Results 31 to 40 of about 3,652,202 (242)
In this study, rapid loss of relativistic radiation belt electrons at low L* values (2.4–3.2) during a strong geomagnetic storm on 22 June 2015 is investigated along with five possible loss mechanisms.
M. Qin +8 more
semanticscholar +1 more source
Relativistic Microburst Scale Size Induced by a Single Point‐Source Chorus Element
Relativistic microbursts are impulsive, sub‐second precipitation bursts of relativistic electrons. They are one of the main loss mechanisms of outer radiation belt electrons, and are driven by chorus waves.
Ning Kang +4 more
doaj +1 more source
Electron flux in the Earth’s outer radiation belt is highly variable due to a delicate balance between competing acceleration and loss processes. It has been long recognized that Electromagnetic Ion Cyclotron (EMIC) waves may play a crucial role in the ...
Xing Cao +3 more
semanticscholar +1 more source
Relativistic Electron Microbursts as High‐Energy Tail of Pulsating Aurora Electrons
In this study, by simulating the wave‐particle interactions, we show that subrelativistic/relativistic electron microbursts form the high‐energy tail of pulsating aurora (PsA).
Y. Miyoshi +12 more
semanticscholar +1 more source
The effect of external magnetic field on the electron energy deposition in dense fuel for fast-shock ignition concept by using Geant4 simulation toolkit [PDF]
In the present work, the effect of the external magnetic field of on the energy deposition of the relativistic electrons into high density fuel of in fast-shock ignition concept has been investigated by using the Geant4 simulation toolkit.
S. A. Ghasemi, A. Moslehi, S. Faghih
doaj +1 more source
Local heating of radiation belt electrons to ultra-relativistic energies
Electrically charged particles are trapped by the Earth’s magnetic field, forming the Van Allen radiation belts. Observations show that electrons in this region can have energies in excess of 7 MeV.
H. Allison, Y. Shprits
semanticscholar +1 more source
Relativistic Electrons Produced by Foreshock Disturbances Observed Upstream of Earth's Bow Shock. [PDF]
Charged particles can be reflected and accelerated by strong (i.e., high Mach number) astrophysical collisionless shock waves, streaming away to form a foreshock region in communication with the shock.
L. Wilson +5 more
semanticscholar +1 more source
Geosynchronous satellites are exposed to the relativistic electrons, which may cause irreparable damage to the satellites. The prediction of the relativistic electron flux is therefore important for the safety of the satellites.
Hui Zhang +11 more
doaj +1 more source
We conduct test particle simulations to examine the acceleration mechanism of relativistic electrons through interaction with multi-subpacket chorus waves.
Ryoko Hiraga, Yoshiharu Omura
doaj +1 more source
Acceleration of sub-relativistic electrons with an evanescent optical wave at a planar interface.
We report on a theoretical and experimental study of the energy transfer between an optical evanescent wave, propagating in vacuum along the planar boundary of a dielectric material, and a beam of sub-relativistic electrons.
M. Kozák +14 more
semanticscholar +1 more source

