Dr. Sean Oughton
Department of Mathematics
University of Waikato

Click here to see all papers available to download [organised by topic]

Publications and Preprints

oughton
[1] Matthaeus WH, Stribling WT, Martínez D, Oughton S, and Montgomery D.
Decaying, two-dimensional, Navier-Stokes turbulence at very long times.
Physica D 51:531-538 (1991).
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[2] Matthaeus WH, Stribling WT, Martínez D, Oughton S, and Montgomery D.
Selective decay and coherent vortices in two-dimensional incompressible turbulence.
Phys. Rev. Lett. 66:2731-2734, doi:10.1103/PhysRevLett.66.2731 (1991).
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[3] Zank GP, Oughton S, Neubauer FM, and Webb GM.
Mass-loading and parallel magnetized shocks.
Geophys. Res. Lett. 18:1809-1812 (1991).
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[4] Zank GP and Oughton S.
Properties of mass-loading shocks 1. Hydrodynamic considerations.
J. Geophys. Res. 96:9439-9453 (1991).
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[5] Matthaeus WH, Zhou Y, Oughton S, and Zank GP.
Weakly inhomogeneous MHD turbulence and transport of solar wind fluctuations.
In Proceedings of Solar Wind 7, COSPAR Colloq. Ser. (eds. E Marsch and R Schwenn), vol. 3, pp. 511-514. Pergamon, Oxford, UK (1992).
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[6] Montgomery DC, Matthaeus WH, Stribling WT, Martínez D, and Oughton S.
Relaxation in two dimensions and the “sinh-Poisson” equation.
Phys. Fluids A 4:3-6, doi:10.1063/1.858525 (1992).
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[7] Oughton S and Matthaeus WH.
Evolution of solar wind fluctuations and the influence of turbulent `mixing'.
In Proceedings of Solar Wind 7, COSPAR Colloq. Ser. (eds. E Marsch and R Schwenn), vol. 3, pp. 523-526. Pergamon, Oxford, UK (1992).
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[8] Zank GP, Oughton S, Neubauer FM, and Webb GM.
Properties of mass-loading shocks 2. Magnetohydrodynamics.
J. Geophys. Res. 97:17051-17074 (1992).
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[9] Oughton S. Transport of Solar Wind Fluctuations: A Turbulence Approach. Ph.D. thesis, University of Delaware, Newark, Delaware, 19716 (1993).
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[10] Matthaeus WH, Oughton S, Pontius D, and Zhou Y.
Evolution of energy containing turbulent eddies in the solar wind.
J. Geophys. Res. 99:19267-19287 (1994).
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[11] Matthaeus WH, Zhou Y, Zank GP, and Oughton S.
Transport theory and the WKB approximation for interplanetary MHD fluctuations.
J. Geophys. Res. 99:23421-23430 (1994).
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[12] Oughton S, Matthaeus WH, and Priest ER.
3D MHD turbulence with a mean magnetic field.
In Current Topics in Astrophysical and Fusion Plasma Research, Proceedings of the IWWPP, Pichl, Austria (1994) (eds. M Heyn, W Kernbichler, and HK Biernat), pp. 81-86. dbv-Verlag Graz (1994).
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[13] Oughton S, Priest ER, and Matthaeus WH.
The influence of a mean magnetic field on three-dimensional MHD turbulence.
J. Fluid Mech. 280:95-117, doi:10.1017/S0022112094002867 (1994).
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[14] Hossain M, Gray PC, Pontius Jr. DH, Matthaeus WH, and Oughton S.
Phenomenology for the decay of energy-containing eddies in homogeneous MHD turbulence.
Phys. Fluids 7:2886-2904, doi:10.1063/1.868665 (1995).
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[15] Matthaeus WH, Oughton S, Pontius D, and Zhou Y.
Reply to comment by C.-Y. Tu and E. Marsch on “Evolution of energy-containing turbulent eddies in the solar wind”.
J. Geophys. Res. 100:12329-12333 (1995).
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[16] Oughton S, Matthaeus WH, and Ghosh S.
Anisotropy in incompressible and compressible 3D MHD turbulence.
In Small-Scale Structures in Three-Dimensional Hydro and Magnetohydrodynamic Turbulence (eds. M Meneguzzi, A Pouquet, and PL Sulem), vol. 462 (Lecture Notes in Physics), pp. 273-279. Springer-Verlag (1995).
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[17] Oughton S and Matthaeus WH.
Linear transport of solar wind fluctuations.
