Superthermal (0.5-~100 keV) Electrons near the ICME-driven shocks

Liu Yang1, Linghua Wang1, Gang Li2, Jiawei Tao3, Jiansen He3 and Chuanyi Tu4, (1)Peking University, Institute of Space Physics and Applied Technology, Beijing, China, (2)University of Alabama in Huntsville, Department of Space Sciences and CSPAR, Huntsville, AL, United States, (3)Peking University, Beijing, China, (4)University of Kiel, Kiel, Germany
Back to: Particle Acceleration and Transport at the Sun and in the Inner Heliosphere I