Looking for evidence of mixing in the solar wind from 0.31 to 0.98 AU
暂无分享,去创建一个
[1] Geert Brethouwer,et al. Micro-structure and Lagrangian statistics of the scalar field with a mean gradient in isotropic turbulence , 2003, Journal of Fluid Mechanics.
[2] J. Gosling,et al. Correlation of solar wind entropy and oxygen ion charge state ratio , 2004 .
[3] J. Richardson,et al. The orientation of plasma structure in the solar wind , 1998 .
[4] K. H. Burrell,et al. Effects of E×B velocity shear and magnetic shear on turbulence and transport in magnetic confinement devices , 1997 .
[5] E. A. Fox,et al. Single‐phase blending of liquids , 1956 .
[6] D. Roberts,et al. The evolution of the spectrum of solar wind velocity fluctuations from 0.3 toSAU , 2011 .
[7] R. Antonia,et al. Decay of passive-scalar fluctuations in slightly stretched grid turbulence , 2012 .
[8] J. Borovsky. On the variations of the solar wind magnetic field about the Parker spiral direction , 2010 .
[9] Interfacial-fluid dynamics and the mixing efficiency of turbulent flows , 2004 .
[10] R. A. Antonia,et al. THE PHENOMENOLOGY OF SMALL-SCALE TURBULENCE , 1997 .
[11] E. Yee,et al. The vertical structure of concentration fluctuation statistics in plumes dispersing in the atmospheric surface layer , 1995 .
[12] Paul E. Dimotakis,et al. TURBULENT MIXING , 2004 .
[13] H. Spence,et al. Relative occurrence rates and connection of discrete frequency oscillations in the solar wind density and dayside magnetosphere , 2009 .
[14] Jos Derksen,et al. Mixing times in a turbulent stirred tank by means of LES , 2006 .
[15] S. Corrsin. Outline of some topics in homogeneous turbulent flow , 1959 .
[16] E. Smith,et al. Identification of trailing edge solar wind stream interfaces: A comparison of Ulysses plasma and composition measurements , 1999 .
[17] R. Skoug,et al. Reply to "Comment on the Paper ''On the Determination of Electron Polytrope Indices Within Coronal Mass Ejections in the Solar Wind'"' , 1999 .
[18] K. W. Norwood,et al. Flow patterns and mixing rates in agitated vessels , 1960 .
[19] Eckart Marsch,et al. MHD structures, waves and turbulence in the solar wind: Observations and theories , 1995 .
[20] I. M. O T A K I S. The mixing transition in turbulent flows , 2022 .
[21] D. Aaron Roberts,et al. Velocity shear generation of solar wind turbulence , 1992 .
[22] T. Horbury,et al. Development and Effects of Turbulence in Connection with CIRs , 1999 .
[23] K. Ogilvie,et al. Solar wind structure suggested by bimodal correlations of solar wind speed and density between the spacecraft SOHO and Wind , 2007 .
[24] S. Suess,et al. Relation between Pressure Balance Structures and polar plumes from Ulysses high latitude observations , 2002 .
[25] D. Berdichevsky,et al. Self-similar evolution of interplanetary magnetic clouds and Ulysses measurements of the polytropic index inside the cloud , 1997 .
[26] J. Borovsky. Eddy viscosity and flow properties of the solar wind: Co-rotating interaction regions, coronal-mass-ejection sheaths, and solar-wind/magnetosphere couplinga) , 2006 .
[27] H. Rosenbauer,et al. Two states of the solar wind at the time of solar activity minimum - II. Radial gradients of plasma parameters in fast and slow streams , 1981 .
[28] Werner J. A. Dahm,et al. Experimental study of the fine-scale structure of conserved scalar mixing in turbulent shear flows. Part 1. Sc [Gt ] 1 , 1996, Journal of Fluid Mechanics.
[29] M. O’Hara,et al. Summary and Implications , 1995 .
[30] The North—South Asymmetry of Soft X-Ray Flare Index During Solar Cycles 21, 22 and 23 , 2004, astro-ph/0609707.
[31] A. Nubile,et al. Long‐period oscillations at discrete frequencies: A comparative analysis of ground, magnetospheric, and interplanetary observations , 2007 .
[32] W. Feldman,et al. Evidence for a structure‐free state at high solar wind speeds , 1977 .
[33] Scale distributions of fluid interfaces in turbulence , 2000 .
[34] E. Marsch,et al. Are structures in high-speed streams signatures of coronal fine structures? , 1989 .
[35] E. Marsch,et al. Relationship between structures in the solar wind and their source regions in the corona , 1987 .
