16 citations as recorded by crossref.

1. North‐South Asymmetric Nightside Distorted Transpolar Arcs Within A Framework of Deformed Magnetosphere‐Ionosphere Coupling: IMF‐By Dependence, Ionospheric Currents, and Magnetotail Reconnection M. Nowada et al. 10.1029/2020JA027991
2. IMF By influence on fast earthward convection flows in the near-lunar magnetotail T. Liu et al. 10.1186/s40562-025-00379-5
3. Observations of Asymmetries in Ionospheric Return Flow During Different Levels of Geomagnetic Activity J. Reistad et al. 10.1029/2017JA025051
4. Dynamics of variable dusk–dawn flow associated with magnetotail current sheet flapping J. Lane et al. 10.5194/angeo-39-1037-2021
5. Convection Electric Field and Plasma Convection in a Twisted Magnetotail: A THEMIS Case Study 1–2 January 2009 T. Pitkänen et al. 10.1029/2018JA025688
6. Enhancement of Field-aligned Current during the Azimuthal Flow in the Near-Earth Magnetotail G. ZHU & Y. MA 10.11728/cjss2020.04.493
7. Response of magnetotail twisting to variations in IMF By: A THEMIS case study 1–2 January 2009 T. Pitkänen et al. 10.1002/2016GL070068
8. Timescales of Dayside and Nightside Field‐Aligned Current Response to Changes in Solar Wind‐Magnetosphere Coupling S. Milan et al. 10.1029/2018JA025645
9. IMF By Influence on Magnetospheric Convection in Earth's Magnetotail Plasma Sheet T. Pitkänen et al. 10.1029/2019GL084190
10. Relevance of the North‐South Electric Field Component in the Propagation of Fast Convective Earthward Flows in the Magnetotail: An Event Study T. Pitkänen et al. 10.1029/2021JA029233
11. Dynamic effects of restoring footpoint symmetry on closed magnetic field lines J. Reistad et al. 10.1002/2015JA022058
12. Importance of the dusk-dawn interplanetary magnetic field component (IMF By) to magnetospheric convection in Earth’s magnetotail plasma sheet T. Pitkänen et al. 10.3389/fspas.2024.1373249
13. Probing the Magnetic Structure of a Pair of Transpolar Arcs With a Solar Wind Pressure Step S. Milan et al. 10.1029/2019JA027196
14. Fast Earthward Convection in the Magnetotail and Nonzero IMF By: MMS Statistics T. Pitkänen et al. 10.1029/2023JA031593
15. How the IMF By induces a By component in the closed magnetosphere and how it leads to asymmetric currents and convection patterns in the two hemispheres P. Tenfjord et al. 10.1002/2015JA021579
16. The Influence of Localized Dynamics on Dusk‐Dawn Convection in the Earth’s Magnetotail J. Lane et al. 10.1029/2021JA030057