@Article{SouzaKogaGonzCard:2017:ObAsMa,
author = "Souza, Vitor Moura de and Koga, Daiki and Gonzalez Alarcon, Walter
Dem{\'e}trio and Cardoso, Fl{\'a}via Reis",
affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto
Nacional de Pesquisas Espaciais (INPE)} and {Instituto Nacional de
Pesquisas Espaciais (INPE)} and {Universidade de S{\~a}o Paulo
(USP)}",
title = "Observational aspects of magnetic reconnection at the Earth’s
magnetosphere",
journal = "Brazilian Journal of Physics",
year = "2017",
volume = "47",
number = "4",
pages = "447--459",
month = "Aug.",
keywords = "Magnetic reconnection, Earth's magnetosphere, In-situ
observations, Plasma physics.",
abstract = "Magnetic field reconnection has shown to be the dominant process
in the solar wind-Earth's magnetosphere interaction. It enables
mass, momentum, and energy exchange between different plasma
regimes, and it is regarded as an efficient plasma acceleration
and heating mechanism. Reconnection has been observed to occur in
laboratory plasmas, at planetary magnetospheres in our Solar
System, and the Sun. In this work, we focus on analyzing the
characteristics of magnetic reconnection at the Earth's
magnetosphere according to spaceborne observations in the vicinity
of our planet. Firstly, the locations where magnetic field
reconnection are expected to occur within the vast magnetospheric
region are addressed, and is shown how they are influenced by
changes in the interplanetary magnetic field direction. The main
magnetic field and plasma signatures of magnetic reconnection are
discussed from both theoretical and observational points of view.
Spacecraft observations of ion inertial length scale reconnection
are also presented.",
doi = "10.1007/s13538-017-0514-z",
url = "http://dx.doi.org/10.1007/s13538-017-0514-z",
issn = "0103-9733",
language = "en",
targetfile = "souza_observational.pdf",
urlaccessdate = "25 abr. 2024"
}