Counter-streaming solar energetic electrons at 1 AU are reflected from precursor ICME shocks beyond 1 AU, shown by multi-spacecraft timing, anisotropy, and prior ICME positioning.
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Reconstruction of whistler-mode magnetic field spectra from electric field and plasma measurements on THEMIS E/D yields values within a factor of ~1.5 of direct measurements from intact instruments.
Simultaneous multi-satellite observations demonstrate that tailward-of-cusp reconnection generates comparable cusp ion dispersions and convection patterns for northward and BX-dominated IMF.
The paper reviews electron transport in tangled magnetic fields, including creation via turbulence, modulation by instabilities, trapping, cross-field diffusion, and energization.
citing papers explorer
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Solar Energetic Particle Reflection by Precursor ICMEs: Multi-spacecraft Observations of Bi-Directional Electron Beams at 1 AU
Counter-streaming solar energetic electrons at 1 AU are reflected from precursor ICME shocks beyond 1 AU, shown by multi-spacecraft timing, anisotropy, and prior ICME positioning.
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Whistler-mode waves in near-equatorial THEMIS measurements: reconstruction of magnetic field spectra from electric field and plasma measurements
Reconstruction of whistler-mode magnetic field spectra from electric field and plasma measurements on THEMIS E/D yields values within a factor of ~1.5 of direct measurements from intact instruments.
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Simultaneous TRACERS and THEMIS Observations of Reversed Cusp Ion Dispersions and Dual-Lobe Reconnection
Simultaneous multi-satellite observations demonstrate that tailward-of-cusp reconnection generates comparable cusp ion dispersions and convection patterns for northward and BX-dominated IMF.
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Transport of electrons in tangled magnetic fields
The paper reviews electron transport in tangled magnetic fields, including creation via turbulence, modulation by instabilities, trapping, cross-field diffusion, and energization.