Energetic electron precipitation (EEP) from the radiation belts into
Earth’s atmosphere leads to several profound effects (e.g., enhancement
of ionospheric conductivity, possible acceleration of ozone destruction
processes). An accurate quantification of the energy input and
ionization due to EEP is still lacking due to instrument limitations of
low-Earth-orbit satellites capable of detecting EEP. The deployment of
the ELFIN CubeSats marks a new era of observations of EEP with an
improved pitch-angle (0°–180°) and energy (50 keV–6 MeV) resolution.
Here, we focus on the EEP recorded by ELFIN coincident with
electromagnetic ion cyclotron (EMIC) waves, which play a major role in
radiation belt electron losses. The EMIC-driven EEP
(~200 keV–~2 MeV) exhibits a
pitch-angle distribution (PAD) that flattens with increasing energy,
indicating a more efficient high-energy precipitation. Leveraging the
combination of unique electron measurements from ELFIN and a
comprehensive ionization model known as the Boulder Electron Radiation
to Ionization (BERI), we quantify the energy input of EMIC-driven
precipitation (on average, ~3.3x10-2 erg/cm2/s),
identify its location (any longitude, 50°–70° latitude), and provide
the expected range of ion-electron production rate (on average, 100–200
pairs/cm3/s), peaking in the mesosphere – a region often overlooked.
Our findings are crucial for improving our understanding of the
magnetosphere-ionosphere-atmosphere system as they accurately specify
the contribution of EMIC-driven EEP, which serves as crucial inputs to
state-of-the-art atmospheric models (e.g., WACCM), to quantify the
accurate impact of EMIC waves on both the atmospheric chemistry and
dynamics.