J. Geophys. Res. 100:14783-14799 (1995).
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[18] Stribling T, Matthaeus WH, and Oughton S.
Magnetic helicity in magnetohydrodynamic turbulence with a mean magnetic field.
Phys. Plasmas 2:1437-1452, doi:10.1063/1.871359 (1995).
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[19] Hossain M, Gray PC, Pontius Jr. DH, Matthaeus WH, and Oughton S.
Is the Alfvén wave propagation effect important for energy decay in homogeneous MHD turbulence? In Solar Wind Eight (eds. D Winterhalter, JT Gosling, SR Habbal, WS Kurth, and M Neugebauer), pp. 358-361. AIP, New York (1996).
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[20] Matthaeus WH, Zank GP, and Oughton S.
Phenomenology of hydromagnetic turbulence in a uniformly expanding medium.
J. Plasma Phys. 56:659-675 (1996).
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[21] Matthaeus WH, Ghosh S, Oughton S, and Roberts DA.
Anisotropic three-dimensional MHD turbulence.
J. Geophys. Res. 101:7619-7629, doi:10.1029/95JA03830 (1996).
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[22] Oughton S.
Ion parallel viscosity and anisotropy in MHD turbulence.
J. Plasma Phys. 56:641-657 (1996).
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[23] Oughton S.
Energy dynamics in linear MHD with ion parallel viscosity.
J. Plasma Phys. 58:571-576, doi:10.1017/S0022377897005928 (1997).
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[24] Oughton S, Rädler KH, and Matthaeus WH.
General second-rank correlation tensors for homogeneous magnetohydrodynamic turbulence.
Phys. Rev. E 56:2875-2888, doi:10.1103/PhysRevE.56.2875 (1997).
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[25] Matthaeus WH, Smith CW, and Oughton S.
Dynamical age of solar wind turbulence in the outer heliosphere.
J. Geophys. Res. 103:6495-6502, doi:10.1029/97JA03729 (1998).
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[26] Matthaeus WH, Oughton S, Ghosh S, and Hossain M.
Scaling of anisotropy in hydromagnetic turbulence.
Phys. Rev. Lett. 81:2056-2059, doi:10.1103/PhysRevLett.81.2056 (1998).
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[27] Oughton S, Matthaeus WH, and Ghosh S.
Anisotropy and energy decay in magnetohydrodynamic turbulence: Theory and solar wind observations.
In Advances in Turbulence VII (ed. U Frisch), pp. 475-478. Kluwer, Dordrecht (1998).
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[28] Oughton S, Matthaeus WH, and Ghosh S.
Scaling of spectral anisotropy with magnetic field strength in decaying MHD turbulence.
Phys. Plasmas 5:4235-4242, doi:10.1063/1.873159 (1998).
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[29] Matthaeus WH, Zank GP, and Oughton S.
Coronal heating by quasi-2D MHD turbulence driven by non-WKB wave reflection.
In Solar Wind Nine (eds. S Habbal, R Esser, JV Hollweg, and PA Isenberg), vol. 471, pp. 361-364. AIP, Woodbury, NY (1999).
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[30] Matthaeus WH, Zank GP, Leamon RJ, Smith CW, Mullan DJ, and Oughton S.
Fluctuations, dissipation and heating in the corona.
Space Sci. Rev. 87:269-275 (1999). Proc. of the 7th SoHO Workshop.
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[31] Matthaeus WH, Zank GP, Smith CW, and Oughton S.
Turbulence, spatial transport, and heating of the solar wind.
Phys. Rev. Lett. 82:3444-3447, doi:10.1103/PhysRevLett.82.3444 (1999).
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[32] Matthaeus WH, Zank GP, Oughton S, Mullan DJ, and Dmitruk P.
Coronal heating by MHD turbulence driven by reflected low-frequency waves.
Astrophys. J. 523:L93-L96 (1999).
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[33] Oughton S, Matthaeus WH, and Smith CW.
Measurement of spectral anisotropy using single spacecraft data.
In Solar Wind Nine (eds. S Habbal, R Esser, JV Hollweg, and PA Isenberg), vol. 471, pp. 507-510. AIP, Woodbury, NY (1999).
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[34] Oughton S, Matthaeus WH, Zank GP, and Mullan DJ.
Coronal heating via Alfvén waves and 2D MHD turbulence.
In Proc. of the 8th SoHO Workshop `Plasma Dynamics and Diagnostics in the Solar Transition Region and Corona' (eds. JC Vial and B Kaldeich-Schürmann), vol. ESA SP-446, pp. 525-530. ESA, Noordwijk, The Netherlands (1999).
