Nonstationarity of two-dimensional supercrititical perpendicular shocks: evidence of competing mechanims

Details Nonstationarity of two-dimensional supercrititical perpendicular shocks: evidence of competing mechanims Nonstationarity of two-dimensional supercrititical perpendicular shocks: evidence of competing mechanims

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008agufmsm51a1616l&link_type=abstract

American Geophysical Union, Fall Meeting 2008, abstract #SM51A-1616

Physics

2154 Planetary Bow Shocks, 2159 Plasma Waves And Turbulence, 4455 Nonlinear Waves, Shock Waves, Solitons (0689, 2487, 3280, 3285, 4275, 6934, 7851, 7852), 7851 Shock Waves (4455)

Scientific paper

Two-dimensional (2-D) full particle electromagnetic simulations are used for analysing in detail different nonstationary behaviors of perpendicular supercritical shocks. A recent study (Hellinger et al., 2007) has evidenced that the shock front is dominated by the emission of coherent large amplitude whistler waves for some plasma conditions and shock regimes. These whistler waves are emitted in two-dimensional perpendicular shocks and inhibit the self-reformation driven by the accumulation of reflected ions: then, the shock front appears almost "quasi-stationary", a result which could seem in apparent contradiction with previous results. The present study allows to clarify the situation by bringing new complementary results: (i) there exists a transition regime around a critical Mach number threshold Mwwe, within which both self- reformation and whistler waves emission can co-exist. (ii) Below (above) this threshold regime, the self- reformation (whistler waves emission) is fully retrieved and becomes dominant. (iii) As MA is larger than Mwwe, , this shock front looks "quasi-stationary" in 1-D y-averaged fields profiles, but in fact is nonstationary in full 2-D profiles and over a smaller time scale (lower than one ion gyroperiod). Moreover, this nonstationarity is characterized by a quasi-periodic reinforcement of nonlinear waves emission from the ramp. This effect results from the fact that the emission of nonlinear whistler waves varies in time according to the local need for balancing the nonlinear effects at the shock ramp (steepening). (iv) These results are observed for a strictly perpendicular shock, as B0 is within the simulation plane; in contrast, as B0 is perpendicular to the simulation plane, no whistler waves emission is evidenced even for large Mach number; only self-reformation is observed. Present results, even if unexpected, are shown to be not in disagreement with previous 2-D PIC and 2-D hybrid simulations these are compared with.

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