The two-way relationship between ionospheric outflow and the ring current

Welling, Daniel T.; Jordanova, Vania Koleva; Glocer, Alex; Toth, Gabor; Liemohn, Michael W.; Weimer, Dan R.

doi:10.1002/2015JA021231

Title: The two-way relationship between ionospheric outflow and the ring current

Journal Article · Mon Jun 01 00:00:00 EDT 2015 · Journal of Geophysical Research. Space Physics

DOI: https://doi.org/10.1002/2015JA021231 · OSTI ID:1215633

Welling, Daniel T. ^[1]; Jordanova, Vania Koleva ^[2]; Glocer, Alex ^[3]; Toth, Gabor ^[1]; Liemohn, Michael W. ^[1]; Weimer, Dan R. ^[4]

Univ. of Michigan, Ann Arbor, MI (United States)
Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
NASA Goddard Space Flight Center, Greenbelt, MD (United States)
Virginia Polytechnic Inst. and State Univ. (Virginia Tech), Blacksburg, VA (United States)

It is now well established that the ionosphere, because it acts as a significant source of plasma, plays a critical role in ring current dynamics. However, because the ring current deposits energy into the ionosphere, the inverse may also be true: the ring current can play a critical role in the dynamics of ionospheric outflow. This study uses a set of coupled, first-principles-based numerical models to test the dependence of ionospheric outflow on ring current-driven region 2 field-aligned currents (FACs). A moderate magnetospheric storm event is modeled with the Space Weather Modeling Framework using a global MHD code (Block Adaptive Tree Solar wind Roe-type Upwind Scheme, BATS-R-US), a polar wind model (Polar Wind Outflow Model), and a bounce-averaged kinetic ring current model (ring current atmosphere interaction model with self-consistent magnetic field, RAM-SCB). Initially, each code is two-way coupled to all others except for RAM-SCB, which receives inputs from the other models but is not allowed to feed back pressure into the MHD model. The simulation is repeated with pressure coupling activated, which drives strong pressure gradients and region 2 FACs in BATS-R-US. It is found that the region 2 FACs increase heavy ion outflow by up to 6 times over the non-coupled results. The additional outflow further energizes the ring current, establishing an ionosphere-magnetosphere mass feedback loop. This study further demonstrates that ionospheric outflow is not merely a plasma source for the magnetosphere but an integral part in the nonlinear ionosphere-magnetosphere-ring current system.

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Research Organization:: Los Alamos National Laboratory (LANL)

Sponsoring Organization:: USDOE

Grant/Contract Number:: AC52-06NA25396

OSTI ID:: 1215633

Report Number(s):: LA-UR-14-28956

Journal Information:: Journal of Geophysical Research. Space Physics, Journal Name: Journal of Geophysical Research. Space Physics Journal Issue: 6 Vol. 120; ISSN 2169-9380

Country of Publication:: United States

Language:: English

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Recent Advancements and Remaining Challenges Associated With Inner Magnetosphere Cross‐Energy/Population Interactions (IMCEPI) Yu, Yiqun; Liemohn, Mike W.; Jordanova, Vania K. Journal of Geophysical Research: Space Physics, Vol. 124, Issue 2 https://doi.org/10.1029/2018ja026282	journal	February 2019
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