[36] K. Sreenivasan,et al. Scalar interfaces in digital images of turbulent flows , 1989 .
[37] D. Roberts,et al. Evolution of the spectrum of solar wind velocity fluctuations from 0.3 to 5 AU , 2010 .
[38] T. Ataç. Time variation of the flare index during the 21st solar cycle , 1987 .
[39] Z. Warhaft. Passive Scalars in Turbulent Flows , 2000 .
[40] J. Niemela,et al. Turbulent Mixing and Beyond , 2010, Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences.
[41] Passive-scalar wake behind a line source in grid turbulence , 2000, Journal of Fluid Mechanics.
[42] Wolfgang Baumjohann,et al. On the thermodynamics of the plasma sheet , 1991 .
[43] D. Weimer,et al. Improved calculations of interplanetary magnetic field phase front angles and propagation time delays , 2008 .
[44] J. Borovsky,et al. Entropy mapping of the outer electron radiation belt between the magnetotail and geosynchronous orbit , 2011 .
[45] J. Gosling,et al. Solar wind streamer belt structure , 1996 .
[46] T. Horbury,et al. The Variation of Solar Wind Correlation Lengths Over Three Solar Cycles , 2010, 1002.2319.
[47] Suzanne M. Kresta,et al. Turbulence in Mixing Applications , 2004 .
[48] K. Sreenivasan,et al. The measurement and interpretation of fractal dimensions of the scalar interface in turbulent flows , 1990 .
[49] F. Mariani,et al. A statistical study of MHD discontinuities in the inner solar system: Helios 1 and 2 , 1983 .
[50] R. Brodkey,et al. Turbulent motion, mixing, and kinetics in a chemical reactor configuration , 1975 .
[51] J. Borovsky,et al. Solar wind turbulence and shear: A superposed-epoch analysis of corotating interaction regions at 1 AU , 2010 .
[52] H. Kramers,et al. A comparative study on the rate of mixing in stirred tanks , 1953 .
[53] J. Steinberg,et al. Evidence of a solar origin for pressure balance structures in the high‐latitude solar wind , 1999 .
[54] Spectrum of a passive scalar in stretched grid turbulence at low Reynolds numbers , 2011 .
[55] V. Carbone,et al. The Solar Wind as a Turbulence Laboratory , 2005 .
[56] Pui-Kuen Yeung,et al. LAGRANGIAN INVESTIGATIONS OF TURBULENCE , 2003 .
[57] V. Carbone,et al. Identifying intermittency events in the solar wind , 2001 .
[58] P. J. Williams,et al. Simultaneous interplanetary scintillation and optical measurements of the acceleration of the slow solar wind , 2000 .
[59] J. Borovsky. Contribution of strong discontinuities to the power spectrum of the solar wind. , 2010, Physical review letters.
[60] J. Gollub,et al. Mixing rates and symmetry breaking in two-dimensional chaotic flow , 2003 .
[61] J. Borovsky. The velocity and magnetic field fluctuations of the solar wind at 1 AU: Statistical analysis of Fourier spectra and correlations with plasma properties , 2012 .
[62] M. Eselevich,et al. The structure of the coronal-streamer belt , 2005 .
[63] Werner J. A. Dahm,et al. Direct, high resolution, four‐dimensional measurements of the fine scale structure of Sc≫1 molecular mixing in turbulent flows , 1991 .
[64] Examining Periodic Solar-Wind Density Structures Observed in the SECCHI Heliospheric Imagers , 2010, 1009.5885.
[65] R. Britter,et al. Mixing due to grid-generated turbulence of a two-layer scalar profile , 1995, Journal of Fluid Mechanics.
[66] A. Miura,et al. Nonlocal stability analysis of the MHD Kelvin-Helmholtz instability in a compressible plasma. [solar wind-magnetosphere interaction] , 1982 .
[67] E. A. Frieman,et al. An energy principle for hydromagnetic stability problems , 1958, Proceedings of the Royal Society of London. Series A. Mathematical and Physical Sciences.
[68] H. Rosenbauer,et al. A Survey on Initial Results of the Helios Plasma Experiment , 1977 .
[69] H. Rosenbauer,et al. Anisotropy and minimum variance of magnetohydrodynamic fluctuations in the inner heliosphere , 1993 .
[70] Edward J. Smith,et al. Power spectra and discontinuities of the interplanetary magnetic field - Mariner 4. , 1968 .
[71] H. Spence,et al. Observations of discrete, global magnetospheric oscillations directly driven by solar wind density variations , 2003 .
[72] J. Freeman,et al. Estimates of solar wind velocity gradients between 0.3 and 1 AU based on velocity probability distributions from Helios 1 at perihelion and aphelion , 1991 .
