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Alfvén Ion Cyclotron Waves in Sheath Regions Driven by Interplanetary Coronal Mass Ejections

  1. 1.
    0510735 - ÚFA 2020 RIV US eng J - Článek v odborném periodiku
    Ala-Lahti, M. - Kilpua, E. K. J. - Souček, Jan - Pulkkinen, T. I. - Dimmock, A.
    Alfvén Ion Cyclotron Waves in Sheath Regions Driven by Interplanetary Coronal Mass Ejections.
    Journal of Geophysical Research-Space Physics. Roč. 124, č. 6 (2019), s. 3893-3909. ISSN 2169-9380. E-ISSN 2169-9402
    Grant CEP: GA ČR(CZ) GA17-08772S
    Institucionální podpora: RVO:68378289
    Klíčová slova: low-frequency waves * temperature anisotropy * Earths magnetosheath * mirror instability * magnetic clouds * flux-rope * origin * shocks * CMEs * fluctuations
    Obor OECD: Fluids and plasma physics (including surface physics)
    Impakt faktor: 2.799, rok: 2019
    Způsob publikování: Open access
    https://helda.helsinki.fi/bitstream/10138/305158/1/AICwaves_in_ICMEsheaths.pdf

    We report on a statistical analysis of the occurrence and properties of Alfven 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 beta(parallel to) than mirror modes. The results suggest that the ion beta anisotropy beta(perpendicular to)/beta(parallel to) > 1 appearing in ICME sheaths is regulated by both ion cyclotron and mirror instabilities.
    Trvalý link: http://hdl.handle.net/11104/0301147

     
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