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\begin{document}

\title{Magnetospheric Multiscale Statistics of High Energy Electrons Trapped in
Diamagnetic Cavities}



\author[1]{Brandon Burkholder}%
\author[1]{Katariina Nykyri}%
\author[2]{Xuanye Ma}%
\affil[1]{Embry Riddle Aeronautical University}%
\affil[2]{Embry-Riddle Aeronautical University,University of Alaska Fairbanks}%


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  \date{June 15, 2024}


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\begin{abstract}
High energy electrons observed in the magnetosheath must be accelerated
by some mech- anism that is as yet undetermined. We present observations
of high-energy electrons trapped in diamagnetic cavities as measured by
Magnetospheric Multiscale from 2015-2018. The observations support the
notion of local acceleration in the reconnection quasi-potential as many
of events show particles with pitch angles that are increasingly closer
to 90 de- grees with increasing energy. It is suggested that these
particles can end up in the loss cone and be transported to the
magnetosheath. We also characterize each diamagnetic cavity as formed
due to low- or high-latitude reconnection based on prevailing solar wind
conditions. The character of the ions in the diamagnetic cavity is only
briefly mentioned as their properties warrant another stand-alone
investigation.%
\end{abstract}%



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