@Article{JauerWSAAPMSLLVLGEMCD:2019:CoInRe,
author = "Jauer, Paulo Ricardo and Wang, C. and Souza, Vitor Moura Cardoso e
Silva and Alves, Maria Virginia and Alves, Livia Ribeiro and
P{\'a}dua, Marcelo Banik de and Marchezi, Jos{\'e} Paulo and
Silva, L. A. da and Liu, Z. and Li, H. and Vieira, Luis Eduardo
Antunes and Lago, Alisson Dal and Gonzalez Alarcon, Walter
Dem{\'e}trio and Echer, Ezequiel and Medeiros, Cl{\'a}udia and
Costa, Joaquim Eduardo Rezende and Denardin, Clezio Marcos",
affiliation = "{Chinese Academy of Science} and {Chinese Academy of Science} 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 {Chinese Academy of Science} and {Chinese Academy of
Science} and {Chinese Academy of Science} 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 wave activity in the inner magnetosphere:
corotating interaction region + alfv{\'e}nic fluctuations",
journal = "The Astrophysical Journal",
year = "2019",
volume = "886",
number = "1",
pages = "59--75",
abstract = "Using global magnetohydrodynamic (MHD) simulations, we investigate
the role played by a complex solar structure composed of a
corotating interaction region (CIR) followed by solar wind
Alfv{\'e}nic fluctuations on the magnetospheres nightside,
equatorial electric field oscillations in the ultra-low-frequency
range. A series of numerical experiments are performed employing
synthetic solar wind inputs resembling those of a real CIR
+Alfv{\'e}nic fluctuation event that reached Earths magnetosphere
on 2003 April 20. The following is found: (i) Radial electric
field component fluctuations are excited via magnetopause boundary
motions driven either by solar wind density variations
characteristic of CIRs or by solar wind Alfv{\'e}nic fluctuations
with a given oscillation period. (ii) Azimuthal electric field
component fluctuations nearer to Earth, that is, at radial
distances R less than about 5RE (RE = 1 Earth radius), are
apparently not related to either of the two types of sinusoidal
solar wind Alfv{\'e}nic fluctuations used in this study featuring
monochromatic frequencies of 0.833 mHz (20-minute period) and
1.666 mHz (10-minute period). Instead, these innermost azimuthal
component fluctuations show enhanced activity when inner
magnetosphere convection increases as a result of a southward
turning of the interplanetary magnetic field component Bz. (iii)
Lastly, outermost (R \ 7 RE) azimuthal electric field
oscillations weakly respond to monochromatic solar wind
Alfv{\'e}nic fluctuations by showing power spectral density peaks
at both driving frequencies, but only near the flanks of the
magnetopause, thus suggesting that such oscillations are being
excited also owing to magnetopause boundary motions driven by
solar wind Alfv{\'e}nic fluctuations.",
doi = "10.3847/1538-4357/ab4db5",
url = "http://dx.doi.org/10.3847/1538-4357/ab4db5",
issn = "0004-637X",
label = "lattes: 2768849231719678 12 JauerWSAAPMSLLVLGEMCD:2019:CoInRe",
language = "pt",
targetfile = "jauer_global.pdf",
urlaccessdate = "27 abr. 2024"
}