@InProceedings{SavianBSLSEGVMKS:2006:EfNeEa,
author = "Savian, Jairo Francisco and Braga, Carlos Roberto and Silva,
Samuel Martins da and Lago, Alisson Dal and Silva, Marlos
Rockenbach da and Echer, Ezequiel and Guarnieri, Fernando Luis and
Vieira, Luis Eduardo Antunes and Munakata, Kazuoki and Kuwabara,
Takao and Schuch, Nelson Jorge",
affiliation = "Instituto Nacional de Pesquisas Espaciais (INPE), Unidade Regional
Sul de Pesquisas Espaciais (RSU) and Instituto Nacional de
Pesquisas Espaciais (INPE), Unidade Regional Sul de Pesquisas
Espaciais (RSU) and Instituto Nacional de Pesquisas Espaciais
(INPE), Unidade Regional Sul de Pesquisas Espaciais (RSU) and
{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto
Nacional de Pesquisas Espaciais (INPE)} and {Instituto Nacional de
Pesquisas Espaciais (INPE)} and {Instituto Nacional de Pesquisas
Espaciais (INPE)} and {Instituto Nacional de Pesquisas Espaciais
(INPE)} and Physics Department, Shinshu University, Matsumoto,
Japan and Bartol Research Institute and Departament of Physics and
Astronomy, University of Delaware, Newark, Delaware, USA and
Instituto Nacional de Pesquisas Espaciais (INPE), Unidade Regional
Sul de Pesquisas Espaciais (RSU)",
title = "Coronal Mass Ejection SPEED Measuremnt: Effects near The Earth and
Cosmic Ray Vartiations",
booktitle = "Resumos...",
year = "2006",
pages = "106",
organization = "Simp{\'o}sio Brasileiro de Geof{\'{\i}}sica Espacial e
Aeronomia, (SBGEA).",
abstract = "CMEs ejected from the sun into the interplanetary space are
gigantic clouds of ionized gas, that after a few hours or days may
eventually hit the Earth and cause, among other effects,
geomagnetic storms. Geomagnetic storms are disturbances caused by
gusts in the solar wind, injecting a substantial quantity of
energy into the magnetosphere. In this work we analyze intense
geomagnetic storms (Dst < -100nT) using images of the solar corona
made by the Large Angle and Spectroscopic Coronagraph (LASCO) and
images of the solar disk made by the Extreme Ultraviolet Imaging
Telescope (EIT), both aboard the Solar and Heliospheric
Observatory (SOHO). Observations of plasma and interplanetary
magnetic field at one astronomic unit (1 AU), obtained by the
Advanced Composition Explorer (ACE) were also used. We analyze
high energy cosmic ray observations obtained by the high energy
50GeV Muon Multidirectional Telescope of the Brazilian Southern
Space Observatory-SSO of the INPEs Southern Regional Space
Research Center for identifying Forbush decreases in the cosmic
ray intensity. The objective of this work is to study intense
geomagnetic storms, that occurred in a relatively small time
interval, in order to identify their solar origin, interplanetary
counterparts and cosmic ray modulation near the Earth. This study
is important for the study of energetic cosmic rays modulation due
to a subsequent chain of interplanetary disturbances.",
conference-location = "S{\~a}o Jos{\'e} dos Campos, SP",
conference-year = "23-26 Outubro",
language = "pt",
volume = "F{\'{\i}}sica Solar - Terrestre",
urlaccessdate = "18 jun. 2024"
}