Emission of nonlinear whistler waves at the front of perpendicular supercritical shocks:: Hybrid versus full particle simulations

被引:51
作者
Hellinger, Petr [1 ]
Travnicek, Pavel
Lembege, Bertrand
Savoini, Philippe
机构
[1] Acad Sci Czech Republic, Inst Atmospher Phys, Prague, Czech Republic
[2] CNRS, IPSL, UVSQ, Ctr Etud Environm Terrestre & Planetaires, Velizy Villacoublay, France
关键词
D O I
10.1029/2007GL030239
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
New behavior of strictly perpendicular shocks in supercritical regime is analyzed with the help of both two-dimensional (2-D) hybrid and full particle electromagnetic simulations. Surprisingly, in both simulation cases, the shock front region appears to be dominated by emission of coherent large amplitude whistler waves for some plasma conditions and shock regimes. These whistler waves are oblique with respect to the shock normal as well as to the upstream magnetic field and are phase-standing in the shock rest frame. A parametric study shows that these whistler waves are emitted in 2-D perpendicular shocks and, simultaneously, the self-reformation of the shock front associated with reflected ions disappears; the 2-D shock front is almost quasi-stationary. In contrast, both corresponding one-dimensional (1-D) hybrid and full particle simulations performed in similar plasma and Mach regime conditions show that the self-reformation takes place for 1-D perpendicular shock. These results indicate that the emission of these 2-D whistler waves can inhibit the self-reformation in 2-D shocks. Possible generating mechanisms of these waves emissions and comparison with previous works are discussed.
引用
收藏
页数:5
相关论文
共 23 条
  • [1] Experimental determination of the dispersion of waves observed upstream of a quasi-perpendicular shock
    Balikhin, MA
    deWit, TD
    Alleyne, HSK
    Wolliscroft, LJC
    Walker, SN
    Krasnoselskikh, V
    MierJedrzejeowicz, WAC
    Baumjohann, W
    [J]. GEOPHYSICAL RESEARCH LETTERS, 1997, 24 (07) : 787 - 790
  • [2] Shock front nonstationarity of supercritical perpendicular shocks -: art. no. 1233
    Hada, T
    Oonishi, M
    Lembège, B
    Savoini, P
    [J]. JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2003, 108 (A6)
  • [3] Reformation of perpendicular shocks:: Hybrid simulations -: art. no. 2234
    Hellinger, P
    Trávnícek, P
    Matsumoto, H
    [J]. GEOPHYSICAL RESEARCH LETTERS, 2002, 29 (24)
  • [4] Whistler waves in 3D hybrid simulations of quasiperpendicular shocks
    Hellinger, P
    Mangeney, A
    Matthews, A
    [J]. GEOPHYSICAL RESEARCH LETTERS, 1996, 23 (06) : 621 - 624
  • [5] Structure and stationarity of quasi-perpendicular shocks: Numerical simulations
    Hellinger, P
    [J]. PLANETARY AND SPACE SCIENCE, 2003, 51 (11) : 649 - 657
  • [6] Upstream whistlers generated by protons reflected from a quasi-perpendicular shock
    Hellinger, P
    Mangeney, A
    [J]. JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1997, 102 (A5): : 9809 - 9819
  • [7] Nonstationarity of strong collisionless quasiperpendicular shocks:: Theory and full particle numerical simulations
    Krasnoselskikh, VV
    Lembège, B
    Savoini, P
    Lobzin, VV
    [J]. PHYSICS OF PLASMAS, 2002, 9 (04) : 1192 - 1209
  • [8] KRASNOSELSKIKH VV, 1991, ADV SPACE RES-SERIES, V11, P15, DOI 10.1016/0273-1177(91)90002-2
  • [9] KRAUSSVARBAN D, 1995, GEOPHYS RES LETT, V26, P2091
  • [10] Numerical simulations of local shock reformation and ion acceleration in supernova remnants
    Lee, RE
    Chapman, SC
    Dendy, RO
    [J]. ASTROPHYSICAL JOURNAL, 2004, 604 (01) : 187 - 195