Triggered Ion-acoustic Waves
Forrest Mozer, Stuart Bale, Paul Kellogg, Roberto Livi, Orlando Romeo,, Ivan Vasko, Jaye Verniero

TL;DR
This study reports the observation of phase-locked ion-acoustic waves by the Parker Solar Probe in the solar corona, revealing a new wave regime with potential implications for electron heating and plasma instability understanding.
Contribution
It introduces the detection of a novel phase-locked ion-acoustic wave regime in the solar corona, with detailed analysis of their properties and potential impact on plasma processes.
Findings
Ion-acoustic waves observed with phase locking between low and high frequencies.
Estimated wave potential of ~10 Volts suggests electron heating via Landau resonance.
Waves exhibit pure sine wave characteristics over hours, indicating a new instability regime.
Abstract
The Parker Solar Probe is in a solar orbit with a perihelion for orbit 12 at 13.3 solar radii. The electric field experiment on this satellite observes what we call triggered ion-acoustic waves as the most dominant wave mode above a few Hz within the solar radial distance of 15-25 solar radii. In this mode, a few Hz electrostatic wave is typically accompanied by bursts of a few hundred Hz wave whose bursts are phase locked with each low frequency wave period. Plasma density fluctuations with {\Delta}n/n~0.1 accompany these waves and they have no magnetic field component. The wave durations can be hours and their field and density fluctuations are nearly pure sine waves. They are identified as ion-acoustic waves. The low and high frequency waves are measured to have the same phase velocity within experimental uncertainties, which is a requirement associated with their phase locked…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Earthquake Detection and Analysis · Astro and Planetary Science