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[35] Smith CW, Zank GP, Matthaeus WH, and Oughton S.
Heating of the solar wind beyond 1 AU by turbulent dissipation.
In Proceedings of the 26th ICRC (eds. D Kieda, M Salanov, and B Dingus), vol. 7, pp. 480-483 (1999).
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[36] Zank GP, Matthaeus WH, Smith CW, and Oughton S.
Heating of the solar wind beyond 1AU by turbulent dissipation.
In Solar Wind Nine (eds. S Habbal, R Esser, JV Hollweg, and PA Isenberg), vol. 471, pp. 523-526. AIP, Woodbury, NY (1999).
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[37] Leamon RJ, Matthaeus WH, Smith CW, Zank GP, Mullan DJ, and Oughton S.
MHD-driven kinetic dissipation in the solar wind and corona.
Astrophys. J. 537:1054-1062, doi:10.1086/309059 (2000).
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[38] Oughton S and Prandi R.
Kinetic helicity and MHD turbulence.
J. Plasma Phys. 64:179-193 (2000).
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[39] Dmitruk P, Matthaeus WH, Milano LJ, and Oughton S.
Conditions for sustainment of magnetohydrodynamic turbulence driven by Alfvén waves.
Phys. Plasmas 8:2377-2384, doi:10.1063/1.1344563 (2001).
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[40] Oughton S, Matthaeus WH, Dmitruk P, Milano LM, Zank GP, and Mullan DJ.
A reduced magnetohydrodynamic model of coronal heating in open magnetic regions driven by reflected low-frequency Alfvén waves.
Astrophys. J. 551:565-575, doi:10.1086/320069 (2001).
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[41] Smith CW, Matthaeus WH, Zank GP, Ness NF, Oughton S, and Richardson JD.
Heating of the low-latitude solar wind by dissipation of turbulent magnetic fluctuations.
J. Geophys. Res. 106:8253-8272 (2001).
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[42] Watkins NW, Oughton S, and Freeman MP.
What can we infer about the underlying physics from burst distributions observed in an RMHD simulation? Planet. Space Sci. 49:1233-1237 (2001).
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[43] Chapman S, Freeman M, and Oughton S.
Complexity in astroplasmas.
Astronomy and Geophysics 42:22-2 (2001).
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[44] Dmitruk P, Matthaeus WH, Milano LJ, Oughton S, Zank GP, and Mullan DJ.
Coronal heating distribution due to low-frequency, wave-driven turbulence.
Astrophys. J. 575:571-577, doi:10.1086/341188 (2002).
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[45] Matthaeus WH, Mullan DJ, Dmitruk P, Milano L, and Oughton S.
MHD turbulence and heating of the open field line solar corona.
Nonlin. Process. Geophys. 10:93-100, doi:10.5194/npg-10-93-2003 (2003).
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[46] Matthaeus WH, Dmitruk P, Smith D, Ghosh S, and Oughton S.
Impact of Hall effect on energy decay in magnetohydrodynamic turbulence.
Geophys. Res. Lett. 30:2104, doi:10.1029/2003GL017949 (2003).
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[47] Matthaeus WH, Dmitruk P, Oughton S, and Mullan D.
Turbulent dissipation in the solar wind and corona.
In Solar Wind Ten (eds. M Velli, R Bruno, and F Malara), vol. 679, pp. 427-432. AIP, Melville, NY (2003).
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[48] Milano L, Matthaeus WH, Dmitruk P, and Oughton S.
Coronal MHD transport theory and phenomenology.
In Solar Wind Ten (eds. M Velli, R Bruno, and F Malara), vol. 679, pp. 343-346. AIP, Melville, NY (2003).
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[49] Oughton S.
Solar wind fluctuations: Waves and turbulence.
In Solar Wind Ten (eds. M Velli, R Bruno, and F Malara), vol. 679, pp. 421-426. AIP, Melville, NY (2003), doi:10.1063/1.1618626.
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[50] Oughton S, Dmitruk P, and Matthaeus WH.
Coronal heating and reduced MHD.
In Turbulence and Magnetic Fields in Astrophysics (eds. E Falgarone and T Passot), vol. 614 (LNP), pp. 28-55. Springer (2003).
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[51] Matthaeus WH, Minnie J, Breech B, Parhi S, Bieber JW, and Oughton S.
Transport of cross helicity and the radial evolution of Alfvénicity in the solar wind.
