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\begin{document}

\title{Energetic charged particles in the terrestrial magnetosphere:
Cluster/RAPID results}



\author[1]{Elena A. Kronberg}%
\author[2]{Patrick W. Daly}%
\author[3]{Elena E. Grigorenko}%
\author[4]{Artem Smirnov}%
\author[5]{Berndt Klecker}%
\author[3]{Andrey Yu. Malykhin}%
\affil[1]{Ludwig Maximilian University of Munich}%
\affil[2]{Max-Planck Institut fuer Sonnensystemforschung}%
\affil[3]{Space Research Institute of RAS}%
\affil[4]{Helmholtz Centre Potsdam GFZ German Research Centre for Geosciences}%
\affil[5]{MPI}%


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  \date{June 04, 2024}


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\begin{abstract}
Energetic charged particles \textasciitilde{}\textgreater{}40 keV can
affect the plasma temperature and pressure and as a consequence the
whole dynamics of the magnetosphere. How do particles get to such
energies is a fundamental science question. Energetic particles are also
potentially hazardous for the space observations. It is, therefore,
necessary to study the origin of energetic plasma, its acceleration,
distribution and consequences on the magnetospheric dynamics. In this
work we review the related results based on observations from the
Cluster/RAPID energetic charged particle detector. These results
represent new insights in plasma acceleration, unexpected features in
its distributions, effects on substorm and geomagnetic storm dynamics
and remediated observations in the radiation belts during approximately
1.5 solar cycles.%
\end{abstract}%



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