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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 hemispheresP. Tenfjord, S. E. Milan, N. Østgaard et al.|Bergen Open Research Archive (BORA) (University of Bergen)|2015Cited by 107
Magnetospheric response and reconfiguration times following IMF <i>B<sub>y</sub></i> reversalsP. Tenfjord, S. E. Milan, Jone Peter Reistad et al.|Journal of Geophysical Research Space Physics|2016Cited by 53
Intensity asymmetries in the dusk sector of the poleward auroral oval due to IMF <i>B</i> <sub> <i>x</i> </sub>Jone Peter Reistad, S. E. Milan, N. Østgaard et al.|Journal of Geophysical Research Space Physics|2014Cited by 41
How the IMF <i> B <sub>y</sub> </i> Induces a Local <i> B <sub>y</sub> </i> Component During Northward IMF <i> B <sub>z</sub> </i> and Characteristic TimescalesP. Tenfjord, Anders Ohma, Nikolai Østgaard et al.|Journal of Geophysical Research Space Physics|2018Cited by 39