Japan Geoscience Union Meeting 2019

Presentation information

[E] Oral

P (Space and Planetary Sciences ) » P-EM Solar-Terrestrial Sciences, Space Electromagnetism & Space Environment

[P-EM13] Inner magnetosphere: Recent understanding and new insights

Wed. May 29, 2019 10:45 AM - 12:15 PM A04 (TOKYO BAY MAKUHARI HALL)

convener:Yusuke Ebihara(Research Institute for Sustainable Humanosphere, Kyoto University), Danny Summers(Memorial University of Newfoundland), Yoshizumi Miyoshi(Institute for Space-Earth Environmental Research, Nagoya University), Shinji Saito(Graduate School of Science, Nagoya University), Chairperson:Yusuke Ebihara(RISH, Kyoto University), Shinji Saito(ISEE, Nagoya University)

11:05 AM - 11:25 AM

[PEM13-18] Dipolarization in the Inner Magnetosphere: Comparison between Geosynchronous Orbit and Further Inside

★Invited Papers

*Shinichi Ohtani1, Tetsuo Motoba1, Matina Gkioulidou1, Kazue Takahashi1 (1.The Johns Hopkins University Applied Physics Laboratory)

Keywords:Dipolarization, Inner magnetosphere, Substorms, Field-aligned currents

The present study addresses the current system associated with dipolarization in the inner magnetosphere. Ohtani et al. [2018] examined dipolarization events observed by the Van Allen Probes (RBSP) satellites within 5.8 RE from Earth, and by statistically comparing signatures at nearby RBSP or GOES satellites, they found that dipolarization signatures are often highly correlated (c.c. > 0.8) within 1 hr in MLT and 1 RE in RXY, and the dipolarization region expands earthward as well as azimuthally. In the present study we use, as a reference, the GOES geosynchronous satellites instead, and we examine how the magnetic field at the RBSP position changes responding to sharp dipolarizations at geosynchronous orbit. As expected from the aforementioned result, the two spacecraft occasionally observe similar dipolarization signatures with some time delay. It is, however, also found that in some events the magnetic field changes far less systematically at the RBSP probes, and in other events it barely changes or changes very gradually even if the RBSP probes are located very close to the GOES location in longitude (DMLT = 0.0 ~ 0.5 hr in MLT). By examining such variability with respect to the radial distance and magnetic latitude of the RBSP probes, we address the spatial structure of the associated current system. We also examine the variation of particle fluxes at the RBSP probes for each type of the magnetic response, and discuss the result in terms of the enhancement of local plasma pressure and the formation of a R2-sense field-aligned current system, which we suggest coexists along with the conventional substorm wedge current system.



Reference:

Ohtani, S., Motoba, T., Gkioulidou, M., Takahashi, K., & Singer, H. J. (2018). Spatial development of the dipolarization region in the inner magnetosphere. Journal of Geophysical Research: Space Physics, 123, 5452–5463. https://doi.org/10.1029/2018JA025443.