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\begin{document}

\title{Wide-energy-range electron characterization of the Aug 2018 geomagnetic
storm: CSES-01 contribution}



\author[1]{Alexandra Parmentier}%
\author[2]{Matteo Martucci}%
\author[1]{Alessandro Sotgiu}%
\author[1]{Luca Carfora}%
\author[1]{Mirko Piersanti}%
\author[1]{Simona Bartocci}%
\author[1]{Roberto Battiston}%
\author[1]{William Jerome Burger}%
\author[1]{Donatella Campana}%
\author[3]{Guido Castellini}%
\author[4]{Livio Conti}%
\author[5]{Andrea Contin}%
\author[1]{Cinzia De Donato}%
\author[1]{Fulvio De Persio}%
\author[1]{Cristian De Santis}%
\author[6]{Piero Diego}%
\author[7]{Francesco Maria Follega}%
\author[7]{Roberto Iuppa}%
\author[7]{Ignazio Lazzizzera}%
\author[1]{Giuseppe Masciantonio}%
\author[1]{Matteo Mergé}%
\author[1]{Giuseppe Osteria}%
\author[1]{Francesco Palma}%
\author[5]{Federico Palmonari}%
\author[1]{Beatrice Panico}%
\author[1]{F Perfetto}%
\author[1]{Piergiorgio Picozza}%
\author[1]{Michele Pozzato}%
\author[7]{Irina Rashevskaya}%
\author[7]{Ester Ricci}%
\author[1]{Marco Ricci}%
\author[3]{Sergio Ricciarini}%
\author[8]{X Shen}%
\author[1]{Valentina Scotti}%
\author[1]{Roberta Sparvoli}%
\author[1]{Bruno Spataro}%
\author[6]{Pietro Ubertini}%
\author[1]{Vincenzo Vitale}%
\author[8]{Zhima Zeren}%
\author[9]{Simona Zoffoli}%
\author[1]{Paolo Zuccon}%
\affil[1]{National Institute for Nuclear Physics}%
\affil[2]{University of Roma Tor Vergata}%
\affil[3]{IFAC-CNR}%
\affil[4]{Uninettuno University}%
\affil[5]{University of Bologna}%
\affil[6]{INAF-IAPS}%
\affil[7]{INFN-TIFPA}%
\affil[8]{Institute of Crustal Dynamics-CEA}%
\affil[9]{Italian Space Agency}%


\vspace{-1em}



  
  \date{May 21, 2024}


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\selectlanguage{english}
\begin{abstract}
On Aug 25, 2018, a G3-class geomagnetic storm, driven by a slow coronal
mass ejection from the Sun, impacted the Earth's magnetosphere causing a
transient rearrangement of the charged-particle environment around the
planet, which was clearly detected by the entire suite of detectors on
board the CSES-01 satellite. In this work, a systematic characterization
of the magnetospheric response to the disturbance is reported on the
base of complementary electron-flux measurements from the high-energy
particle detectors (HEPP-L/H, and HEPD) embarked on CSES-01. CSES-01
results are compared to homologous data from active ground-based and
in-orbit instrumentation, and assessed to fit established scenarios in
mainstream space-weather scientific literature.%
\end{abstract}%



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