Search Publications

Particle Dynamics in the Earth's Radiation Belts: Review of Current Research and Open Questions
DOI: 10.1029/2019JA026735 Bibcode: 2020JGRA..12526735R

Li, X.; Ukhorskiy, A. Y.; Fennell, J. F. +4 more

The past decade transformed our observational understanding of energetic particle processes in near-Earth space. An unprecedented suite of observational systems was in operation including the Van Allen Probes, Arase, Magnetospheric Multiscale, Time History of Events and Macroscale Interactions during Substorms, Cluster, GPS, GOES, and Los Alamos N…

2020 Journal of Geophysical Research (Space Physics)
Cluster DoubleStar 99
Atmospheric Escape Processes and Planetary Atmospheric Evolution
DOI: 10.1029/2019JA027639 Bibcode: 2020JGRA..12527639G

Simon Wedlund, C.; Maggiolo, R.; Cessateur, G. +17 more

The habitability of the surface of any planet is determined by a complex evolution of its interior, surface, and atmosphere. The electromagnetic and particle radiation of stars drive thermal, chemical, and physical alteration of planetary atmospheres, including escape. Many known extrasolar planets experience vastly different stellar environments …

2020 Journal of Geophysical Research (Space Physics)
Cluster 95
Magnetic Reconnection in the Space Sciences: Past, Present, and Future
DOI: 10.1029/2018JA025935 Bibcode: 2020JGRA..12525935H

Hesse, M.; Cassak, P. A.

Magnetic reconnection converts, often explosively, stored magnetic energy to particle energy in space and in the laboratory. Through processes operating on length scales that are tiny, it facilitates energy conversion over dimensions of, in some cases, hundreds of Earth radii. In addition, it is the mechanism behind large current disruptions in fu…

2020 Journal of Geophysical Research (Space Physics)
Cluster 86
Magnetic Reconnection Inside a Flux Rope Induced by Kelvin-Helmholtz Vortices
DOI: 10.1029/2019JA027665 Bibcode: 2020JGRA..12527665H

Liu, Y.; Russell, C. T.; Escoubet, C. P. +23 more

On 5 May 2017, MMS observed a crater-type flux rope on the dawnside tailward magnetopause with fluctuations. The boundary-normal analysis shows that the fluctuations can be attributed to nonlinear Kelvin-Helmholtz (KH) waves. Reconnection signatures such as flow reversals and Joule dissipation were identified at the leading and trailing edges of t…

2020 Journal of Geophysical Research (Space Physics)
Cluster 35
Do Statistical Models Capture the Dynamics of the Magnetopause During Sudden Magnetospheric Compressions?
DOI: 10.1029/2019JA027289 Bibcode: 2020JGRA..12527289S

Wild, J. A.; Milan, S. E.; Imber, S. M. +9 more

Under periods of strong solar wind driving, the magnetopause can become compressed, playing a significant role in draining electrons from the outer radiation belt. Also termed "magnetopause shadowing," this loss process has traditionally been attributed to a combination of magnetospheric compression and outward radial diffusion of electrons. Howev…

2020 Journal of Geophysical Research (Space Physics)
Cluster 29
Electron Pitch-Angle Distribution in Earth's Magnetotail: Pancake, Cigar, Isotropy, Butterfly, and Rolling-Pin
DOI: 10.1029/2020JA027777 Bibcode: 2020JGRA..12527777L

Wang, Z.; Xu, Y.; Chen, G. +4 more

Electron pitch-angle distributions, including isotropy, pancake, cigar, butterfly, and recently discovered rolling-pin distributions, are crucial to understanding electron dynamics in the magnetotail. However, occurrence rates of these distributions remain unclear. Here, for the first time, we reveal the occurrence rates of these distributions in …

2020 Journal of Geophysical Research (Space Physics)
Cluster 26
Effects of Fluctuating Magnetic Field on the Growth of the Kelvin-Helmholtz Instability at the Earth's Magnetopause
DOI: 10.1029/2019JA027515 Bibcode: 2020JGRA..12527515N

Hasegawa, H.; Nakamura, R.; Narita, Y. +5 more

At the Earth's magnetopause, the Kelvin-Helmholtz (KH) instability, driven by the persistent velocity shear between the magnetosheath and the magnetosphere, has been frequently observed during northward interplanetary magnetic field periods and considered as one of the most important candidates for transporting and mixing plasmas across the magnet…

2020 Journal of Geophysical Research (Space Physics)
Cluster 22
Drift-Bounce Resonance Between Charged Particles and Ultralow Frequency Waves: Theory and Observations
DOI: 10.1029/2019JA027067 Bibcode: 2020JGRA..12527067Z

Zong, Qiu-Gang; Liu, Ying; Zhang, Shuai +7 more

Ultralow frequency (ULF) waves have long been known to resonate with magnetospheric charged particles through their drift and bounce motions. Most research interest has focused on the resonance with drift motion, which can accelerate charged particles at very high energies. The role of the bounce motion, especially for particles with lower energie…

2020 Journal of Geophysical Research (Space Physics)
Cluster 21
Outer Radiation Belt Electron Lifetime Model Based on Combined Van Allen Probes and Cluster VLF Measurements
DOI: 10.1029/2020JA028018 Bibcode: 2020JGRA..12528018A

Aryan, Homayon; Boynton, Richard; Balikhin, Michael A. +4 more

The flux of energetic electrons in the outer radiation belt shows a high variability. The interactions of electrons with very low frequency (VLF) chorus waves play a significant role in controlling the flux variation of these particles. Quantifying the effects of these interactions is crucially important for accurately modeling the global dynamics…

2020 Journal of Geophysical Research (Space Physics)
Cluster 19
Evolution of High-Speed Jets and Plasmoids Downstream of the Quasi-Perpendicular Bow Shock
DOI: 10.1029/2019JA027667 Bibcode: 2020JGRA..12527667G

Gunell, H.; Hamrin, M.; Goncharov, O. +1 more

Plasma structures with enhanced dynamic pressure, density, or speed are often observed in Earth's magnetosheath. We present a statistical study of these structures, known as jets and fast plasmoids, in the magnetosheath, downstream of both the quasi-perpendicular and quasi-parallel bow shocks. Using measurements from the four Magnetospheric Multis…

2020 Journal of Geophysical Research (Space Physics)
Cluster 18