Geophys. Res. Lett. 31:L12803, doi:10.1029/2004GL019645 (2004).
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[52] Oughton S, Dmitruk P, and Matthaeus WH.
Reduced magnetohydrodynamics and parallel spectral transfer.
Phys. Plasmas 11:2214-2225, doi:10.1063/1.1705652 (2004).
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[53] Smith CW, Isenberg PA, Matthaeus WH, Richardson JD, Oughton S, and Zank GP.
Heating the outer heliosphere by pickup protons.
In Physics of the Outer Heliosphere, vol. 719 of AIP Conf. Proc., pp. 359-364 (2004).
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[54] Verdini A, Velli M, and Oughton S.
Nonlinear evolution of a turbulent spectrum of outwardly propagating Alfvén waves in solar and stellar coronae.
In Proc. of the SoHO 15 Workshop: Coronal Heating (ed. D Danesy), vol. SP-575, pp. 454-459. ESA, Noordwijk, The Netherlands (2004).
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[55] Breech B, Matthaeus WH, Minnie J, Oughton S, Parhi S, Bieber JW, and Bavassano B.
Radial evolution of cross helicity in high-latitude solar wind.
Geophys. Res. Lett. 32:L06103, doi:10.1029/2004GL022321 (2005).
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[56] Breech B, Matthaeus WH, Minnie J, Oughton S, Parhi S, Bieber JW, and Bavassano B.
Radial evolution of cross helicity at low and high latitudes in the solar wind.
In Proc. Solar Wind 11 - Soho 16 “Connecting Sun and Heliosphere” (eds. B Fleck, T Zurbuchen, and H Lacoste), vol. SP-592, pp. 597-600. ESA, Noordwijk, The Netherlands (2005).
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[57] Dmitruk P, Matthaeus WH, and Oughton S.
Direct comparisons of compressible magnetohydrodynamics and reduced magnetohydrodynamics turbulence.
Phys. Plasmas 12:112304, doi:10.1063/1.2128573 (2005).
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[58] Horbury T, Forman MA, and Oughton S.
Spacecraft observations of solar wind turbulence: An overview.
Plasma Phys. Controlled Fusion 47:B703-B717, doi:10.1088/0741-3335/47/12B/S52 (2005).
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[59] Oughton S and Matthaeus WH.
Parallel and perpendicular cascades in solar wind turbulence.
Nonlin. Process. Geophys. 12:299-310, doi:10.5194/npg-12-299-2005 (2005).
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[60] Oughton S, Dmitruk P, and Matthaeus WH.
A two-component phenomenology for the evolution of MHD turbulence.
In Proc. Solar Wind 11 - Soho 16 “Connecting Sun and Heliosphere” (eds. B Fleck, T Zurbuchen, and H Lacoste), vol. SP-592, pp. 633-636. ESA, Noordwijk, The Netherlands (2005).
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[61] Verdini A, Velli M, and Oughton S.
Nonlinear evolution of Alfvén waves in the solar atmosphere.
In Proc. Solar Wind 11 - Soho 16 “Connecting Sun and Heliosphere” (eds. B Fleck, T Zurbuchen, and H Lacoste), vol. SP-592, pp. 567-570. ESA, Noordwijk, The Netherlands (2005).
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[62] Verdini A, Velli M, and Oughton S.
Propagation and dissipation of Alfvén waves in stellar atmospheres permeated by isothermal winds.
Astron. Astrophys. 444:233-244, doi:10.1051/0004-6361:20052748 (2005).
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[63] Oughton S, Matthaeus WH, and Dmitruk P.
A two-component phenomenology for homogeneous magnetohydrodynamic turbulence.
Phys. Plasmas 13:042306, doi:10.1063/1.2188088 (2006).
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[64] Verdini A, Dmitruk P, Matthaeus WH, Oughton S, and Velli M.
A turbulence model for acceleration of the high latitude fast solar wind.
In SOHO-17. 10 Years of SOHO and Beyond (ed. H Lacoste), vol. SP-617. ESA, Noordwijk, The Netherlands (2006).
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[65] Watson PG, Oughton S, and Craig IJD.
The impact of small-scale turbulence on laminar magnetic reconnection.
Phys. Plasmas 14:032301, doi:10.1063/1.2458595 (2007).
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[66] Breech B, Matthaeus WH, Minnie J, Bieber JW, Oughton S, Smith CW, and Isenberg PA.
Turbulence transport throughout the heliosphere.
