Need to Know: Van Allen Belts
Learn about the Van Allen Belts and how new findings from NASA’s Van Allen Probes could impact how we protect technology in space.
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Learn about the Van Allen Belts and how new findings from NASA’s Van Allen Probes could impact how we protect technology in space.
Van Allen radiation belts consist of relativistic electrons trapped by Earth's magnetic field. Trapped electrons often drift azimuthally around Earth and display a butterfly pitch angle distribution of a minimum at 90° further out than geostationary orbit. This is usually attributed to drift shell splitting resulting from day–night asymmetry in Earth’s magnetic field. However, direct observation of a butterfly distribution well inside of geostationary orbit and the origin of this phenomenon have not been provided so far. Here we report high-resolution observation that a unusual butterfly pitch angle distribution of relativistic electrons occurred within 5 Earth radii during the 28 June 2013 geomagnetic storm. In conclusion, simulation results show that combined acceleration by chorus and magnetosonic waves can successfully explain the electron flux evolution both in the energy and butterfly pitch angle distribution. Finally, the current provides a great support for the mechanism of wave-driven butterfly distribution of relativistic electrons.
Interchange stability of Van Allen belt in electrostatic approximation
Interchange stability of Van Allen belt studied in electrostatic approximation, using stabilizing and destabilizing current
Van Allen radiation belt and energetic protons and electrons trapped in geomagnetic field
Van Allen radiation belts energetic electrons injection and distribution due to magnetic storms, using satellite-borne spectrometers
Electron energy spectrum in the inner van allen belt
Van Allen belt radiation on Tiros/TOS/ITOS spacecrafts - graphs
Energy spectrum and distribution of Van Allen proton belt
Proton fluxes along trajectories through inner van allen belt
Bifurcation of the outer van allen belt and related auroral phenomena
Approximation error on interchange stability of Van Allen belt corrected
Plasma turbulence in Van Allen belts, examining weak turbulent electromagnetic wave properties, with emphasis on trapped energetic particles radiation
Proton fluxes along low acceleration trajectories through van allen belt - radiation hazard for manned interplanetary space flights
A recent study shows that the inner Van Allen belt has less radiation than previously believed. Observations from NASA’s Van Allen probes show the fastest, most energetic electrons in the inner radiation belt are actually much rarer and harder to find than scientists expected. This is good news for spacecraft that are orbiting in the region and can be damaged by high levels of radiation. The results will also help scientists better understand—and detect—effects from high-altitude nuclear explosions.
Proton flux, dosage, and damage estimates in Van Allen belt
Radiation dose from electrons and bremsstrahlung in van allen belt - spacecraft shielding