Whistler mode chorus wave is considered to play a critical role in accelerating and precipitating the electrons in the outer radiation belt. In this paper we test a conventional scenario of triggering chorus using THEMIS satellite observations of waves and particles. Specifically, we test if the chorus onset is consistent with development of anisotropy in the electron phase space density (PSD). After analyzing electron PSD for 73 chorus events, we find that, for ~80 % of them, their onsets are indeed associated with development of the positive anisotropy in PSD where the pitch angle distribution of electron velocity peaks at 90 degrees. This PSD anisotropy is prominent mainly at the electron energy range of ≤ ~20 keV. Interestingly, we further find that there is sometimes a time delay among energies in the increases of the anisotropy: A development of the positive anisotropy occurs earlier by several minutes for lower energy than for an adjacent higher energy.

1. INTRODUCTION
 2. DATA AND METHODOLOGY
 3. ANALYSIS RESULTS
 4. CONCLUSION AND DISCUSSION
 ACKNOWLEDGEMENTS
 REFERENCES

• Dong-Hee Lee(Department of Astronomy and Space Science, Chungbuk National University)
• Dae-Young Lee(Department of Astronomy and Space Science, Chungbuk National University) Corresponding Author
• Dae-Kyu Shin(Department of Astronomy and Space Science, Chungbuk National University)
• Jin-Hee Kim(Department of Astronomy and Space Science, Chungbuk National University)
• Jung-Hee Cho(Department of Astronomy and Space Science, Chungbuk National University)