[73] B. Cheng. Review of turbulent mixing models , 2009 .
[74] C. Garrett. On the initial streakness of a dispersing tracer in two- and three-dimensional turbulence , 1983 .
[75] N. Sheeley,et al. The dynamical nature of coronal streamers , 2000 .
[76] J. Freeman. Estimates of solar wind heating inside 0.3 AU , 1988 .
[77] Q. Hu,et al. Effect of current sheets on the solar wind magnetic field power spectrum from the Ulysses observation: from Kraichnan to Kolmogorov scaling. , 2011, Physical review letters.
[78] S. Pope,et al. Direct numerical simulations of the turbulent mixing of a passive scalar , 1988 .
[79] R. Woo,et al. Extension of coronal structure into interplanetary space , 1997 .
[80] L. Ofman. The origin of the slow solar wind in coronal streamers , 2002 .
[81] Alan R. Kerstein,et al. Linear-eddy modeling of turbulent transport. II: Application to shear layer mixing , 1989 .
[82] S. Corrsin. Simple theory of an idealized turbulent mixer , 1957 .
[83] M. Hoshino,et al. Turbulent mixing and transport of collisionless plasmas across a stratified velocity shear layer , 2006 .
[84] J. Steinberg,et al. Solar wind stream interaction regions without sector boundaries , 2004 .
[85] J. Borovsky. Flux tube texture of the solar wind: Strands of the magnetic carpet at 1 AU?: FLUX TUBE TEXTURE OF SOLAR WIND , 2008 .
[86] P. Dimotakis,et al. Stochastic geometric properties of scalar interfaces in turbulent jets , 1991 .
[87] S. Corrsin,et al. Temperature fluctuations and scales in grid-generated turbulence , 1980, Journal of Fluid Mechanics.
[88] J. W. Sari,et al. Power spectra of the interplanetary magnetic field , 1969 .
[89] S. Dinev,et al. Spectral and spatial evolution of a conical emission in Na vapor , 1998 .
[90] Catrakis. Distribution of scales in turbulence , 2000, Physical review. E, Statistical physics, plasmas, fluids, and related interdisciplinary topics.
[91] W. Feldman,et al. Solar wind stream interfaces , 1978 .
[92] J. Lumley,et al. The decay of temperature fluctuations in isotropic turbulence , 1977 .
[93] David J. McComas,et al. Evidence for ion jets in the high‐speed solar wind , 1993 .
[94] L. Burlaga,et al. Thermodynamic properties of the heliospheric plasma , 1989 .
[95] T. Horbury,et al. Magnetic Discontinuities in the Near-Earth Solar Wind: Evidence of In-Transit Turbulence or Remnants of Coronal Structure? , 2011 .
[96] L. Sorriso-Valvo,et al. Magnetically dominated structures as an important component of the solar wind turbulence , 2007 .
[97] H. Rosenbauer,et al. The dependence of MHD turbulence spectra on the inner solar wind stream structure near solar minimum , 1990 .
[98] A. Ridley. Estimations of the uncertainty in timing the relationship between magnetospheric and solar wind processes , 2000 .
[99] W. Seale. Turbulent diffusion of heat between connected flow passages Part 2: Predictions using the “κ-ϵ” turbulence model , 1979 .
[100] Eugene Yee,et al. Measurements of level-crossing statistics of concentration fluctuations in plumes dispersing in the atmospheric surface layer , 1995 .
[101] J. Ristorcelli,et al. Variable-density mixing in buoyancy-driven turbulence , 2007, Journal of Fluid Mechanics.
[102] E. Marsch,et al. Spectral and spatial evolution of compressible turbulence in the inner solar wind , 1990 .
[103] Alain Pumir,et al. Turbulent mixing of a passive scalar , 1999 .
[104] E. L. Paul,et al. Handbook of Industrial Mixing , 2003 .
[105] Roddam Narasimha,et al. Zero-crossings in turbulent signals , 1983, Journal of Fluid Mechanics.
[106] R. Britter,et al. Structure of the temperature field downwind of a line source in grid turbulence , 1986 .
[107] F. Neubauer,et al. Statistical properties of low‐frequency magnetic field fluctuations in the solar wind from 0.29 to 1.0 AU during solar minimum conditions: HELIOS 1 and HELIOS 2 , 1982 .
[108] E. Marsch,et al. On the nature of compressive fluctuations in the solar wind , 1994 .
[109] David H. Sharp,et al. Theoretical methods for the determination of mixing , 2003 .
[110] J. R. Ristorcelli,et al. Passive scalar mixing: Analytic study of time scale ratio, variance, and mix rate , 2006 .
