An important question that is being increasingly studied across subdisciplines of
Heliophysics is “how do mesoscale phenomena contribute to the global response of the …

Abstract Large‐amplitude (Bw> 1 nT) electromagnetic ion cyclotron (EMIC) waves can
cause the rapid loss of> 1 MeV electrons, greatly impacting radiation belt dynamics. With …

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 …

Magnetic dip plays a potentially important role in the ring‐current‐radiation‐belt‐coupling.
Here, we report a proton‐driven magnetic dip event accompanied by the expected …

Ion-scale magnetic holes are nonlinear plasma structures commonly observed in the solar
wind and Earth's magnetosphere. These holes are characterized by the magnetic field …

The cold ions, which are generally “invisible” to most instruments, have strong impacts on
plasma wave and magnetic reconnection. Under particular situations, these cold ions could …

Energetic particle injections, usually observed as sudden flux enhancements of charged
particles from tens to hundreds of keV, are one of the main mechanisms for ring current …

Recent studies have found that magnetic dips resulting from the diamagnetic motion of
injected plasmas can provide a favorable environment for electromagnetic ion cyclotron …

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

Injection flux tubes, characterized by localized equatorial magnetic field enhancements and
concomitant hot plasma populations, contribute to Saturn's magnetospheric convection cycle …