| [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). [ bib | Local pdf ] |
| [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). [ bib | DOI | Local pdf ] |
| [3] |
Zank GP, Oughton S, Neubauer FM, and Webb GM.
Mass-loading and parallel magnetized shocks. Geophys. Res. Lett. 18:1809--1812 (1991). [ bib | Local pdf ] |
| [4] |
Zank GP and Oughton S.
Properties of mass-loading shocks 1. Hydrodynamic considerations. J. Geophys. Res. 96:9439--9453 (1991). [ bib | Local pdf ] |
| [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). [ bib | Local pdf ] |
| [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). [ bib | DOI | Local pdf ] |
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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). [ bib | Local pdf ] |
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Zank GP, Oughton S, Neubauer FM, and Webb GM.
Properties of mass-loading shocks 2. Magnetohydrodynamics. J. Geophys. Res. 97:17051--17074 (1992). [ bib | Local pdf ] |
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Oughton S.
Transport of Solar Wind Fluctuations: A Turbulence Approach.
Ph.D. thesis, University of Delaware, Newark, Delaware, 19716 (1993).
[ bib | Local pdf ] |
| [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, doi:10.1029/94JA01233 (1994). [ bib | DOI | Local pdf ] |
| [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, doi:10.1029/94JA02326 (1994). [ bib | DOI | Local pdf ] |
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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). [ bib | Local pdf ] |
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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). [ bib | DOI | Local pdf ] |
| [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). [ bib | DOI | Local pdf ] |
| [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). [ bib | Local pdf ] |
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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). [ bib | Local pdf ] |
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Oughton S and Matthaeus WH.
Linear transport of solar wind fluctuations. J. Geophys. Res. 100:14783--14799 (1995). [ bib | Local pdf ] |
| [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). [ bib | DOI | Local pdf ] |
| [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). [ bib | Local pdf ] |
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Matthaeus WH, Zank GP, and Oughton S.
Phenomenology of hydromagnetic turbulence in a uniformly expanding medium. J. Plasma Phys. 56:659--675, doi:10.1017/S0022377800019516 (1996). [ bib | DOI | Local pdf ] |
| [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). [ bib | DOI | Local pdf ] |
| [22] |
Oughton S.
Ion parallel viscosity and anisotropy in MHD turbulence. J. Plasma Phys. 56:641--657 (1996). [ bib | DOI | Local pdf ] |
| [23] |
Oughton S.
Energy dynamics in linear MHD with ion parallel viscosity. J. Plasma Phys. 58:571--576, doi:10.1017/S0022377897005928 (1997). [ bib | DOI | Local pdf ] |
| [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). [ bib | DOI | Local pdf ] |
| [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). [ bib | DOI | Local pdf ] |
| [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). [ bib | DOI | Local pdf ] |
| [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). [ bib | Local pdf ] |
| [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). [ bib | DOI | Local pdf ] |
| [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). [ bib | Local pdf ] |
| [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. [ bib | Local pdf ] |
| [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). [ bib | DOI | Local pdf ] |
| [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). [ bib | Local pdf ] |
| [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). [ bib | Local pdf ] |
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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). [ bib | Local pdf ] |
| [35] |
Smith CW, Zank GP, Matthaeus WH, and Oughton S.
Heating of the solar wind beyond 1AU by turbulent dissipation. In Proceedings of the 26th ICRC (eds. D Kieda, M Salanov, and B Dingus), vol. 7, pp. 480--483 (1999). [ bib | Local pdf ] |
| [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). [ bib | Local pdf ] |
| [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). [ bib | DOI | Local pdf ] |
| [38] |
Oughton S and Prandi R.
Kinetic helicity and MHD turbulence. J. Plasma Phys. 64:179--193 (2000). [ bib | DOI | Local pdf ] |
| [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). [ bib | DOI | Local pdf ] |
| [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). [ bib | DOI | Local pdf ] |
| [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). [ bib | Local pdf ] |
| [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). [ bib | Local pdf ] |
| [43] |
Chapman S, Freeman M, and Oughton S.
