Auroral Beads in Conjunction With Kinetic Alfven Waves in the Equatorial Inner-Magnetosphere

Auroral beads are spatially wavy forms routinely seen before the onset of auroral substorms and are closely related to the onset-related instabilities. To date, the acceleration mechanism of electrons that create auroral beads is not fully determined. Here, we present a fortuitous event when the Van Allen Probe A (RBSP-A) was in magnetic conjunction with auroral beads. RBSP-A observed Alfven waves, locally generated kinetic Alfven waves (KAWs) and Alfvenic accelerated electrons at several 100 eV. The Alfven waves and KAWs carried sufficient Poynting flux to power visible aurora and may control the beads' motion. These observations and previous simulations support that the Alfvenic acceleration is the acceleration mechanism of the auroral beads. Specifically, KAWs are generated around the equator and accelerate local cold electrons to several 100 eV. The waves are suggested to propagate to both hemispheres and accelerate electrons to several keV, which directly account for the auroral beads.