The spatial development of the low-latitude boundary layer

作者: John R. Manuel , J. C. Samson

DOI: 10.1029/93JA01524

关键词:

摘要: The low-latitude boundary layer (LLBL) comprises a large fraction of the magnetospheric making it potentially important site for transport mass, momentum, and energy from magnetosheath into magnetosphere. We have used an ideal magnetohydrodynamic computer simulation with nonperiodic inflow outflow conditions to investigate processes responsible spatial development 6.4 Earth radii ( RE) long section dayside LLBL. Initializing realistic configuration, slightly modified computational efficiency, leads LLBL which broadens downstream distance thin (0.12 RE thick) laminar broad (∼0.7 turbulent one capable significant transport. Broadening occurs through action Reynolds Maxwell stresses that develop during roll-up merging vortices generated by Kelvin-Helmholtz instability in simulated indicates steep gradients at magnetopause between may further aid encouraging wave-particle diffusion transporting plasma presence flow-aligned component magnetic field, on other hand, can hinder slowing then stopping transfer their rotational kinetic deformations field.

参考文章(71)
N. D. Sandham, W. C. Reynolds, Some Inlet-Plane Effects on the Numerically Simulated Spatially-Developing Mixing Layer Turbulent Shear Flows 6. pp. 441- 454 ,(1989) , 10.1007/978-3-642-73948-4_33
Jay P. Boris, On large eddy simulation using subgrid turbulence models Comment 1 Whither Turbulence? Turbulence at the Crossroads. ,vol. 357, pp. 344- 353 ,(1990) , 10.1007/3-540-52535-1_53
K.-P. Wenzel, P. Daly, T. R. Sanderson, E. J. Smith, Observations of a large-scale vortex-like structure in the deep-tail plasma sheet boundary layer Solar Wind Magnetosphere Coupling. pp. 739- ,(1986) , 10.1007/978-90-277-2303-1_51
D. J. Southwood, Magnetopause Kelvin-Helmholtz instability ESASP. ,vol. 148, pp. 357- 364 ,(1979)
Henry Keith Moffatt, Magnetic field generation in electrically conducting fluids Cambridge Monographs on Mechanics and Applied Mathematics. ,(1978)
W. C. Reynolds, The potential and limitations of direct and large eddy simulations Whither Turbulence? Turbulence at the Crossroads. ,vol. 357, pp. 313- 343 ,(1990) , 10.1007/3-540-52535-1_52
M. Roth, On impulsive penetration of solar wind plasmoids into the geomagnetic field Planetary and Space Science. ,vol. 40, pp. 193- 201 ,(1992) , 10.1016/0032-0633(92)90057-U
W. Horton, T. Tajima, T. Kamimura, Kelvin-Helmholtz instability and vortices in magnetized plasma Physics of Fluids. ,vol. 30, pp. 3485- 3495 ,(1987) , 10.1063/1.866429
N.A. Tsyganenko, A magnetospheric magnetic field model with a warped tail current sheet Planetary and Space Science. ,vol. 37, pp. 5- 20 ,(1989) , 10.1016/0032-0633(89)90066-4