Complexity in astroplasmas. Astronomy and Geophysics 42:22--2 (2001). [ bib ] |
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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). [ bib | DOI | Local pdf ] |
| [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). [ bib | DOI | Local pdf ] |
| [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). [ bib | DOI | Local pdf ] |
| [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). [ bib | Local pdf ] |
| [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). [ bib | Local pdf ] |
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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. [ bib | DOI | Local pdf ] |
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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). [ bib | Local pdf ] |
| [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). [ bib | DOI | Local pdf ] |
| [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). [ bib | DOI | Local pdf ] |
| [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). [ bib | Local pdf ] |
| [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). [ bib | DOI | Local pdf ] |
| [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). [ bib | DOI | Local pdf ] |
| [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). [ bib | Local pdf ] |
| [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). [ bib | DOI | Local pdf ] |
| [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). [ bib | DOI | Local pdf ] |
| [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). [ bib | DOI | Local pdf ] |
| [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). [ bib | DOI | Local pdf ] |
| [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). [ bib | DOI | Local pdf ] |
| [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). [ bib | DOI | Local pdf ] |
| [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). [ bib | DOI | Local pdf ] |
| [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). [ bib | Local pdf ] |
| [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). [ bib | DOI | Local pdf ] |
| [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). [ bib | DOI | Local pdf ] |
| [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). [ bib | DOI | Local pdf ] |
| [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). [ bib | DOI | Local pdf ] |
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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). [ bib | DOI | Local pdf ] |
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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). [ bib | DOI | Local pdf ] |
| [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). [ bib | DOI | Local pdf ] |
| [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). [ bib | DOI | Local pdf ] |
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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). [ bib | DOI | Local pdf ] |
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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. [ bib | DOI | Local pdf ] |
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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). [ bib | DOI | Local pdf ] |
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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. Lett. 708:L116--L120, doi:10.1088/2041-8205/708/2/L116 (2010). [ bib | DOI | Local pdf ] |
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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). [ bib | DOI | Local pdf ] |
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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). [ bib | DOI | Local pdf ] |
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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). [ bib | DOI | Local pdf ] |
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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). [ bib | DOI | Local pdf ] |
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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). [ bib | DOI | Local pdf ] |
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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). [ bib | DOI | Local pdf ] |
| [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). [ bib | DOI | Local pdf ] |
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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). [ bib | DOI | Local pdf ] |
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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). [ bib | DOI | Local pdf ] |
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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). [ bib | DOI | Local pdf ] |
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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. [ bib | DOI | Local pdf ] |
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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. [ bib | DOI | Local pdf ] |
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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). [ bib | DOI | Local pdf ] |
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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). [ bib | DOI | Local pdf ] |
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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). [ bib | DOI | Local pdf ] |
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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 ] |
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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 ] |
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Wan M, Rappazzo AF, Matthaeus WH, Servidio S, and Oughton
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Dissipation and reconnection in boundary-driven reduced magnetohydrodynamics. Astrophys. J. 797:63, doi:10.1088/0004-637X/797/1/63 (2014). [ bib | DOI | Local pdf ] |
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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 373:20140154, doi:10.1098/rsta.2014.0154 (2015). [ bib | DOI | Local pdf ] |
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Oughton S, Matthaeus WH, Wan M, and Osman KT.
Anisotropy in solar wind plasma turbulence. Phil. Trans. R. Soc. A 373:20140152, doi:10.1098/rsta.2014.0152 (2015). [ bib | DOI | Local pdf ] |
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Oughton S, Matthaeus WH, Wan M, and Parashar TN.
Variance anisotropy in compressible 3-D MHD. J. Geophys. Res. 121:5041--5054, doi:10.1002/2016JA022496 (2016). [ bib | DOI | Local pdf ] |
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Parashar TN, Matthaeus WH, Wan M, and Oughton S.
Variance anisotropy in kinetic plasmas. Astrophys. J. 824:44, doi:10.3847/0004-637X/824/1/44 (2016). [ bib | DOI | Local pdf ] |
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Wiengarten T, Oughton S, Engelbrecht NE, Fichtner H, Kleimann J,
and Scherer K.
