MMS Observations of Multi‐Species Wave‐Particle Interactions and Rapid Foreshock Evolution

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Abstract
The ion foreshock is the region upstream of Earth's bow shock where magnetic field lines connect to the quasi‐parallel shock surface. Within this region, there exist a variety of backstreaming ion populations from the shock ramp that can generate ultra‐low frequency (ULF) waves through wave‐particle interactions. In this work, we use data from the Magnetospheric Multiscale (MMS) mission to study such ULF waves and backstreaming ions during a prolonged interval of above‐average solar wind helium abundance, embedded in a multi‐day period of strong solar activity driven by a coronal mass ejection. When interplanetary magnetic field orientations positioned MMS within the ion foreshock, the spacecraft captured the complete evolutionary sequence of the backstreaming ion velocity distributions: the initial formation of a reflected ion beam, followed by phase bunching and generation of coherent ULF waves, and eventual thermalization and randomization in velocity space to form diffuse ions. Intervals with elevated energetic He++ flux exhibited broadened and frequency‐downshifted wave spectra, consistent with heavy‐ion cyclotron resonance effects. The unusually rapid beam‐to‐diffuse transitions observed near the foreshock boundary likely result from the combined effects of multi‐species wave‐particle interactions and higher backstreaming ion densities during this active interval. These findings underscore the need for simulations and modeling that incorporate multi‐species effects.

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