[111] M. Mierla,et al. THE NORTH-SOUTH ASYMMETRY OF SOFT X-RAY SOLAR FLARES , 2002 .
[112] H. Rosenbauer,et al. Cooling of solar wind electrons inside 0.3 AU , 1989 .
[113] J. Richardson,et al. Plasma and magnetic field correlations in the solar wind , 2001 .
[114] V. Pizzo. A three-dimensional model of corotating streams in the solar wind. 1: Theoretical foundations , 1978 .
[115] Alan R. Kerstein,et al. Linear-eddy modeling of turbulent transport. Part V: Geometry of scalar interfaces , 1991 .
[116] Kolmogorov similarity hypotheses for scalar fields: sampling intermittent turbulent mixing in the ocean and galaxy , 1991, Proceedings of the Royal Society of London. Series A: Mathematical and Physical Sciences.
[117] J. Freeman,et al. The cold solar wind , 1985 .
[118] W. H. Mish,et al. Coalescence of recurrent streams of different sizes and amplitudes. [low-density flows in solar coronal holes , 1990 .
[119] E. Marsch,et al. On the radial evolution of MHD turbulence in the inner heliosphere , 1990 .
[120] The geometric properties of high-Schmidt-number passive scalar iso-surfaces in turbulent boundary layers , 2007, Journal of Fluid Mechanics.
[121] J. Landau,et al. Studies on mixing. XII. Homogenation of miscible liquids in the turbulent region , 1961 .
[122] D. A. Roberts,et al. Magnetohydrodynamic Turbulence in the Solar Wind , 1995 .
[123] J. M. Ottino,et al. Morphological structures produced by mixing in chaotic flows , 1988, Nature.
[124] Andrew Robert Breen,et al. Slow and fast solar wind acceleration near solar maximum , 2002 .
[125] G. C. Broadhead. CONE IN CONE. , 1907, Science.
[126] Edward J. Smith,et al. Factors controlling degree of correlation between ISEE 1 and ISEE 3 interplanetary magnetic field measurements , 1982 .
[127] Haris J. Catrakis,et al. Shape complexity of whole-field three-dimensional space–time fluid interfaces in turbulence , 2002 .
[128] B. Bavassano,et al. Solar wind fluctuations at large scale: A comparison between low and high solar activity conditions , 1991 .
[129] E. Marsch,et al. Spatial structures in high-speed streams as signatures of fine structures in coronal holes. , 1990 .
[130] J. Dungey. Magnetospheric physics , 1978, Nature.
[131] H. Spence,et al. Are periodic solar wind number density structures formed in the solar corona? , 2009 .
[132] J. Ottino. Mixing, chaotic advection, and turbulence , 1990 .
[133] K. Rehme,et al. The structure of turbulence in rod bundles and the implications on natural mixing between the subchannels , 1992 .
[134] A Three-Dimensional Model of Corotating Streams in the ' Solar Wind 1 , 2011 .
[135] W. Matthaeus,et al. Dynamical age of solar wind turbulence in the outer heliosphere , 1998 .
[136] W. Seale,et al. Turbulent diffusion of heat between connected flow passages Part 1: Outline of problem and experimental investigation , 1979 .
[137] E. Marsch,et al. MHD Structures, Waves and Turbulence in the Solar Wind , 1995 .
[138] E. Villermaux,et al. Histogramme des fluctuations scalaires dans le mélange turbulent transitoire , 1998 .
[139] M. Eselevich,et al. Manifestations of the ray structure of the coronal streamer belt in the form of sharp peaks of the solar wind plasma density in the Earth’s orbit , 2006 .
[140] Claudia Innocenti,et al. On the geometry of turbulent mixing , 1998, Journal of Fluid Mechanics.
[141] R. Schwenn. Large-scale structure of the interplanetary medium , 1990 .
[142] E. Marsch,et al. A case study of very low cross-helicity fluctuations in the solar wind. , 1991 .
[143] Robert L. McPherron,et al. A new interpretation of Weimer et al.'s solar wind propagation delay technique , 2005 .
[144] J. Borovsky,et al. NO EVIDENCE FOR HEATING OF THE SOLAR WIND AT STRONG CURRENT SHEETS , 2011 .
[145] J. Borovsky. The Flux-Tube Texture of the Solar Wind , 2006 .
[146] J. Borovsky,et al. Role of solar wind turbulence in the coupling of the solar wind to the Earth's magnetosphere , 2003 .
[147] W. Dahm,et al. Experimental study of the fine-scale structure of conserved scalar mixing in turbulent shear flows. Part 2. Sc≈1 , 1998, Journal of Fluid Mechanics.