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Modeling Interactions of Narrowband Large Amplitude Whistler-mode Waves with Electrons in the Solar Wind inside ∼0.3 au and at 1 au Using a Particle Tracing Code

  • Authors: Cynthia Cattell, and Tien Vo

2021 The Astrophysical Journal Letters 914 L33.

  • Provider: AAS Journals

Caption: Figure 1.

Example of a CME with whistler-mode waves. (a) Magnetic field in RTN coordinates and magnitude; (b) solar wind velocity (black) and density (pink); (c) electron temperature anisotropy (black) and beta parallel (blue); and (d) parallel electron heat flux. Vertical blue lines are less coherent whistler-mode waves and vertical gold lines are narrowband whistler-mode waves (examples in bottom panels). Bottom: example 2.1 s waveform capture electric field, one perpendicular to the magnetic field component in red and one parallel component in blue.

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