Wavelength and decay length of density overshoot structure in supercritical, collisionless bow shocks

Above some critical Mach number, quasiperpendicular collisionless shocks are known to exhibit “overshoot” and “undershoot” structure thought to be associated with the motion of ions trapped at the shock front. Using spacecraft potential data from the Cluster spacecraft, the overshoot/undershoot density structure at 56 crossings of the quasiperpendicular bow shock is studied. The envelope of the absolute value of the density, in most cases, decays exponentially and these envelopes are fitted to a decaying function from which we calculate the decay length scale. The overshoot/undershoot wavelength is also estimated using the zero crossings of the density profile and a good correlation between the average wavelength and the convected ion gyroradius is found: the wavelength is approximately two to three times the ion gyroradius. There is no evidence of a strong correlation between the wavelength and the ion inertial length. Similar results are found for the decay length, which also seems to be ordered by the ...

[1]  T. Horbury,et al.  Density-transition scale at quasiperpendicular collisionless shocks. , 2003, Physical review letters.

[2]  M. Gedalin,et al.  Role of overshoots in the formation of the downstream distribution of adiabatic electrons , 1999 .

[3]  Mario H. Acuna,et al.  THE CLUSTER MAGNETIC FIELD INVESTIGATION , 1997 .

[4]  J. Rouzaud,et al.  THE CLUSTER ION SPECTROMETRY (CIS) EXPERIMENT , 1997 .

[5]  Per-Arne Lindqvist,et al.  THE ELECTRIC FIELD AND WAVE EXPERIMENT FOR THE CLUSTER MISSION , 1997 .

[6]  Norbert Sckopke,et al.  Ion heating at the Earth's quasi-perpendicular bow shock , 1995 .

[7]  T. Armstrong,et al.  Effect of magnetic overshoot on shock drift acceleration , 1991 .

[8]  M. Mellott,et al.  Shock overshoots revisited , 1987 .

[9]  C. Kennel,et al.  A parametric survey of the first critical Mach number for a fast MHD shock , 1984, Journal of Plasma Physics.

[10]  V. Eselevich On the nature of “overshoot” in a collisionless shock , 1984 .

[11]  K. Papadopoulos,et al.  Microinstabilities associated with a high Mach number, perpendicular bow shock , 1984 .

[12]  C. Russell,et al.  Evolution of ion distributions across the nearly perpendicular bow shock: Specularly and non‐specularly reflected‐gyrating ions , 1983 .

[13]  K. Papadopoulos,et al.  A source of the backstreaming ion beams in the foreshock region , 1983 .

[14]  C. Russell,et al.  ISEE-1 and -2 observations of magnetic field strength overshoots in quasi-perpendicular bow shocks , 1982 .

[15]  Charles C. Goodrich,et al.  The structure of perpendicular bow shocks , 1982 .

[16]  C. Russell,et al.  Overshoots in planetary bow shocks , 1982, Nature.

[17]  Charles C. Goodrich,et al.  Simulation of a perpendicular bow shock , 1981 .