The field-aligned-current system of a sun-aligned arc over Resolute Bay

Gareth William Perry, New Jersey Institute of Technology, Center for Solar-Terrestrial Research, Newark, United States, Hanna Dahlgren, KTH Royal Institute of Technology, Stockholm, Sweden; University of Southampton, Southampton, United Kingdom, Michael J Nicolls, SRI International Menlo Park, Menlo Park, CA, United States, Matthew D Zettergren, Embry-Riddle Aeronautical University, Department of Physical Sciences, Daytona Beach, FL, United States, Jean-Pierre St-Maurice, University of Saskatchewan, Saskatoon, SK, Canada, Joshua L Semeter, Boston Univ, Boston, United States, Keisuke Hosokawa, University of Electro-Communications, Department of Communication Engineering and Informatics, Chofu, Japan and Kazuo Shiokawa, Solar-Terrestrial Environment Laboratory, Nagoya University, Nagoya, Japan
Abstract:
We report on the first imaging measurements of a field-aligned-current system associated with a sun-aligned arc over Resolute Bay, Canada. The plasma parameters of the dusk-to-dawn drifting arc and surrounding ionosphere are extracted using the volumetric imaging capabilities of the Resolute Bay Incoherent Scatter Radar – North (RISR–N). Multipoint, line-of-sight plasma drift measurements are used to construct an image of the field-aligned-current system of the arc. Overlaid with red-line and green-line optical data, the current system is shown to be consistent with what is expected of an arc; namely, an upward field-aligned-current lies within the optical body of the arc, and the corresponding downward current lies adjacent to the arc. In this event, the signature of the latter is identifiable by a zonally narrow and meridionally extended F-region plasma density trough of significant magnitude situated along the leading edge of the arc. The trough is sustained by a convolution of chemical recombination and current closure in the field-aligned-current system, and maintains its orientation and position on the leading edge of the arc for the duration of its transit through the RISR-N field-of-view.