Abstract
We present Van Allen Probe B observations of azimuthally limited, antisymmetric, poloidal Pc 4 electric and magnetic field pulsations in the pre-midnight sector of the magnetosphere from 05:40 to 06:00 UT on 1 May 2013. Oscillation periods were similar for the magnetic and electric fields and proton fluxes. The flux of energetic protons exhibited an energy-dependent response to the pulsations. Energetic proton variations were anticorrelated at medium and low energies. Although we attribute the pulsations to a drift-bounce resonance, we demonstrate that the energy-dependent response of the ion fluxes results from pulsation-associated velocities sweeping energy-dependent radial ion flux gradients back and forth past the spacecraft.
Original language | English (US) |
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Pages (from-to) | 955-964 |
Number of pages | 10 |
Journal | Annales Geophysicae |
Volume | 33 |
Issue number | 8 |
DOIs | |
State | Published - Aug 5 2015 |
Bibliographical note
Publisher Copyright:© Author(s) 2015.
Keywords
- Solar physics astrophysics and astronomy (wave-particle interactions)