgate
magnetometers (saturated nucleus) installed at the SSO.",
conference-location = "Rio de Janeiro",
conference-year = "5 a 10 junho de 2011",
language = "en",
targetfile = "Poster Abstract - -Jos{\'e} Paulo Marchezi (concluido).pdf",
urlaccessdate = "06 maio 2024"
}