@InProceedings{SilvaSRABSVWSJMDZL:2021:EnPaDy,
author = "Silva, L. A. and Shi, J. and Resende, Laysa Cristina Ara{\'u}jo
and Alves, Livia Ribeiro and Batista, Inez Staciarini and Sibeck,
D. and Vieira, Luis Eduardo Antunes and Wang, C. and Souza, Vitor
Moura Cardoso e Silva and Jauer, P. R. and Marchezi, Jos{\'e}
Paulo and Denardini, Clezio Marcos and Zhang, S. Y. and Liu, Z.",
affiliation = "{State Key Laboratory of Space Weather} and {State Key Laboratory
of Space Weather} and {Instituto Nacional de Pesquisas Espaciais
(INPE)} and {Instituto Nacional de Pesquisas Espaciais (INPE)} and
{Instituto Nacional de Pesquisas Espaciais (INPE)} and {NASA
Goddard Space Flight Center} and {Instituto Nacional de Pesquisas
Espaciais (INPE)} and {State Key Laboratory of Space Weather} and
{Instituto Nacional de Pesquisas Espaciais (INPE)} and {State Key
Laboratory of Space Weather} and jose.marchezi@inpe.br and
{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Chinese
Academy of Sciences} and {State Key Laboratory of Space Weather}",
title = "Energetic particle dynamic on the radiation belts and the
generation of the sporadic E- layer (Esa) on the SHMA",
year = "2021",
organization = "Simp{\'o}sio Brasileiro de Geof{\'{\i}}sica Espacial e
Aeronomia, 8. (SBGEA)",
abstract = "The energetic particle population in the radiation belts can be
affected through the coupling between the solar wind structures
and the Earths magnetosphere. When such particles precipitate into
the upper atmosphere they may also affect both the ionosphere and
the neutral atmosphere, especially at high-latitudes and the
Southern Hemisphere Magnetic Anomaly (SHMA). Presently, the impact
of the energetic particle precipitation into the highlatitude
ionosphere is well understood. On the other hand, the direct
impact into the SHMA ionosphere is still lacking in more
information. Therefore, a case study (May 28, 2017) is selected
during the strong geomagnetic-storm (Dst: -125 nT) associated with
an Interplanetary Coronal Mass Ejection. The Van Allen Probes
recorded a significant reduction on the radiation belts electron
fluxes concomitant with a shock detected by ACE-satellite in the
Interplanetary Medium. Particles in a wide range of energy levels
were lost to the atmosphere. POES satellite data and FengYun
series spacecraft 3C confirm a strong increase of the energetic
particle flux in the SHMA region during this storm. Data from a
digisonde installed near the center of the SHMA (29.68\◦S,
53.81\◦W) show the type sporadic E-layer (Esa), unusual in
low-latitudes, during several hours. The increase of charged
particles in this region can be related to the generation of the
Esa layers, which occurrence is associated with particle
precipitation. We conclude that the radiation belt dynamics, as
well as the particle precipitation on the SHMA region during this
storm, are the main components responsible for the generation of
the Esa layers over the Brazilian region.",
conference-location = "Online",
conference-year = "22-26 mar.",
language = "en",
urlaccessdate = "09 maio 2024"
}