We present a set of neural network models that reproduce the dynamics of electron fluxes in
the range of 50 keV∼ 1 MeV in the outer radiation belt. The Outer Radiation belt Electron …

As society becomes more reliant on satellite technology, it is becoming increasingly
important to understand the radiation environment throughout the Van Allen radiation belts …

Earth's radiation belts consist of high-energy charged particles trapped by Earth's magnetic
field. Strong pitch angle diffusion of electrons caused by wave-particle interaction in Earth's …

Gyroresonant wave‐particle interactions with very low frequency whistler mode chorus
waves can accelerate subrelativistic seed electrons (hundreds of keV) to relativistic energies …

We describe an artificial neural network model of the near‐Earth space radiation
environment. The geomagnetic activity index K p and low‐earth‐orbit (LEO) electron flux …

Pulsating aurora (PsA) is a diffuse type of aurora with different structures switching on and
off with a period of a few seconds. It is often associated with energetic electron precipitation …

Satellite charging is one of the most important risks for satellites on orbit. Satellite charging
can lead to an electrostatic discharge resulting in component damage, phantom commands …

With new satellite constellations being launched into low Earth orbit, the growing use of
medium Earth orbit for radio‐navigation and timing signals, slot region orbits for …

Following the end of the Van Allen Probes mission, the Arase satellite offers a unique
opportunity to continue in‐situ radiation belt and ring current particle measurements into the …

There have been a number of theories proposed concerning the loss of relativistic electrons
from the radiation belts. However, direct observations of loss were not possible on a number …