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Observations of Deep Ionospheric F-Region Density Depletions with FPMU Instrumentation and their Relationship with the Global Dynamics of the June 22-23, 2015 Geomagnetic StormThe magnetic storm that commenced on June 22-23, 2015 was one of the largest storms in our current solar cycle, resulting from an active region on the Sun that produced numerous coronal mass ejections (CMEs) and associated interplanetary shock waves. On June 22 at 18:36 UT the magnetosphere was impacted by the shock wave on the magnetosphere. Observations from several spacecraft observed the dynamic response of the magnetosphere and ionosphere. MMS observatories in the near earth tail These low altitude measurements are correlated in the magnetosphere with particle flux dropouts measured by MMS We follow the timing of this storm in the ionosphere with the density depletions throughout the ISS orbits, DMSP drift velocities, and enhanced AMPERE Birkland currents. Together these observations and simulation results will be assembled to provide each region's context to the global dynamics and time evolution of the storm. The models during these event support and flesh out the puzzle of the global dynamics.
Document ID
20170005296
Acquisition Source
Marshall Space Flight Center
Document Type
Presentation
Authors
Coffey, Victoria
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Sazykin, Stan
(Rice Univ. Houston, TX, United States)
Chandler, Michael O.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Hairston, Marc
(Texas Univ. Dallas, TX, United States)
Minow, Joseph I.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Anderson, Brian J.
(Johns Hopkins Univ. Laurel, MD, United States)
Date Acquired
June 7, 2017
Publication Date
May 15, 2017
Subject Category
Solar Physics
Report/Patent Number
M17-6048
Meeting Information
Meeting: Applied Space Environments Conference (ASEC) 2017
Location: Huntsville, AL
Country: United States
Start Date: May 15, 2017
End Date: May 19, 2017
Sponsors: NASA Headquarters
Distribution Limits
Public
Copyright
Public Use Permitted.
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