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Alfvén Ion Cyclotron Waves in Sheath Regions Driven by Interplanetary Coronal Mass Ejections
Author(s) -
AlaLahti Matti,
Kilpua Emilia K. J.,
Souček Jan,
Pulkkinen Tuija I.,
Dimmock Andrew P.
Publication year - 2019
Publication title -
journal of geophysical research: space physics
Language(s) - English
Resource type - Journals
eISSN - 2169-9402
pISSN - 2169-9380
DOI - 10.1029/2019ja026579
Subject(s) - physics , cyclotron , solar wind , interplanetary spaceflight , coronal mass ejection , ion , ion cyclotron resonance , shock wave , astrophysics , interplanetary medium , computational physics , instability , plasma , atomic physics , nuclear physics , mechanics , quantum mechanics
We report on a statistical analysis of the occurrence and properties of Alfvén ion cyclotron (AIC) waves in sheath regions driven by interplanetary coronal mass ejections (ICMEs). We have developed an automated algorithm to identify AIC wave events from magnetic field data and apply it to investigate 91 ICME sheath regions recorded by the Wind spacecraft. Our analysis focuses on waves generated by the ion cyclotron instability. AIC waves are observed to be frequent structures in ICME‐driven sheaths, and their occurrence is the highest in the vicinity of the shock. Together with previous studies, our results imply that the shock compression has a crucial role in generating wave activity in ICME sheaths. AIC waves tend to have their frequency below the ion cyclotron frequency, and, in general, occur in plasma that is stable with respect to the ion cyclotron instability and has lower ion β ‖ than mirror modes. The results suggest that the ion beta anisotropy β ⊥ / β ‖ >1 appearing in ICME sheaths is regulated by both ion cyclotron and mirror instabilities.