R
Robert L. Richard
Researcher at University of California, Los Angeles
Publications - 55
Citations - 1177
Robert L. Richard is an academic researcher from University of California, Los Angeles. The author has contributed to research in topics: Magnetosphere & Plasma sheet. The author has an hindex of 19, co-authored 55 publications receiving 1077 citations.
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Observations and simulations of non-local acceleration of electrons in magnetotail magnetic reconnection events
Maha Ashour-Abdalla,Mostafa El-Alaoui,Melvyn L. Goldstein,Meng Zhou,David Schriver,Robert L. Richard,Raymond J. Walker,Margaret G. Kivelson,Margaret G. Kivelson,Kyoung Joo Hwang,Kyoung Joo Hwang +10 more
TL;DR: In this article, the authors demonstrate that electrons are energized in two distinct regions: a low-energy population (less than or equal to a few kiloelectronvolts) that arises in a diffusion region where particles are demagnetized and the magnetic topology changes, and a high-energy component (approaching 100 keV) that results from betatron acceleration within dipolarization fronts that sweep towards the inner magnetosphere far from the diffusion region.
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Consequences of magnetotail ion dynamics
TL;DR: In this paper, the trajectories of a large ensemble of particles are calculated in a modified Tsyganenko magnetic field model with a uniform cross-tail electric field, and the moments of the ion distribution function are constructed from the ion trajectories, including density, temperature, and pressure in the x-z and x-y planes.
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The formation of the wall region : consequences in the near Earth magnetotail
Maha Ashour-Abdalla,Lev Zelenyi,Jean-Michel Bosqued,Vahé Peroomian,Zhi Wang,David Schriver,Robert L. Richard +6 more
TL;DR: In this article, a region of strongly nonadiabatic ion acceleration (known as the wall region) exists in the near earth tail and demarcates two very different regimes of ion motion: adiabatic and quasi-adabatic.
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The population of the magnetosphere by solar winds ions when the interplanetary magnetic field is northward
TL;DR: In this paper, the trajectories of thousands of non-interacting ions in the magnetic and electric fields from a three dimensional global magnetohydrodynamic (MHD) simulation of the magnetosphere and the magnetosheath, under northward interplanetary magnetic field (IMF) conditions were examined.
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Substorm evolution as revealed by THEMIS satellites and a global MHD simulation
Mostafa El-Alaoui,Maha Ashour-Abdalla,Raymond J. Walker,Vahé Peroomian,Robert L. Richard,Vassilis Angelopoulos,Andrei Runov +6 more
TL;DR: In this article, a global magnetohydrodynamic simulation of the major substorm that occurred on 1 March 2008, driven by wind solar wind observations, accurately reproduced the magnetospheric observations and revealed the complexity of magnetotail dynamics during the substorm, in particular in the near-Earth plasma sheet.