Astronomy and Astrophysics – Astrophysics
Scientific paper
Dec 1976
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976ap%26ss..45..303l&link_type=abstract
Astrophysics and Space Science, vol. 45, Dec. 1976, p. 303-325.
Astronomy and Astrophysics
Astrophysics
16
Boundary Layer Plasmas, Kinetic Theory, Magnetohydrodynamic Stability, Plasma Dynamics, Solar Wind, Boundary Conditions, Magnetic Fields, Magnetohydrodynamic Flow, Maxwell Equation, Self Consistent Fields, Solar Wind Velocity, Vlasov Equations
Scientific paper
A kinetic theory is presented for boundary layers associated with MHD tangential 'discontinuities' in a collisionless magnetized plasma, such as those observed in the solar wind. The theory consists of finding self-consistent solutions of Vlasov's equation and Maxwell's equation for stationary one-dimensional boundary layers separating two Maxwellian plasma states. Layers in which the current is carried by electrons are found to have a thickness of the order of a few electron gyroradii, but the drift speed of the current-carrying electrons is found to exceed the Alfven speed, and accordingly such layers are not stable. Several types of layers in which the current is carried by protons are discussed; in particular, cases are considered in which the magnetic-field intensity, direction, or both, changed across the layer. In every case, the thickness was of the order of a few proton gyroradii, and the field changed smoothly, although the characteristics depended somewhat on the boundary conditions. The drift speed was always less than the Alfven speed, consistent with stability of such structures. These results are consistent with observations of boundary layers in the solar wind near 1 AU.
Burlaga Leonard Francis
Lemaire Joseph
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