Field‐Aligned Current During an Interval of BY‐Dominated Interplanetary‐Field; Modeled‐to‐Observed Comparisons

We model an interval of remarkable interplanetary magnetic field (IMF), for which we have a comprehensive set of observational data. This interval is associated with the arrival of an interplanetary coronal mass ejection. The solar wind densities at the time are particularly high and the IMF is prim...

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Veröffentlicht in:	Journal of geophysical research. Space physics 2021-12, Vol.126 (12), p.n/a
Hauptverfasser:	Carter, J. A., Samsonov, A. A., Milan, S. E., Branduardi‐Raymont, G., Ridley, A. J., Paxton, L. J., Anderson, B. J., Waters, C. L., Edwards, T.
Format:	Artikel
Sprache:	eng
Schlagworte:	Aurora Auroral emissions Coronal mass ejection Cusps field‐aligned currents Interplanetary magnetic field Ionosphere Latitude Magnetic clouds Magnetic fields Magnetic reconnection Magnetopause Magnetopause reconnection Magnetospheres Magnetosphere‐ionosphere coupling modeling to observation comparison Modelling Northern Hemisphere polar cap phenomena Polar caps Polar cusps Position (location) Solar corona Solar wind Solar wind density Southern Hemisphere Spatial distribution
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