Image Details

Choose export citation format:

Acceleration of Electrons and Ions by an “Almost” Astrophysical Shock in the Heliosphere

  • Authors: Immanuel Christopher Jebaraj, Oleksiy Agapitov, Vladimir Krasnoselskikh, Laura Vuorinen, Michael Gedalin, Kyung-Eun Choi, Erika Palmerio, Nicolas Wijsen, Nina Dresing, Christina Cohen, Athanasios Kouloumvakos, Michael Balikhin, Rami Vainio, Emilia Kilpua, Alexandr Afanasiev, Jaye Verniero, John Grant Mitchell, Domenico Trotta, Matthew Hill, Nour Raouafi, Stuart D. Bale

Immanuel Christopher Jebaraj et al 2024 The Astrophysical Journal Letters 968 .

  • Provider: AAS Journals

Caption: Figure 3.

Analysis of the waves at the shock transition. Panels (A) and (B) show the magnetic and electric field components. The duration of the precursor whistlers (between 07:13:11.10 and 07:13:11.45) is annotated on top. Panel (A) also indicates the approximate spatial scale of the upstream in units of λ i estimated in the plasma frame. Panels (C) and (D) show the Morlet wavelet spectrum of the magnetic and electric fields. The θ kB angle between the wavevector k and the magnetic field B is shown in panel (E). In panel (F), we show the Poynting flux estimated in the spacecraft frame S sc. Finally, the hodographs of precursor whistler waves in the maximum vs. intermediate variance plane and the maximum vs. minimum variance planes are presented in panels (G) and (H), respectively. In both panels, the blue arrow denotes the mean field B 0.

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse