Charged particle scattering in dipolarized magnetotail
arXiv:2105.05397 · doi:10.1063/5.0062160
Abstract
The Earth's magnetotail is characterized by stretched magnetic field lines. Energetic particles are effectively scattered due to the field-line curvature, which then leads to isotropization of energetic particle distributions and particle precipitation to the Earth's atmosphere. Measurements of these precipitation at low-altitude spacecraft are thus often used to remotely probe the magnetotail current sheet configuration. This configuration may include spatially localized maxima of the curvature radius at equator (due to localized humps of the equatorial magnetic field magnitude) that reduce the energetic particle scattering and precipitation. Therefore, the measured precipitation patterns are related to the spatial distribution of the equatorial curvature radius that is determined by the magnetotail current sheet configuration. In this study, we show that, contrary to previous thoughts, the magnetic field line configuration with the localized curvature radius maximum can actually enhance the scattering and subsequent precipitation. The spatially localized magnetic field dipolarization (magnetic field humps) can significantly curve magnetic field lines far from the equator and create off-equatorial minima in the curvature radius. Scattering of energetic particles in these off-equatorial regions alters the scattering (and precipitation) patterns, which has not been studied yet. We discuss our results in the context of remote-sensing the magnetotail current sheet configuration with low-altitude spacecraft measurements.
References in corpus (4)
- The ELFIN Mission
- 3D Magnetic Reconnection with a spatially confined X-line extent -- Implications for Dipolarizing Flux Bundles and the Dawn-Dusk Asymmetry
- Substorm Onset Latitude and the Steadiness of Magnetospheric Convection
- On the accuracy of conservation of adiabatic invariants in slow-fast systems
Cited by in corpus (3)
- Energetic electron precipitation driven by electromagnetic ion cyclotron waves from ELFIN's low altitude perspective
- Tens to hundreds of keV electron precipitation driven by kinetic Alfvén waves during an electron injection
- Regimes of charged particle dynamics in current sheets: the machine learning approach