Japan Geoscience Union Meeting 2014

Presentation information

Oral

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

[P-EM37_30PM1] Structure and Dynamics of the Magnetosphere

Wed. Apr 30, 2014 2:15 PM - 4:00 PM 414 (4F)

Convener:*Yoshizumi Miyoshi(Solar-Terrestrial Environement Laboratory, Nagoya University), Hiroshi Hasegawa(Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency), Chair:Satoshi Kurita(Planetary Plasma and Atmospheric Research Center, Graduate School of Science, Tohoku University), Shigeto Watanabe(Department of Cosmosciences, Hokkaido University)

2:30 PM - 2:45 PM

[PEM37-09] Pi pulsations in the near-earth magnetotail at substorm onset

*Tohru SAKURAI1, Akira KADOKURA2, Yoshimasa TANAKA2, Natsuo SATO2 (1.Tokai University, 2.National Institute of Polar Research)

Keywords:Magnetospheric Physics, Substorm, Pi pulsations

The THEMIS satellite observations showed that Pi 1 and Pi 2 period range oscillations of the magnetic and electric fields play an important role at a substorm onset in the near-Earth magnetotail. They associated energetic particle accelerations toward the inner magnetosphere. The energetic particle accelerations were observed with very similar oscillation signatures to the Pi 1 and Pi 2 period range oscillations observed in the magnetic and electric fields.. This observation suggests that the Pi 1 and Pi 2 period range oscillations might play an important role for contribution to the auroral particle accelerations at substorm onset in the near-Earth magnetotail . The examination has been done on a substorm event observed on 28 February, 2009 at a THEMIS GBO station, Kuujjuaq (KUUJ) (Mag. Lat.=66.89 N, Mag. Lon.=13.23 E, Mag. Midnight =4.15 UT, L-value = 6.4 ) in the west coast at the high latitude of the North America Continent. This substorm event was simultaneously observed in the near-Earth magnetotail by the three THEMIS satellites, THEMIS-A, -E, and ?D located in the midnight region at ~8 Re, ~8 Re and ~11 Re, respectively. The data examined in this study are the magnetic field, all-sky images (ASI) and keograms (ASK) obtained at KUUJ and the satellite observations of the magnetic field, electric field, and the electron and ion energy spectra in the ESA peir, and peer data. The results show very interesting facts of the Pi 1 and Pi 2 period range oscillations in the magnetic field and auroral activities observed on the ground and their conjunctions of the magnetic, electric fields, and the associated accelerated particles in the near-Earth magnetotail. The implication of this work provides the importance of the Pi 1 and Pi 2 period range oscillations for controlling the substorm onset plasma processes in the near-Earth magnetotail.