SM41E-2538
Ring Current Response to Different Storm Drivers. Van Allen Probes and Cluster Observations.
Thursday, 17 December 2015
Poster Hall (Moscone South)
Sam Bingham1, Christopher Mouikis1, Lynn M Kistler1, Harlan E. Spence2, Matina Gkioulidou3, Seth G Claudepierre4 and Charles J Farrugia1, (1)University of New Hampshire Main Campus, Durham, NH, United States, (2)University of New Hampshire Main Campus, Space Science Center, Durham, NH, United States, (3)Applied Physics Laboratory Johns Hopkins, Laurel, MD, United States, (4)Aerospace Corporation Santa Monica, Santa Monica, CA, United States
Abstract:
The ring current responds differently to the different solar and interplanetary storm drivers such as coronal mass injections, (CME’s), co-rotating interaction regions (CIR’s), high-speed streamers and other structures. The resulting changes in the ring current particle pressure change the global magnetic field, which affects the transport of the radiation belts. In order to determine the field changes during a storm it is necessary to understand the transport, sources and losses of the particles that contribute to the ring current. The source population of the storm time ring current is the night side plasma sheet. However, it is not clear how these convecting particles affect the storm time ring current pressure development. We use Van Allen Probes and Cluster observations together with the Volland-Stern and dipole magnetic field models to determine the contribution in the ring current pressure of the plasma sheet particles convecting from the night side that are on open drift paths, during the storm evolution. We compare storms that are related to different interplanetary drivers, CME and CIR, as observed at different local times.
