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 W.H., Stribling W.T., 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 W.H., Stribling W.T., 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 G.P., Oughton S., Neubauer F.M., and Webb G.M.
Mass-loading and parallel magnetized shocks.
Geophys. Res. Lett. 18:1809-1812 (1991).
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[4] Zank G.P. and Oughton S.
Properties of mass-loading shocks 1. Hydrodynamic considerations.
J. Geophys. Res. 96:9439-9453 (1991).
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[5] Matthaeus W.H., Zhou Y., Oughton S., and Zank G.P.
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 D.C., Matthaeus W.H., Stribling W.T., 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 W.H.
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 G.P., Oughton S., Neubauer F.M., and Webb G.M.
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 W.H., 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 W.H., Zhou Y., Zank G.P., 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 W.H., and Priest E.R.
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 H.K. Biernat), pp. 81-86. dbv-Verlag Graz (1994).
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[13] Oughton S., Priest E.R., and Matthaeus W.H.
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 P.C., Pontius Jr. D.H., Matthaeus W.H., 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 W.H., 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 W.H., 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 P.L. Sulem), vol. 462 (Lecture Notes in Physics), pp. 273-279. Springer-Verlag (1995).
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[17] Oughton S. and Matthaeus W.H.
Linear transport of solar wind fluctuations.
J. Geophys. Res. 100:14783-14799 (1995).
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[18] Stribling T., Matthaeus W.H., 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 P.C., Pontius Jr. D.H., Matthaeus W.H., and Oughton S.
Is the Alfvén wave propagation effect important for energy decay in homogeneous MHD turbulence? In Solar Wind Eight (eds. D. Winterhalter, J.T. Gosling, S.R. Habbal, W.S. Kurth, and M. Neugebauer), pp. 358-361. AIP, New York (1996).
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[20] Matthaeus W.H., Zank G.P., 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 W.H., Ghosh S., Oughton S., and Roberts D.A.
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 K.H., and Matthaeus W.H.
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 W.H., Smith C.W., 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 W.H., 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 W.H., 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 W.H., 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 W.H., Zank G.P., 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, J.V. Hollweg, and P.A. Isenberg), vol. 471, pp. 361-364. AIP, Woodbury, NY (1999).
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[30] Matthaeus W.H., Zank G.P., Leamon R.J., Smith C.W., Mullan D.J., 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 W.H., Zank G.P., Smith C.W., 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 W.H., Zank G.P., Oughton S., Mullan D.J., 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 W.H., and Smith C.W.
Measurement of spectral anisotropy using single spacecraft data.
In Solar Wind Nine (eds. S. Habbal, R. Esser, J.V. Hollweg, and P.A. Isenberg), vol. 471, pp. 507-510. AIP, Woodbury, NY (1999).
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[34] Oughton S., Matthaeus W.H., Zank G.P., and Mullan D.J.
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. J.C. Vial and B. Kaldeich-Schürmann), vol. ESA SP-446, pp. 525-530. ESA, Noordwijk, The Netherlands (1999).
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[35] Smith C.W., Zank G.P., Matthaeus W.H., 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 G.P., Matthaeus W.H., Smith C.W., and Oughton S.
Heating of the solar wind beyond 1AU by turbulent dissipation.
In Solar Wind Nine (eds. S. Habbal, R. Esser, J.V. Hollweg, and P.A. Isenberg), vol. 471, pp. 523-526. AIP, Woodbury, NY (1999).
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[37] Leamon R.J., Matthaeus W.H., Smith C.W., Zank G.P., Mullan D.J., 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 W.H., Milano L.J., 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 W.H., Dmitruk P., Milano L.M., Zank G.P., and Mullan D.J.
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 C.W., Matthaeus W.H., Zank G.P., Ness N.F., Oughton S., and Richardson J.D.
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 N.W., Oughton S., and Freeman M.P.
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 W.H., Milano L.J., Oughton S., Zank G.P., and Mullan D.J.
