Field‐Aligned Currents in Saturn's Nightside Magnetosphere: Subcorotation and Planetary Period Oscillation Components During Northern Spring

• Published in: Journal of geophysical research. Space physics 2018-05, Vol.123 (5), p.3602-3636
• Main Authors: Bradley, T. J., Cowley, S. W. H., Provan, G., Hunt, G. J., Bunce, E. J., Wharton, S. J., Alexeev, I. I., Belenkaya, E. S., Kalegaev, V. V., Dougherty, M. K.
• Format: Article
• Language: English
• Subjects: aurora; Auroral zones; Cassini mission; Equatorial regions; field‐aligned currents; Hemispheres; Intervals; Ionosphere; Ionospheric currents; Magnetic fields; Magnetosphere; Northern Hemisphere; Oscillations; Planetary magnetic fields; Planetary magnetospheres; Planetary rotation; Polar environments; Polar regions; Rotating plasmas; Rotation; Saturn; Saturn ionosphere; Seasonal variations; Spring; Summer; Winter
• ISSN: 2169-9380; 2169-9402
• DOI: 10.1029/2017JA024885

We newly analyze Cassini magnetic field data from the 2012/2013 Saturn northern spring interval of highly inclined orbits and compare them with similar data from late southern summer in 2008, thus providing unique information on the seasonality of the currents that couple momentum between Saturn's ionosphere and magnetosphere. Inferred meridional ionospheric currents in both cases consist of a steady component related to plasma subcorotation, together with the rotating current systems of the northern and southern planetary period oscillations (PPOs). Subcorotation currents during the two intervals show opposite north‐south polar region asymmetries, with strong equatorward currents flowing in the summer hemispheres but only weak currents flowing to within a few degrees of the open‐closed boundary (OCB) in the winter hemispheres, inferred due to weak polar ionospheric conductivities. Currents peak at ~1 MA rad−1 in both hemispheres just equatorward of the open‐closed boundary, associated with total downward polar currents ~6 MA, then fall across the narrow auroral upward current region to small values at subauroral latitudes. PPO‐related currents have a similar form in both summer and winter with principal upward and downward field‐aligned currents peaking at ~1.25 MA rad−1 being essentially collocated with the auroral upward current and approximately equal in strength. Though northern and southern PPO currents were approximately equal during both intervals, the currents in both hemispheres were dual modulated by both systems during 2012/2013, with approximately half the main current closing in the opposite ionosphere and half cross field in the magnetosphere, while only the northern hemisphere currents were similarly dual modulated in 2008. Key Points We study Saturn's postequinox magnetosphere‐ionosphere currents (2012/2013), comparing with previous analyses of preequinox currents (2008) Subcorotation currents have similar ~6‐MA totals north and south, but a central polar current “hole” occurs in both winter hemispheres PPO currents are dual modulated by both systems in both hemispheres in 2012/2013 but only in the north in 2008