Alfvén Waves and Turbulence in the Solar Atmosphere and Solar Wind
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[1] John V. Shebalin,et al. Anisotropy in MHD turbulence due to a mean magnetic field , 1983, Journal of Plasma Physics.
[2] L. C. Woods. Physics of plasmas , 2003 .
[3] October I. Physical Review Letters , 2022 .
[4] M. Heinemann,et al. Non‐WKB Alfvén waves in the solar wind , 1980 .
[5] J. Hollweg,et al. Alfvén waves in the solar atmosphere , 1978 .
[6] W. Matthaeus,et al. Dynamical age of solar wind turbulence in the outer heliosphere , 1998 .
[7] M. Velli,et al. Propagation and dissipation of Alfvén waves in stellar atmospheres permeated by isothermal winds , 2005 .
[8] S. Cranmer,et al. On the Generation, Propagation, and Reflection of Alfvén Waves from the Solar Photosphere to the Distant Heliosphere , 2004, astro-ph/0410639.
[9] Z. Pu,et al. The power spectrum of interplanetary Alfvénic fluctuations: Derivation of the governing equation and its solution , 1984 .
[10] M. Velli,et al. Turbulent cascade of incompressible unidirectional Alfvén waves in the interplanetary medium. , 1989, Physical review letters.
[11] P. Dmitruk,et al. Reduced magnetohydrodynamics and parallel spectral transfer , 2004 .
[12] L. Milano,et al. Conditions for sustainment of magnetohydrodynamic turbulence driven by Alfvén waves , 2001 .
[13] B. Bavassano,et al. Alfvénic turbulence in the polar wind: A statistical study on cross helicity and residual energy variations , 2000 .
[14] P. Dmitruk,et al. Low-Frequency Waves and Turbulence in an Open Magnetic Region: Timescales and Heating Efficiency , 2003 .
[15] C. Tu. The damping of interplanetary Alfvénic fluctuations and the heating of the solar wind , 1988 .
[16] Marco Velli,et al. Parametric decay of circularly polarized Alfvén waves: Multidimensional simulations in periodic and open domains , 2001 .
[17] W. Matthaeus,et al. Transport and turbulence modeling of solar wind fluctuations , 1990 .
[18] P. Dmitruk,et al. Coronal Heating by Magnetohydrodynamic Turbulence Driven by Reflected Low-Frequency Waves , 1999 .
[19] J. Hollweg,et al. Heating and cooling of protons by turbulence-driven ion cyclotron waves in the fast solar wind , 1999 .
[20] L. Milano,et al. Coronal Heating Distribution Due to Low-Frequency, Wave-driven Turbulence , 2002, astro-ph/0204347.
[21] Louis J. Lanzerotti,et al. Discrete modes and turbulence in a wave‐driven strongly magnetized plasma , 2004 .
[22] Shadia Rifai Habbal,et al. Flow properties of the solar wind derived from a two-fluid model with constraints from white light and in situ interplanetary observations , 1995 .
[23] W. Matthaeus,et al. Turbulent generation of outward-traveling interplanetary Alfvenic fluctuations , 1983 .
[24] P. Similon,et al. Alfven wave transmission through the solar atmosphere , 1992 .
[25] L. Milano,et al. A Reduced Magnetohydrodynamic Model of Coronal Heating in Open Magnetic Regions Driven by Reflected Low-Frequency Alfvén Waves , 2001 .
[26] Eric Ronald Priest,et al. Advances in solar system magnetohydrodynamics , 1991 .
[27] S. Fineschi,et al. Plasma Properties in Coronal Holes Derived from Measurements of Minor Ion Spectral Lines and Polarized White Light Intensity , 1998 .
[28] L. Milano,et al. Wave-driven Turbulent Coronal Heating in Open Field Line Regions: Nonlinear Phenomenological Model , 2001 .
[29] M. Velli,et al. Waves from the sun , 1991 .
[30] Pierluigi Veltri,et al. Fully developed anisotropic hydromagnetic turbulence in interplanetary space , 1980 .
[31] W. Matthaeus,et al. Non-WKB evolution of solar wind fluctuations - A turbulence modeling approach , 1989 .
[32] M. Velli,et al. Coronal plumes and the expansion of pressure-balanced structures in the fast solar wind , 1999 .
[33] L. Ofman,et al. Estimating random transverse velocities in the fast solar wind from EISCAT Interplanetary Scintillation measurements , 2002 .
[34] W. Matthaeus,et al. Radial evolution of cross helicity in high‐latitude solar wind , 2005 .
[35] D. Galloway,et al. Alfvén waves in the solar atmosphere , 1982 .
[36] J. Richardson,et al. Heating of the low‐latitude solar wind by dissipation of turbulent magnetic fluctuations , 2001 .
[37] S. Inutsuka,et al. Making the Corona and the Fast Solar Wind: A Self-consistent Simulation for the Low-Frequency Alfvén Waves from the Photosphere to 0.3 AU , 2005, astro-ph/0506639.
[38] Alyson G. Wilson. Fifth SOHO Workshop: The Corona and Solar Wind Near Minimum Activity , 1997 .
[39] T. Holzer,et al. Dynamics of coronal hole regions , 1976 .
[40] W. Matthaeus,et al. Evolution of turbulent magnetic fluctuation power with heliospheric distance , 1996 .
[41] W. Matthaeus,et al. Transport theory and the WKB approximation for interplanetary MHD fluctuations , 1994 .
[42] B. Bavassano,et al. On the evolution of outward and inward Alfvénic fluctuations in the polar wind , 2000 .
[43] J. Hollweg,et al. Alfvn waves in the solar atmosphere: II: Open and closed magnetic flux tubes , 1981 .
[44] B. Jackson,et al. Physical properties of a polar coronal hole from 2 to 5 solar radii , 1977 .