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Electromagnetic Energy Conversion at Reconnection Fronts

Science (American Association for the Advancement of Science), 2013-09, Vol.341 (6153), p.1478-1482

2013

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Magnetotail Fast Flow Occurrence Rate and Dawn‐Dusk Asymmetry at XGSM ∼ −60 RE

Journal of geophysical research. Space physics, 2018-03, Vol.123 (3), p.1767-1778

2018

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The Inertia‐Based Model for Reconstruction of the Electron Diffusion Region

Journal of geophysical research. Space physics, 2021-05, Vol.126 (5), p.n/a

2021

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Antidipolarization fronts observed by ARTEMIS

Journal of geophysical research. Space physics, 2014-09, Vol.119 (9), p.7181-7198

2014

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Grad–Shafranov reconstruction of the magnetic configuration in the reconnection X-point vicinity in compressible plasma

Physics of plasmas, 2020-08, Vol.27 (8)

2020

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On the azimuthal size of flux ropes near lunar orbit

Journal of geophysical research. Space physics, 2013-07, Vol.118 (7), p.4415-4424

2013

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Large‐scale energy budget of impulsive magnetic reconnection: Theory and simulation

Journal of geophysical research. Space physics, 2017-03, Vol.122 (3), p.3212-3231

2017

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Azimuthal extent and properties of midtail plasmoids from two-point ARTEMIS observations at the Earth-Moon Lagrange points

Journal of geophysical research. Space physics, 2014-03, Vol.119 (3), p.1781-1796

2014

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On the formation of tilted flux ropes in the Earth's magnetotail observed with ARTEMIS

Journal of Geophysical Research: Space Physics, 2012-05, Vol.117 (A5), p.n/a

2012

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Generalized double-gradient model of flapping oscillations: Oblique waves

Physics of plasmas, 2016-09, Vol.23 (9)

2016

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Magnetotail Fast Flow Occurrence Rate and Dawn-Dusk Asymmetry at X GSM ∼ -60 R E

Journal of geophysical research. Space physics, 2018-03, Vol.123 (3), p.1767-1778

2018

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The transition from “double-gradient” to ballooning unstable mode in bent magnetotail-like current sheet

Physics of plasmas, 2019-10, Vol.26 (10)

2019

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Current sheet bending as destabilizing factor in magnetotail dynamics

Physics of plasmas, 2018-09, Vol.25 (9)

2018

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Electron magnetohydrodynamics Grad–Shafranov reconstruction of the magnetic reconnection electron diffusion region

Frontiers in astronomy and space sciences, 2023-03, Vol.10

2023

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On the influence of the local maxima of total pressure on the current sheet stability to the kink-like (flapping) mode

Physics of plasmas, 2018-02, Vol.25 (2)

2018

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Numerical linearized MHD model of flapping oscillations

Physics of plasmas, 2016-06, Vol.23 (6)

2016

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Plasmoid growth and expulsion revealed by two-point ARTEMIS observations

Journal of geophysical research. Space physics, 2013-05, Vol.118 (5), p.2133-2144

2013

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Cluster observations of a transient signature in the magnetotail: implications for the mode of reconnection

Annales geophysicae (1988), 2011-11, Vol.29 (11), p.2131-2146

2011

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The structure of an earthward propagating magnetic flux rope early in its evolution: comparison of methods

Annales geophysicae (1988), 2009-05, Vol.27 (5), p.2215-2224

2009

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First application of a Petschek‐type reconnection model with time‐varying reconnection rate to THEMIS observations

Journal of Geophysical Research - Space Physics, 2009-01, Vol.114 (A1), p.A00C20-n/a

2009

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Inverse reconstruction technique based on time-dependent Petschek-type reconnection model: first application to THEMIS magnetotail observations

Annales geophysicae (1988), 2009-12, Vol.27 (12), p.4369-4377

2009

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Transport of reconnected magnetic flux and magnetic energy due to magnetotail reconnection

Planetary and space science, 2009-03, Vol.57 (3), p.424-425

Kiehas, S.A.

2009

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Energy budget of the reconnection process

Journal of Geophysical Research - Space Physics, 2009-08, Vol.114 (A8), p.A08201-n/a

2009

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Estimating the magnetic energy inside traveling compression regions

Annales geophysicae (1988), 2009-05, Vol.27 (5), p.1969-1978

2009

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Magnetotail Fast Flow Occurrence Rate and Dawn‐Dusk Asymmetry at X GSM ∼ −60 RE

Journal of geophysical research. Space physics, 2018-03, Vol.123 (3), p.1767-1778

2018

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Electromagnetic Energy Conversion at Reconnection Fronts

Magnetotail Fast Flow Occurrence Rate and Dawn‐Dusk Asymmetry at XGSM ∼ −60 RE

The Inertia‐Based Model for Reconstruction of the Electron Diffusion Region

Antidipolarization fronts observed by ARTEMIS

Grad–Shafranov reconstruction of the magnetic configuration in the reconnection X-point vicinity in compressible plasma

On the azimuthal size of flux ropes near lunar orbit

Large‐scale energy budget of impulsive magnetic reconnection: Theory and simulation

Azimuthal extent and properties of midtail plasmoids from two-point ARTEMIS observations at the Earth-Moon Lagrange points

On the formation of tilted flux ropes in the Earth's magnetotail observed with ARTEMIS

Generalized double-gradient model of flapping oscillations: Oblique waves

Magnetotail Fast Flow Occurrence Rate and Dawn-Dusk Asymmetry at X GSM ∼ -60 R E

The transition from “double-gradient” to ballooning unstable mode in bent magnetotail-like current sheet

Current sheet bending as destabilizing factor in magnetotail dynamics

Electron magnetohydrodynamics Grad–Shafranov reconstruction of the magnetic reconnection electron diffusion region

On the influence of the local maxima of total pressure on the current sheet stability to the kink-like (flapping) mode

Numerical linearized MHD model of flapping oscillations

Plasmoid growth and expulsion revealed by two-point ARTEMIS observations

Cluster observations of a transient signature in the magnetotail: implications for the mode of reconnection

The structure of an earthward propagating magnetic flux rope early in its evolution: comparison of methods

First application of a Petschek‐type reconnection model with time‐varying reconnection rate to THEMIS observations

Inverse reconstruction technique based on time-dependent Petschek-type reconnection model: first application to THEMIS magnetotail observations

Transport of reconnected magnetic flux and magnetic energy due to magnetotail reconnection

Energy budget of the reconnection process

Estimating the magnetic energy inside traveling compression regions

Magnetotail Fast Flow Occurrence Rate and Dawn‐Dusk Asymmetry at X GSM ∼ −60 RE

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