Currents Associated With Saturn's Intra‐D Ring Azimuthal Field Perturbations. Issue 7 (30th July 2019)

• Record Type: Journal Article
• Authors: Hunt, G.J.; Cowley, S.W.H.; Provan, G.; Cao, H.; Bunce, E.J.; Dougherty, M.K.; Southwood, D.J.
• Is Part Of: Journal of geophysical research. Volume 124:Issue 7(2019)
• Page Start: 5675
• Page End: 5691
• Publication Date: 2019-07-30
• Subjects: Saturn -- field‐aligned currents -- proximal orbits -- magnetospheric‐ionospheric coupling -- current densities -- grand finale; Magnetospheric physics -- Periodicals; Space environment -- Periodicals; Cosmic physics -- Periodicals; Planets -- Atmospheres -- Periodicals; Heliosphere (Astrophysics) -- Periodicals; Geophysics -- Periodicals; 523.01
• DOI: 10.1029/2019JA026588
• Languages: English
• ISSNs: 2169-9380

Abstract

Abstract: During the final 22 full revolutions of the Cassini mission in 2017, the spacecraft passed at periapsis near the noon meridian through the gap between the inner edge of Saturn's D ring and the denser layers of the planet's atmosphere, revealing the presence of an unanticipated low‐latitude current system via the associated azimuthal perturbation field peaking typically at ~10–30 nT. Assuming approximate axisymmetry, here we use the field data to calculate the associated horizontal meridional currents flowing in the ionosphere at the feet of the field lines traversed, together with the exterior field‐aligned currents required by current continuity. We show that the ionospheric currents are typically~0.5–1.5 MA per radian of azimuth, similar to auroral region currents, while the field‐aligned current densities above the ionosphere are typically ~5–10 nA/m 2, more than an order less than auroral values. The principal factor involved in this difference is the ionospheric areas into which the currents map. While around a third of passes exhibit unidirectional currents flowing northward in the ionosphere closing southward along exterior field lines, many passes also display layers of reversed northward field‐aligned current of comparable or larger magnitude in the region interior to the D ring, which may reverse sign again on the innermost field lines traversed. Overall, however, the currents generally show a high degree of north‐south conjugacy indicative of an interhemispheric system, certainly on the larger overall spatial scales involved, if less so for the smaller‐scale structures, possibly due to rapid temporal or local time variations. Key Points: We calculate ionospheric and field‐aligned currents associated with the intra‐D ring azimuthal fields observed on Cassini's proximal passes Ionospheric currents are 0.5‐1.5 MA/rad similar to auroral values, while current densities are 5‐10 nA/m 2 more than an order smaller Complex current patterns often show close north‐south conjugacy on larger spatial scales consistent with a variable interhemispheric system