Effect of the radial boundary condition on Alfvén wave dynamics in reduced magnetohydrodynamics

The effects of different boundary conditions on Alfven wave dynamics in reduced magnetohydrodynamics are described. If one assumes that the derivative or the second derivative of the electrostatic potential Φ is zero at one of the radial (across the magnetic field) boundaries, radially localized (guided) Alfven wave solutions are possible, but if Φ is set to zero (grounded) at both boundaries, the solutions consistent with the boundary condition exhibit radial propagation of energy. To confirm the ideas discussed, numerical tests were done in slab geometry with a density gradient across the magnetic field.

[1]  T. Tajima,et al.  Book Review: Plasma physics via computer simulation. C.K. Birdsall and A.B. Langdon, McGraw-Hill, New York, 1985. xxiii + 479 pages. US $45 , 1986 .

[2]  Robert Rankin,et al.  Spatiotemporal characteristics of ultra-low frequency dispersive scale shear Alfvén waves in the Earth’s magnetosphere , 2004 .

[3]  R. Lysak,et al.  An MHD simulation study of the poloidal mode field line resonance in the Earth's dipole magnetosphere , 1995 .

[4]  William Lotko,et al.  Small‐scale electric fields in downward auroral current channels , 2003 .

[5]  R. Ergun,et al.  Auroral ion acceleration in dispersive Alfvén waves , 2004 .

[6]  Dong-Hun Lee,et al.  Effects of ionospheric damping on MHD wave mode structure , 2004 .

[7]  Alain J. Brizard Energy-conserving finite-β electromagnetic drift-fluid equations , 2005 .

[8]  A. Streltsov,et al.  Discrete auroral arc, electrostatic shock and suprathermal electrons powered by dispersive, anomalously resistive field line resonance , 1998 .

[9]  A. Streltsov,et al.  Small‐scale, “electrostatic” auroral structures and Alfvén waves , 1999 .

[10]  Hiroshi Matsumoto,et al.  Computer Simulation of Space Plasmas , 1985 .

[11]  C. Birdsall,et al.  Plasma Physics via Computer Simulation , 2018 .

[12]  A. Streltsov,et al.  Ultra‐low‐frequency electrodynamics of the magnetosphere‐ionosphere interaction , 2005 .

[13]  D. Winske,et al.  A nonspecialist's guide to kinetic simulations of space plasmas , 1996 .

[14]  Robert L. Lysak,et al.  Magnetospheric ULF Waves: Synthesis and New Directions , 2006 .

[15]  D. Southwood Some features of field line resonances in the magnetosphere , 1974 .

[16]  C. Meister Cross, R., An introduction to Alfven waves; Bristol [u.a.], Hilger, 1988 , 1995 .

[17]  A. Streltsov,et al.  Coupling between density structures, electromagnetic waves and ionospheric feedback in the auroral zone , 2008 .

[18]  佐藤 哲也,et al.  Computer simulation of space plasmas , 1985 .

[19]  Dong-Hun Lee,et al.  Quantitative test of the cavity resonance explanation of plasmaspheric Pi2 frequencies , 2002 .

[20]  Toshiki Tajima,et al.  Computational Plasma Physics: With Applications To Fusion And Astrophysics , 2019 .

[21]  C. Chaston ULF Waves and Auroral Electrons , 2013 .