@InProceedings{JauerSPWAADVLECDSDMMSBS:2018:CoInRe,
author = "Jauer, Paulo Ricardo and Souza, Vitor Moura Cardoso e Silva and
P{\'a}dua, Marcelo Banik de and Wang, C. and Alves, Maria
Virginia and Alves, Livia Ribeiro and Da Silva, L. S. and Vieira,
Lu{\'{\i}}s Eduardo Antunes and Lopez, R. E. and Echer, Ezequiel
and Costa, Joaquim Eduardo Rezende and Denardin, Clezio Marcos and
Silva, Marlos Rockenbach da and Deggeroni, Vinicius and Medeiros,
Cl{\'a}udia and Marchezi, Jos{\'e} Paulo and Silva, G. and
Barbosa, Marcos Vin{\'{\i}}cius Grala and Schmitz, Roberta
Gon{\c{c}}alves",
affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto
Nacional de Pesquisas Espaciais (INPE)} and {Instituto Nacional de
Pesquisas Espaciais (INPE)} and {State Key Laboratory of Space
Weather (NSSC/CAS)} 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 {University of Texas
at Arlington} 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 {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)}",
title = "A global magnetohydrodynamic simulation study of ultra-low
frequency waves activity in the inner magnetosphere: corotating
interaction region + alfvenic fluctuations",
year = "2018",
organization = "Simp{\'o}sio Brasileiro de Geof{\'{\i}}sica Espacial e
Aeronomia, 7. (SBGEA)",
abstract = "The interaction between the disturbed solar wind and the
geomagnetic field gives rise to different physical processes that
can significantly affect technological systems as well as human
life. The goal of this work is to investigate the role of a
complex solar structure, i.e., a corotating interaction region
(CIR) followed by solar winds magnetic field Alfv{\'e}nic
fluctuations, in the generation of disturbances in the inner
magnetosphere in terms of the power spectral density (PSD) of the
ultra low frequency waves (ULF) in the nightside, equatorial
region. There are several studies that show the correlation
between fluctuations of solar winds magnetic field and plasma
parameters characteristic of CIRs and Alfv{\'e}nic fluctuations
and the corresponding generation of ULF waves in the internal
magnetosphere. However, some issues remain, namely, during such a
complex event it is not straightforward to decisively say which
solar wind parameters or which combinations thereof are most
effective in causing disturbances in the inner magnetosphere, or
how each part of the complex interplanetary structure influences
the most the temporal evolution of the magnetosphere. Using global
magnetohydrodynamical (MHD) simulations we perform a study which
try to address some of these questions. Firstly, we use the
magnetic field and plasma parameters of a real, complex
CIR+Alfv{\'e}nic fluctuations event as input to the
SWMF/BATS-R-US code and then calculate from the model outputs the
PSD of ULF waves in the aforementioned region. Then, we separate
the complex event into its constituent parts by building synthetic
magnetic field and plasma profiles based on the physical
parameters that characterize each of these parts. The MHD code is
then fed with each new synthetic profile to provide ULF PSDs that
are compared with those from the simulation with real solar wind
inputs. This numerical experiment will help us to understand which
solar wind parameters contribute the most for the ULF waves
activity in the nightside magnetosphere, as far as MHD simulations
are concerned, and which combination of these synthetic parameters
can reproduce the results obtained when running the MHD code with
input data from the actual event. This work might also provide
important information for future forecasting studies of ULF wave
activity in the Earths magnetosphere whenever the geospace is
under the influence of recurrent events as the one analyzed
here.",
conference-location = "Santa Maria, RS",
conference-year = "05-09 nov",
language = "pt",
urlaccessdate = "26 abr. 2024"
}