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 W.H., Mullan D.J., Dmitruk P., Milano L., and Oughton S.
MHD turbulence and heating of the open field line solar corona.
Nonlin. Process. Geophys. 10:93-100 (2003).
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[46] Matthaeus W.H., 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 W.H., 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 W.H., 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 W.H.
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 W.H., Minnie J., Breech B., Parhi S., Bieber J.W., 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 W.H.
Reduced magnetohydrodynamics and parallel spectral transfer.
Phys. Plasmas 11:2214-2225, doi:10.1063/1.1705652 (2004).
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[53] Smith C.W., Isenberg P.A., Matthaeus W.H., Richardson J.D., Oughton S., and Zank G.P.
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 W.H., Minnie J., Oughton S., Parhi S., Bieber J.W., 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 W.H., Minnie J., Oughton S., Parhi S., Bieber J.W., 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 W.H., 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 M.A., 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 W.H.
Parallel and perpendicular cascades in solar wind turbulence.
Nonlin. Process. Geophys. 12:299-310 (2005).
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[60] Oughton S., Dmitruk P., and Matthaeus W.H.
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 W.H., 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 W.H., 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 P.G., Oughton S., and Craig I.J.D.
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 W.H., Minnie J., Bieber J.W., Oughton S., Smith C.W., and Isenberg P.A.
Turbulence transport throughout the heliosphere.
J. Geophys. Res. 113:A08105, doi:10.1029/2007JA012711 (2008).
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[67] Horbury T.S., 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 W.H., Cranmer S.R., Kasper J.C., 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 W.H., 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 W.H.
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 W.H.
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 S.R., Matthaeus W.H., Kasper J.C., 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 W.H., 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 P.A., Oughton S., Smith C.W., and Matthaeus W.H.
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, G.P. Zank, A.J. Coates, and V. Florinski), vol. 1302, pp. 180-185. AIP (2010), doi:10.1063/1.3529967.
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[75] Oughton S., Matthaeus W.H., Smith C.W., 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 W.H., 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 W.H.
The third-order law for magnetohydrodynamic turbulence with shear: Numerical investigation.
Phys. Plasmas 17(5):052307, doi:10.1063/1.3398481 (2010).
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[78] Wan M., Oughton S., Servidio S., and Matthaeus W.H.
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 W.H.
On the accuracy of simulations of turbulence.
Phys. Plasmas 17:082308, doi:10.1063/1.3474957 (2010).
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[80] Osman K.T., Wan M., Matthaeus W.H., 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 W.H., Smith C.W., Breech B., and Isenberg P.A.
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 W.H., Servidio S., Dmitruk P., Carbone V., Oughton S., Wan M., and Osman K.T.
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 K.T., Matthaeus W.H., 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 W.H.
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 R.T., Forman M.A., Horbury T.S., 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 M.A., Wicks R.T., Horbury T.S., and Oughton S.
Scaling anisotropy of the solar wind magnetic parallel and perpendicular power.
In Solar Wind 13 (eds. G.P. 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 W.H., and Servidio S.
Solar wind fluctuations and the von Kármán-Howarth equations: The role of fourth-order correlations.
In Solar Wind 13 (eds. G.P. Zank et al.), vol. 1539, pp. 251-254. AIP, Melville, New York (2013), doi:10.1063/1.4811035.
bib | DOI | Local pdf ]
[89] Oughton S., Wan M., Servidio S., and Matthaeus W.H.
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).
bib | DOI | Local pdf ]
[90] Snodin A.P., Ruffolo D., Oughton S., Servidio S., and Matthaeus W.H.
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).
bib | DOI | Local pdf ]
[91] Wan M., Matthaeus W.H., 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).
bib | DOI | Local pdf ]
[92] Servidio S., Matthaeus W.H., Wan M., Ruffolo D., Rappazzo A.F., 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 ]

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2014-03-26