J. Geophys. Res. 113:A08105, doi:10.1029/2007JA012711 (2008).
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[67] Horbury TS, Forman M, and Oughton S.
Anisotropic scaling of magnetohydrodynamic turbulence.
Phys. Rev. Lett. 101:175005, doi:10.1103/PhysRevLett.101.175005 (2008).
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[68] Breech B, Matthaeus WH, Cranmer SR, Kasper JC, and Oughton S.
Electron and proton heating by solar wind turbulence.
J. Geophys. Res. 114:A09103, doi:10.1029/2009JA014354 (2009).
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[69] Matthaeus WH, Oughton S, and Zhou Y.
Anisotropic magnetohydrodynamic spectral transfer in the diffusion approximation.
Phys. Rev. E 79:035401, doi:10.1103/PhysRevE.79.035401 (2009).
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[70] Wan M, Oughton S, Servidio S, and Matthaeus WH.
Generation of non-Gaussian statistics and coherent structures in ideal MHD.
Phys. Plasmas 16:080703, doi:10.1063/1.3206949 (2009).
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[71] Wan M, Servidio S, Oughton S, and Matthaeus WH.
The third-order law for increments in magnetohydrodynamic turbulence with constant shear.
Phys. Plasmas 16:090703, doi:10.1063/1.3240333 (2009).
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[72] Breech B, Cranmer SR, Matthaeus WH, Kasper JC, and Oughton S.
Heating of the solar wind with electron and proton effects.
In Twelfth International Solar Wind Conference (eds. M Maksimovic, K Issautier, N Meyer-Vernet, M Moncuquet, and F Pantellini), vol. CP1216, pp. 214-217. AIP, Melville, New York (2010).
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[73] Greco A, Matthaeus WH, Servidio S, Dmitruk P, Wan M, Oughton S, and Chuychai P.
Statistical properties of solar wind discontinuities, intermittent turbulence, and rapid emergence of non-Gaussian distributions.
In Twelfth International Solar Wind Conference (eds. M Maksimovic, K Issautier, N Meyer-Vernet, M Moncuquet, and F Pantellini), vol. CP1216, pp. 202-205. AIP, Melville, New York (2010).
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[74] Isenberg PA, Oughton S, Smith CW, and Matthaeus WH.
Solar wind turbulent heating by interstellar pickup protons: 2-component model.
In 9th Annual International Astrophysics Conference: Pickup Ions Throughout the Heliosphere and Beyond (eds. J le Roux, GP Zank, AJ Coates, and V Florinski), vol. 1302, pp. 180-185. AIP (2010), doi:10.1063/1.3529967.
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[75] Oughton S, Matthaeus WH, Smith CW, and Breech B.
A two-component transport model for solar wind fluctuations: Waves plus quasi-2d turbulence.
In Twelfth International Solar Wind Conference (eds. M Maksimovic, K Issautier, N Meyer-Vernet, M Moncuquet, and F Pantellini), vol. CP1216, pp. 210-213. AIP, Melville, New York (2010).
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[76] Verdini A, Velli M, Matthaeus WH, Oughton S, and Dmitruk P.
A turbulence-driven model for heating and acceleration of the fast wind in coronal holes.
Astrophys. J. 708:L116-L120, doi:10.1088/2041-8205/708/2/L116 (2010).
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[77] Wan M, Servidio S, Oughton S, and Matthaeus WH.
The third-order law for magnetohydrodynamic turbulence with shear: Numerical investigation.
Phys. Plasmas 17:052307, doi:10.1063/1.3398481 (2010).
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[78] Wan M, Oughton S, Servidio S, and Matthaeus WH.
The third-order law for magnetohydrodynamic turbulence with constant shear.
In Twelfth International Solar Wind Conference (eds. M Maksimovic, K Issautier, N Meyer-Vernet, M Moncuquet, and F Pantellini), vol. CP1216, pp. 172-175. AIP, Melville, New York (2010).
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[79] Wan M, Oughton S, Servidio S, and Matthaeus WH.
On the accuracy of simulations of turbulence.
Phys. Plasmas 17:082308, doi:10.1063/1.3474957 (2010).
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[80] Osman KT, Wan M, Matthaeus WH, Breech B, and Oughton S.
Directional alignment and non-Gaussian statistics in solar wind turbulence.
Astrophys. J. 741:75, doi:10.1088/0004-637X/741/2/75 (2011).
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[81] Oughton S, Matthaeus WH, Smith CW, Breech B, and Isenberg PA.
Transport of solar wind fluctuations: A two-component model.