A generalized two-component model of solar wind turbulence and ab initio diffusion mean-free paths and drift lengthscales of cosmic rays. Astrophys. J. 833:17, doi:10.3847/0004-637X/833/1/17 (2016). [ bib | DOI | Local pdf ] |
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Oughton S, Matthaeus WH, and Dmitruk P.
Reduced MHD in astrophysical applications: Two-dimensional or three-dimensional? Astrophys. J. 839:2, doi:10.3847/1538-4357/aa67e2 (2017). [ bib | DOI | Local pdf ] |
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Bandyopadhyay R, Oughton S, Wan M, Matthaeus WH, Chhiber R,
and Parashar TN.
Finite dissipation in anisotropic magnetohydrodynamic turbulence. Phys. Rev. X 8:041052, doi:10.1103/PhysRevX.8.041052 (2018). [ bib | DOI | Local pdf ] |
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Brandenburg A and Oughton S.
Cross-helically forced and decaying hydromagnetic turbulence. Astron. Nachr. 339:641--646, doi:10.1002/asna.201913602 (2018). [ bib | DOI | Local pdf ] |
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Bandyopadhyay R, Matthaeus WH, Oughton S, and Wan M.
Evolution of similarity lengths in anisotropic magnetohydrodynamic turbulence. J. Fluid Mech. 876:5--18, doi:10.1017/jfm.2019.513 (2019). [ bib | DOI | Local pdf ] |
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Chhiber R, Matthaeus WH, Oughton S, and Parashar T.
A detailed examination of anisotropy and timescales in three-dimensional incompressible magnetohydrodynamic turbulence. Phys. Plasmas 27(6):062308, doi:10.1063/5.0005109 (2020). [ bib | DOI | Local pdf ] |
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Fichtner H, Kleimann J, Yoon PH, Scherer K, Oughton S,
and Engelbrecht NE.
On the generation of compressible mirror-mode fluctuations in the inner heliosheath. Astrophys. J. 901:76, doi:10.3847/1538-4357/abaf52 (2020). [ bib | DOI | Local pdf ] |
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Oughton S and Matthaeus WH.
Critical balance and the physics of magnetohydrodynamic turbulence. Astrophys. J. 897:37, doi:10.3847/1538-4357/ab8f2a (2020). [ bib | DOI | Local pdf ] |
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Oughton S and Engelbrecht NE.
Solar wind turbulence: Connections with energetic particles. New Astron. 83:101507, doi:10.1016/j.newast.2020.101507 (2021). [ bib | DOI | Local pdf ] |
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Fraternale F, Adhikari L, Fichtner H, Kim TK, Kleimann J, Oughton S,
Pogorelov NV, Roytershteyn V, Smith CW, Usmanov AV, Zank GP,
and Zhao L.
Turbulence in the outer heliosphere. Space Sci. Rev. 218(6):50 (pages 70), doi:10.1007/s11214-022-00914-2 (2022). [ bib | DOI | Local pdf ] |
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Wang Y, Chhiber R, Adhikari S, Yang Y, Bandyopadhyay R, Shay MA,
Oughton S, Matthaeus WH, and Cuesta ME.
Strategies for determining the cascade rate in MHD turbulence: Isotropy, anisotropy, and spacecraft sampling. Astrophys. J. 937(2):76, doi:10.3847/1538-4357/ac8f90 (2022). [ bib | DOI | Local pdf ] |
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Capocci D, Johnson PL, Oughton S, Biferale L, and
Linkmann M.
New exact Betchov-like relation for the helicity flux in homogeneous turbulence. J. Fluid Mech. in press:arXiv:2301.04193, doi:10.48550/arXiv.2301.04193 (2023). [ bib | DOI | Local pdf ] |
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Kleimann J, Oughton S, Fichtner H, and Scherer K.
A three-dimensional model for the evolution of MHD turbulence in the outer heliosphere. Astrophys. J. p. submitted (2023). [ bib | DOI | Local pdf ] |
This file was generated by bibtex2html 1.98, and then tweaked using perl.
2023-03-13