Počet záznamů: 1  

Statistical analysis of mirror mode waves in sheath regions driven by interplanetary coronal mass ejection

  1. 1.
    0501832 - ÚFA 2019 RIV DE eng J - Článek v odborném periodiku
    Ala-Lahti, M.M. - Kilpua, E. K. J. - Dimmock, A.P. - Osmane, A. - Pulkkinen, T. - Souček, Jan
    Statistical analysis of mirror mode waves in sheath regions driven by interplanetary coronal mass ejection.
    Annales Geophysicae. Roč. 36, č. 3 (2018), s. 793-808. ISSN 0992-7689. E-ISSN 1432-0576
    Grant CEP: GA ČR(CZ) GA17-08772S
    Institucionální podpora: RVO:68378289
    Klíčová slova: interplanetary physics * plasma waves and turbulence * solar wind plasma * space plasma physics * waves and instabilities
    Obor OECD: Fluids and plasma physics (including surface physics)
    Impakt faktor: 1.585, rok: 2018
    https://www.ann-geophys.net/36/793/2018/

    We present a comprehensive statistical analysis of mirror mode waves and the properties of their plasma surroundings in sheath regions driven by interplanetary coronal mass ejection (ICME). We have constructed a semi-automated method to identify mirror modes from the magnetic field data. We analyze 91 ICME sheath regions from January 1997 to April 2015 using data from the Wind spacecraft. The results imply that similarly to planetary magnetosheaths, mirror modes are also common structures in ICME sheaths. However, they occur almost exclusively as dip-like structures and in mirror stable plasma. We observe mirror modes throughout the sheath, from the bow shock to the ICME leading edge, but their amplitudes are largest closest to the shock. We also find that the shock strength (measured by Alfven Mach number) is the most important parameter in controlling the occurrence of mirror modes. Our findings suggest that in ICME sheaths the dominant source of free energy for mirror mode generation is the shock compression. We also suggest that mirror modes that are found deeper in the sheath are remnants from earlier times of the sheath evolution, generated also in the vicinity of the shock.
    Trvalý link: http://hdl.handle.net/11104/0293825

     
     
Počet záznamů: 1  

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