J. Geophys. Res. 116:A08105, doi:10.1029/2010JA016365 (2011).
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[82] Zhou Y and Oughton S.
Nonlocality and the critical Reynolds numbers of the minimum state magnetohydrodynamic turbulence.
Phys. Plasmas 18:072304, doi:10.1063/1.3606473 (2011).
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[83] Matthaeus WH, Servidio S, Dmitruk P, Carbone V, Oughton S, Wan M, and Osman KT.
Local anisotropy, higher order statistics, and turbulence spectra.
Astrophys. J. 750:103, doi:10.1088/0004-637X/750/2/103 (2012).
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[84] Wan M, Osman KT, Matthaeus WH, and Oughton S.
Investigation of intermittency in magnetohydrodynamics and solar wind turbulence: Scale-dependent kurtosis.
Astrophys. J. 744:171, doi:10.1088/0004-637X/744/2/171 (2012).
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[85] Wan M, Oughton S, Servidio S, and Matthaeus WH.
von Kármán self-preservation hypothesis for magnetohydrodynamic turbulence and its consequences for universality.
J. Fluid Mech. 697:296-315, doi:10.1017/jfm.2012.61 (2012).
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[86] Wicks RT, Forman MA, Horbury TS, and Oughton S.
Power anisotropy in the magnetic field power spectral tensor of solar wind turbulence.
Astrophys. J. 746:103, doi:10.1088/0004-637X/746/1/103 (2012).
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[87] Forman MA, Wicks RT, Horbury TS, and Oughton S.
Scaling anisotropy of the solar wind magnetic parallel and perpendicular power.
In Solar Wind 13 (eds. GP Zank et al.), vol. 1539, pp. 167-170. AIP, Melville, New York (2013), doi:10.1063/1.4811014.
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[88] Oughton S, Wan M, Matthaeus WH, and Servidio S.
Solar wind fluctuations and the von Kármán-Howarth equations: The role of fourth-order correlations.
In Solar Wind 13 (eds. GP Zank et al.), vol. 1539, pp. 251-254. AIP, Melville, New York (2013), doi:10.1063/1.4811035.
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[89] Oughton S, Wan M, Servidio S, and Matthaeus WH.
On the origin of anisotropy in magnetohydrodynamic turbulence: The role of higher-order correlations.
Astrophys. J. 768:10, doi:10.1088/0004-637X/768/1/10 (2013).
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[90] Snodin AP, Ruffolo D, Oughton S, Servidio S, and Matthaeus WH.
Magnetic field line random walk in models and simulations of reduced magnetohydrodynamic turbulence.
Astrophys. J. 779:56, doi:10.1088/0004-637X/779/1/56 (2013).
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[91] Wan M, Matthaeus WH, Servidio S, and Oughton S.
Generation of X-points and secondary islands in 2D magnetohydrodynamic turbulence.
Phys. Plasmas 20:042307, doi:10.1063/1.4802985 (2013).
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[92] Matthaeus WH, Oughton S, Osman KT, Servidio S, Wan M, Gary GP, Shay MA, Valentini F, Roytershteyn V, Karimabadi H, and Chapman SC.
Nonlinear and linear timescales near kinetic scales in solar wind turbulence.
Astrophys. J. 790:155, doi:10.1088/0004-637X/790/2/155 (2014).
bib | DOI | Local pdf ]
[93] Matthaeus WH, Wan M, , Servidio S, Greco A, Osman KT, Oughton S, and Dmitruk P.
Intermittency, nonlinear dynamics, and dissipation in the solar wind and astrophysical plasmas.
Phil. Trans. R. Soc. A submitted (2014).
bib | DOI | Local pdf ]
[94] Oughton S, Matthaeus WH, Wan M, and Osman KT.
Anisotropy in solar wind plasma turbulence.
Phil. Trans. R. Soc. A submitted (2014).
bib | DOI | Local pdf ]
[95] Servidio S, Matthaeus WH, Wan M, Ruffolo D, Rappazzo AF, and Oughton S.
Complexity and diffusion of magnetic flux surfaces in anisotropic turbulence.
Astrophys. J. 785:56, doi:10.1088/0004-637X/785/1/56 (2014).
bib | DOI | Local pdf ]
[96] Wan M, Rappazzo AF, Matthaeus WH, Servidio S, and Oughton S.
Dissipation and reconnection in boundary-driven reduced magnetohydrodynamics.
Astrophys. J. in press (2014).
bib | DOI | Local pdf ]

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2014-11-20