Investigating storm-time magnetospheric electrodynamics: Multi-spacecraft observations of the June 22, 2015 magnetic storm

Thursday, 17 December 2015
Poster Hall (Moscone South)
Patricia H Reiff1, Stanislav Y Sazykin1, Ramkumar Bala2, Victoria N Coffey3, Michael O Chandler3, Joseph I Minow3, Brian J Anderson4, Richard Wolf1, Joseph Huba5, Daniel N. Baker6, Barry Mauk4 and Christopher T Russell7, (1)Rice University, Houston, TX, United States, (2)Boeing Research & Technology, Huntsville, AL, United States, (3)NASA Marshall Space Flight Center, Huntsville, AL, United States, (4)Applied Physics Laboratory Johns Hopkins, Laurel, MD, United States, (5)US Naval Research Laboratory, Washington, DC, United States, (6)University of Colorado at Boulder, Boulder, CO, United States, (7)University of California Los Angeles, IGPP/EPSS, Los Angeles, CA, United States
The magnetic storm that commenced on June 22, 2015 was one of the largest storms in the current solar cycle. Availability of in situ observations from Magnetospheric Multiscale (MMS), the Van Allen Probes (VAP), and THEMIS in the magnetosphere, field-aligned currents from AMPERE, as well as the ionospheric data from the Floating Potential Measurement Unit (FPMU) instrument suite on board the International Space Station (ISS) represents an exciting opportunity to analyze storm-related dynamics. Our real-time space weather alert system sent out a “red alert” warning users of the event 2 hours in advance, correctly predicting Kp indices greater than 8. During this event, the MMS observatories were taking measurements in the magnetotail, VAP were in the inner magnetosphere, THEMIS was on the dayside, and the ISS was orbiting at 400 km every 90 minutes. Among the initial findings are the crossing of the dayside magnetopause into the region earthward of 8 RE, strong dipolarizations in the MMS magnetometer data, and dropouts in the particle fluxes seen by the MMS FPI instrument suite. At ionospheric altitudes, the FMPU measurements of the ion densities show dramatic post-sunset depletions at equatorial latitudes that are correlated with the particle flux dropouts measured by the MMS FPI. AMPERE data show highly variable currents varying from intervals of intense high latitude currents to currents at maximum polar cap expansion to 50 deg MLAT and exceeding 20 MA. In this paper, we use numerical simulations with global magnetohydrodynamic (MHD) models and the Rice Convection Model (RCM) of the inner magnetosphere in an attempt to place the observations in the context of storm-time global electrodynamics and cross-check the simulation global Birkeland currents with AMPERE distributions. Specifically, we will look at model-predicted effects of dipolarizations and the global convection on the inner magnetosphere via data-model comparison.