Bounded anisotropy fluid model for ion temperatures

A bounded anisotropy fluid model is developed which describes the temperature evolution of a collisionless plasma including the effect of pitch angle scattering due to ion cyclotron waves. The model equations accurately describe the proton temperature evolution in the plasma depletion layer, a magnetosheath regime of decreasing plasma density near the magnetopause. As in double adiabatic theory, changes in T⊥ are driven by changes in flux tube area A (∝ 1/B), while changes in T∥ are driven by changes in field line scale length L. In the bounded anisotropy model, if the proton temperature ratio T⊥/T∥ rises above the value 1 + 0.85 β∥p−0.48 (Anderson et al., 1994), where β∥p is the proton parallel beta, energy is transferred from the perpendicular to parallel temperature until this equation is satisfied. This energy exchange represents the effect of ion cyclotron wave pitch angle scattering, which keeps the plasma state near to marginal stability. Equations of the same form, employing bounded anisotropy expressions appropriate to different species, are also applied to He2+ and to electrons. These equations well describe the evolution of the He2+ but do not describe the evolution of the electron temperature, apparently due to the high electron thermal conduction which the model does not include. These results indicate that an energy exchange term may be incorporated into anisotropic fluid equations to simulate the effect of ion cyclotron wave pitch angle scattering in global fluid equations.

[1]  B. Anderson,et al.  Magnetic pulsations from 0.1 to 4.0 Hz and associated plasma properties in the Earth's subsolar magnetosheath and plasma depletion layer , 1993 .

[2]  Brian J. Anderson,et al.  Magnetic spectral signatures in the Earth's magnetosheath and plasma depletion layer , 1994 .

[3]  S. Gary,et al.  Simulations of ion cyclotron anisotropy instabilities in the terrestrial magnetosheath , 1993 .

[4]  S. Gary,et al.  Ion cyclotron anisotropy instabilities in the magnetosheath: Theory and simulations , 1993 .

[5]  S. Gary,et al.  Kinetic properties of mirror waves in magnetosheath plasmas , 1992 .

[6]  C. Wu MHD FLOW PAST AN OBSTACLE : LARGE-SCALE FLOW IN THE MAGNETOSHEATH , 1992 .

[7]  Perkins,et al.  Fluid moment models for Landau damping with application to the ion-temperature-gradient instability. , 1990, Physical review letters.

[8]  B. Anderson,et al.  Ion anisotropies in the magnetosheath , 1993 .

[9]  Michael Hesse,et al.  MHD modeling of magnetotail instability for anisotropic pressure , 1992 .

[10]  G. Paschmann,et al.  ISEE plasma observations near the subsolar magnetopause , 1978 .

[11]  A. Kantrowitz,et al.  MHD CHARACTERISTICS AND SHOCK WAVES. , 1964 .

[12]  B. Anderson,et al.  Low-frequency magnetic fluctuation spectra in the magnetosheath and plasma depletion layer , 1994 .

[13]  Brian J. Anderson,et al.  Ion anisotropy instabilities in the magnetosheath , 1993 .

[14]  L. Lees Interaction between the solar plasma wind and the geomagnetic cavity , 1964 .

[15]  D. Hunten,et al.  Depletion of solar wind plasma near a planetary boundary , 1976 .

[16]  G. S. Stiles,et al.  Observations of plasma depletion in the magnetosheath at the dayside magnetopause , 1979 .

[17]  G. Paschmann,et al.  Double‐polytropic closure in the magnetosheath , 1993 .

[18]  F. Low,et al.  The Boltzmann equation an d the one-fluid hydromagnetic equations in the absence of particle collisions , 1956, Proceedings of the Royal Society of London. Series A. Mathematical and Physical Sciences.

[19]  G. Paschmann,et al.  The magnetosheath region adjacent to the dayside magnetopause: AMPTE/IRM observations , 1994 .

[20]  B. Anderson,et al.  Electromagnetic ion cyclotron waves in the plasma depletion layer , 1993 .

[21]  C. Russell,et al.  Structure and properties of the subsolar magnetopause for northward IMF: ISEE observations , 1990 .

[22]  G. Paschmann,et al.  Structure of the Dayside Magnetopause for Low Magnetic Shear , 1993 .

[23]  G. Siscoe,et al.  Aerodynamic aspects of the magnetospheric flow , 1964 .

[24]  J. Midgley,et al.  Calculation by a moment technique of the perturbation of the geomagnetic field by the solar wind , 1963 .

[25]  B. Anderson,et al.  He2+ and H+ dynamics in the subsolar magnetosheath and plasma depletion layer , 1991 .

[26]  C. Russell,et al.  Wave properties near the subsolar magnetopause - Pc 1 waves in the sheath transition layer , 1993 .