Precipitation of relativistic electrons into the Earth's atmosphere regulates the outer radiation
belt fluxes and contributes to magnetosphere‐atmosphere coupling. One of the main drivers …

Energetic electron precipitation (EEP) during substorms significantly affects ionospheric
chemistry and lower‐ionosphere (< 100 km) conductance. Two mechanisms have been …

Relativistic electron precipitation to the Earth's atmosphere is an important loss mechanism
of inner magnetosphere electrons, contributing significantly to the dynamics of the radiation …

Night‐side chorus waves are often observed during plasma sheet injections, typically
confined around the equator and thus potentially responsible for precipitation of≲ 100 keV …

A global reconfiguration of the magnetotail characterizes substorms. Current sheet thinning,
intensification, and magnetic field stretching are defining features of the substorm growth …

We investigate an unusual sequence and peculiar features of magnetotail changes during a
storm‐range substorm initiated by the interplanetary shock. Auroral observations and …

Energetic electron losses by pitch‐angle scattering and precipitation to the atmosphere from
the radiation belts are controlled, to a great extent, by resonant wave particle interactions …

Electromagnetic ion cyclotron (EMIC) waves lead to rapid scattering of relativistic electrons
in Earth's radiation belts, due to their large amplitudes relative to other waves that interact …

Electron fluxes in Earth's radiation belts are significantly affected by their resonant
interaction with whistler‐mode waves. This wave‐particle interaction often occurs via first …

Electromagnetic ion cyclotron (EMIC) waves can very rapidly and effectively scatter
relativistic electrons into the atmosphere. EMIC‐driven precipitation bursts can be detected …