On the Contribution of EMIC Waves to the Reconfiguration of the Relativistic Electron Butterfly Pitch Angle Distribution Shape on 2014 September 12—A Case Study
Authors: Claudia Medeiros, V. M. Souza, L. E. A. Vieira, D. G. Sibeck, A. J. Halford, S.-B. Kang, L. A. Da Silva, L. R. Alves, J. P. Marchezi, R. S. Dallaqua, P. R. Jauer, M. Rockenbach, O. Mendes, M. V. Alves, A. Dal Lago, M.-C. Fok, S. G. Kanekal, D. N. Baker, and C. A. Kletzing
2019 The Astrophysical Journal87236.
Provider: AAS Journals
Caption: Figure 7.
Time instant where the pitch angle–resolved electron flux drops significantly (about 80% of the maximum value) for energy channels ranging from ∼200 keV to ∼2250 keV by MagEIS (red squares) and from ∼1.8 MeV to ∼3.4 MeV by REPT (blue squares).