FG: Mesoscale drivers of the nightside transition region ionospheric and magnetotail evaluations

General Description

The Nightside Transition Region (NTR) is located between the outer and inner magnetosphere, and is characterized by the transition from a stretched magnetotail to a more dipolar inner magnetospheric field topology. During quiet times, the NTR acts like a “magnetic wall,” deflecting plasma and associated plasma structures around the inner magnetosphere. During active times, the NTR is a location of intense plasma energization and transport, often associated with the formation and evolution of mesoscale structures as the plasma dynamics in the transition region evolve. In recent years, our understanding of the NTR has advanced considerably due to coordinated space- and ground-based observations, as well as magnetosphere and ionosphere modeling efforts. The ground-based observations, particularly imaging systems, are arguably the only way to track the formation and evolution of mesoscale processes over a large enough region of space to tie these observations to a system-level understanding. In coordination with multiple in-situ satellites, this is an incredibly powerful combination that can “drill in” at multiple scale sizes, informing global and local models of plasma interactions. The current understanding of the plasma dynamics in the region is that most of the plasma transport and energization occurs as the plasma moves inwards from the magnetotail to the inner magnetosphere via mesoscale flows (~10s-100s km wide, when observed in the ionosphere). These flows sometimes manifest themselves as optical streamers, while others can remain invisible with current imaging technologies. Despite much research, we still do not fully understand how these mesoscale structures are incorporated in the global dynamics of the NTR, or how they are coupled to (and why they can have multiple manifestations in) the ionospheric system. It is this type of mesoscale structuring of plasma, and its connection to ionospheric processes within the NTR that we are proposing to study within this focus group. Those auroral processes such as beads, streamers, patches, omega bands, SAR arcs, STEVE, etc., all of which are driven by magnetospheric counterparts rooted in the NTR region and whose evolution is intimately tied to the large- scale dynamics of the magnetospheric system. We recognize that this is a very broad topic for a focus group, but we also know these auroral forms (and associated plasma processes) do not occur in isolation. They are often observed together and connected to magnetospheric activity levels, yet historically they have been studied largely independent of each other. Our focus group proposes to unite the study of NTR processes whose scale size sits between 10-100km in the ionosphere (1000km- to a few Re in the magnetotail) and for which the ionosphere-magnetosphere connection is best studied through coordinated ground and in situ observations. We will strive to uncover inter-connections between NTR processes, and connections between NTR processes and the larger magnetospheric dynamics.

The overarching goal of this proposed Focus Group is to utilize ground- and satellite-based data to understand the evolution and drivers of plasma processes in the NTR, and how they connect to ionospheric observations. This will help facilitate more realistic modeling representations of the region.

Focus Group Chairs

Bea Gallardo-Lacourt, NASA-GSFC/ORAU (bea.gallardolacourt@nasa.gov)

Gareth Perry, New Jersey Institute of Technology (gperry@njit.edu)

Emma Spanswick, University of Calgary (elspansw@ucalgary.ca)

Banafsheh (Bashi) Ferdousi, University of New Hampshire (Banafsheh.Ferdousi@unh.edu)

Yaireska (Yari) Collado-Vega, NASA-GSFC (yaireska.m.colladovega@nasa.gov)