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20142026
most citedElectron scale structures and magnetic reconnection signatures in the turbulent magnetosheath

113 citations

Showing physics.space-phShow all

8 papers · 1 filter

physics.space-ph2026★ 1 cited

Turbulent dynamo in the terrestrial magnetosheath

Zoltán Vörös, Owen Wyn Roberts, Yasuhito Narita +10

Dynamo action refers to energy exchange processes through which magnetic fields are generated at the expense of kinetic energy of the plasma flows. Dynamos can generate magnetic fi…

physics.space-ph2023

Comparing 1-year GUMICS-4 simulations of the Terrestrial Magnetosphere with Cluster Measurements

Gabor Facsko, David Sibeck, Ilja Honkonen +18

We compare the predictions of the GUMICS4 global magnetohydrodynamic model for the interaction of the solar wind with the Earth's magnetosphere with Cluster~SC3 measurements for…

physics.space-ph2021★ 9 cited

Magnetic Reconnection within the Boundary Layer of a Magnetic Cloud in the Solar Wind

Zoltán Vörös, Ali Varsani, Emiliya Yordanova +5

The twisted local magnetic field at the front or rear regions of the magnetic clouds (MCs) associated with interplanetary coronal mass ejections (ICMEs) is often nearly opposite to…

physics.space-ph2020★ 12 cited

Sub-ion scale Compressive Turbulence in the Solar wind: MMS spacecraft potential observations

Owen Wyn Roberts, Rumi Nakamura, Klaus Torkar +9

Compressive plasma turbulence is investigated at sub-ion scales in the solar wind using both the Fast Plasma Investigation (FPI) instrument on the Magnetospheric MultiScale mission…

physics.space-ph2020★ 20 cited

MMS Observations of Whistler and Lower Hybrid Drift Waves Associated with Magnetic Reconnection in the Turbulent Magnetosheath

Vörös Zoltán, Emiliya Yordanova, Daniel B. Graham +2

Magnetic reconnection (MR) and the associated concurrently occurring waves have been extensively studied at large-scale plasma boundaries, in quasi-symmetric and asymmetric configu…

physics.space-ph2017★ 113 cited

Electron scale structures and magnetic reconnection signatures in the turbulent magnetosheath

E. Yordanova, Z. Vörös, A. Varsani +26

Collisionless space plasma turbulence can generate reconnecting thin current sheets as suggested by recent results of numerical magnetohydrodynamic simulations. The MMS mission pro…

physics.space-ph2015★ 9 cited

Hot flow anomaly remnant in the far geotail?

Gábor Facskó, Andrea Opitz, Benoit Lavraud +6

A hot flow anomaly (HFA) like event was observed by the Solar TErrestrial RElations Observatory (STEREO) in the night side magnetosheath in the far tail in February-March 2007. The…

physics.space-ph2014★ 15 cited

Windsock memory conditioned RAM (Co-Ram) pressure effect: forced reconnection in the Earth's magnetotail

Z. Vörös, G. Facskó, M. Khodachenko +3

Magnetic reconnection (MR) is a key physical concept explaining the addition of magnetic flux to the magnetotail and closed flux lines back-motion to the dayside magnetosphere. Thi…