
Robert Ergun
· Astrophysical & Planetary SciencesVerifiedUniversity of Colorado Boulder · Astrophysical & Planetary Sciences
Active 1966–2024
Research topics
- Physics
- Quantum mechanics
- Classical mechanics
- Computational physics
Selected publications
Magnetotail reconnection onset caused by electron kinetics with a strong external driver
Nature Communications · 2020 · 119 citations
- Physics
- Classical mechanics
- Quantum mechanics
Magnetotail reconnection plays a crucial role in explosive energy conversion in geospace. Because of the lack of in-situ spacecraft observations, the onset mechanism of magnetotail reconnection, however, has been controversial for decades. The key question is whether magnetotail reconnection is externally driven to occur first on electron scales or spontaneously arising from an unstable configuration on ion scales. Here, we show, using spacecraft observations and particle-in-cell (PIC) simulations, that magnetotail reconnection starts from electron reconnection in the presence of a strong external driver. Our PIC simulations show that this electron reconnection then develops into ion reconnection. These results provide direct evidence for magnetotail reconnection onset caused by electron kinetics with a strong external driver.
Journal of Geophysical Research Space Physics · 2020 · 23 citations
- Physics
- Computational physics
- Quantum mechanics
Abstract Decomposing the electric field ( E ) into the contributions from generalized Ohm's law provides key insight into both nonlinear and dissipative dynamics across the full range of scales within a plasma. Using high‐resolution, multispacecraft measurements of three intervals in Earth's magnetosheath from the Magnetospheric Multiscale mission, the influence of the magnetohydrodynamic, Hall, electron pressure, and electron inertia terms from Ohm's law, as well as the impact of a finite electron mass, on the turbulent E spectrum are examined observationally for the first time. The magnetohydrodynamic, Hall, and electron pressure terms are the dominant contributions to E over the accessible length scales, which extend to scales smaller than the electron gyroradius at the greatest extent, with the Hall and electron pressure terms dominating at sub‐ion scales. The strength of the nonideal electron pressure contribution is stronger than expected from linear kinetic Alfvén waves and a partial antialignment with the Hall electric field is present, linked to the relative importance of electron diamagnetic currents in the turbulence. The relative contribution of linear and nonlinear electric fields scale with the turbulent fluctuation amplitude, with nonlinear contributions playing the dominant role in shaping E for the intervals examined in this study. Overall, the sum of the Ohm's law terms and measured E agree to within ∼20% across the observable scales. These results both confirm general expectations about the behavior of E in turbulent plasmas and highlight features that should be explored further theoretically.
Recent grants
GEM: Small and Medium Scale Modeling of the Auroral Downward Current Region
NSF · $300k · 2005–2008
Frequent coauthors
- 775 shared
C. T. Russell
- 745 shared
R. J. Strangeway
University of Colorado System
- 720 shared
O. Le Contel
Laboratoire de Physique des Plasmas
- 670 shared
R. B. Torbert
University of New Hampshire
- 606 shared
J. L. Burch
Southwest Research Institute
- 583 shared
B. L. Giles
Portsmouth Hospitals NHS Trust
- 450 shared
Peter Lindqvist
KTH Royal Institute of Technology
- 436 shared
B. Lavraud
Centre National de la Recherche Scientifique
Education
- 1989
PhD, Physics
University of California Berkeley
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