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Robert Ergun

Robert Ergun

· Astrophysical & Planetary SciencesVerified

University of Colorado Boulder · Astrophysical & Planetary Sciences

Active 1966–2024

h-index102
Citations46.5k
Papers1.4k300 last 5y
Funding$300k
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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.

  • Comparative Analysis of the Various Generalized Ohm's Law Terms in Magnetosheath Turbulence as Observed by Magnetospheric Multiscale

    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

Frequent coauthors

  • C. T. Russell

    775 shared
  • R. J. Strangeway

    University of Colorado System

    745 shared
  • O. Le Contel

    Laboratoire de Physique des Plasmas

    720 shared
  • R. B. Torbert

    University of New Hampshire

    670 shared
  • J. L. Burch

    Southwest Research Institute

    606 shared
  • B. L. Giles

    Portsmouth Hospitals NHS Trust

    583 shared
  • Peter Lindqvist

    KTH Royal Institute of Technology

    450 shared
  • B. Lavraud

    Centre National de la Recherche Scientifique

    436 shared

Education

  • PhD, Physics

    University of California Berkeley

    1989
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