Alfvénic Turbulence in the Extended Solar Corona: Kinetic Effects and Proton Heating
暂无分享,去创建一个
[1] L. Milano,et al. MHD turbulence and heating of the open field-line solar corona , 2003 .
[2] M. Shay,et al. Formation of Electron Holes and Particle Energization During Magnetic Reconnection , 2003, Science.
[3] S. Spangler. The Amplitude of Magnetohydrodynamic Turbulence in the Inner Solar Wind , 2002 .
[4] R. Lin,et al. Electrostatic Turbulence and Debye-Scale Structures Associated with Electron Thermalization at Collisionless Shocks , 2002 .
[5] M. Sharp,et al. Influence of subglacial drainage system evolution on glacier surface motion: Haut Glacier d'Arolla, Switzerland , 2002 .
[6] L. Milano,et al. Coronal Heating Distribution Due to Low-Frequency, Wave-driven Turbulence , 2002, astro-ph/0204347.
[7] E. Marsch,et al. Kinetic Results for Ions in the Solar Corona with Wave-Particle Interactions and Coulomb Collisions , 2002 .
[8] M. Goossens,et al. Nonlinear excitation of small-scale Alfvén waves by fast waves and plasma heating in the solar atmosphere , 2002 .
[9] P. Isenberg. The kinetic shell model of coronal heating and acceleration by ion cyclotron waves: 2. Inward and outward propagating waves , 2001 .
[10] J. Hollweg,et al. Electron heat flux instabilities in coronal holes: Implications for ion heating , 2001 .
[11] S. Cranmer. Ion cyclotron diffusion of velocity distributions in the extended , 2001 .
[12] S. Markovskii. Generation of Ion Cyclotron Waves in Coronal Holes by a Global Resonant Magnetohydrodynamic Mode , 2001 .
[13] F. Mottez. Instabilities and Formation of Coherent Structures , 2001 .
[14] S. Habbal,et al. Damping of fast and ion cyclotron oblique waves in the multi‐ion fast solar wind , 2001 .
[15] A. Lazarian,et al. Simulations of Magnetohydrodynamic Turbulence in a Strongly Magnetized Medium , 2001, astro-ph/0105235.
[16] E. Marsch,et al. On cyclotron wave heating and acceleration of solar wind ions in the outer corona , 2001 .
[17] Hui Li,et al. Solar wind magnetic fluctuation spectra: Dispersion versus damping , 2001 .
[18] L. Milano,et al. Wave-driven Turbulent Coronal Heating in Open Field Line Regions: Nonlinear Phenomenological Model , 2001 .
[19] J. Maron,et al. Simulations of Incompressible Magnetohydrodynamic Turbulence , 2000, astro-ph/0012491.
[20] E. Marsch,et al. Heating and acceleration of coronal ions interacting with plasma waves through cyclotron and Landau resonance , 2001 .
[21] U. Feldman,et al. Properties of Solar Polar Coronal Hole Plasmas Observed above the Limb , 2001 .
[22] A. Ng,et al. Random Scattering and Anisotropic Turbulence of Shear Alfvén Wave Packets , 2000 .
[23] J. Mataix,et al. The Influence of Dietary Fat Source (sunflower Oil or Olive Oil) on Ldl Composition and Serum Lipid Levels in Miniature Swine (sus Serofa) , 2022 .
[24] T. Arber,et al. A Method to Determine the Heating Mechanisms of the Solar Corona , 2000 .
[25] R. Esser,et al. Velocity Shear-induced Mode Conversion in Solar Wind and Streamer Plasmas , 2000 .
[26] W. Matthaeus,et al. MHD-driven Kinetic Dissipation in the Solar Wind and Corona , 2000 .
[27] Shevchenko,et al. Nonlinear cyclotron resonant wave-particle interaction in a nonuniform magnetic field , 2000, Physical review letters.
[28] Lou‐Chuang Lee,et al. Heating and Acceleration of Protons and Minor Ions by Fast Shocks in the Solar Corona , 2000 .
[29] J. Hollweg. Compressibility of ion cyclotron and whistler waves: Can radio measurements detect high‐frequency waves of solar origin in the corona? , 2000 .
[30] B. Roberts,et al. Waves and Oscillations in the Corona – (Invited Review) , 2000 .
[31] S. Cranmer. Ion Cyclotron Wave Dissipation in the Solar Corona: The Summed Effect of More than 2000 Ion Species , 2000 .
[32] P. Kintner,et al. On the perpendicular scale of electron phase‐space holes , 2000 .
[33] Antonucci,et al. Identification of the Coronal Sources of the Fast Solar Wind , 2000, The Astrophysical journal.
[34] R. Ergun,et al. Properties of fast solitary structures , 1999 .
[35] J. Hollweg,et al. Cyclotron resonance in coronal holes: 1. Heating and acceleration of protons, , 1999 .
[36] H. Matsumoto,et al. Interaction of Small Phase Density Holes , 1999 .
[37] Charles W. Smith,et al. Dissipation range dynamics: Kinetic Alfvn waves and the importance of , 1999 .
[38] Xing Li. Proton temperature anisotropy in the fast solar wind: A 16‐moment bi‐Maxwellian model , 1999 .
[39] P. Dmitruk,et al. Coronal Heating by Magnetohydrodynamic Turbulence Driven by Reflected Low-Frequency Waves , 1999 .
[40] J. Hollweg,et al. Kinetic Alfvén wave revisited , 1999 .
[41] J. F. Mckenzie,et al. Solar coronal heating by high-frequency dispersive Alfvén waves , 1999 .
[42] J. Hollweg,et al. Heating and cooling of protons by turbulence-driven ion cyclotron waves in the fast solar wind , 1999 .
[43] S. Fineschi,et al. An Empirical Model of a Polar Coronal Hole at Solar Minimum , 1999 .
[44] A. Lazarian,et al. Reconnection in a Weakly Stochastic Field , 1998, astro-ph/9811037.
[45] E. Quataert,et al. Turbulence and Particle Heating in Advection-dominated Accretion Flows , 1998, astro-ph/9803112.
[46] S. Cranmer. Non-Maxwellian Redistribution in Solar Coronal Lyα Emission , 1998 .
[47] George B. Field,et al. Spectroscopic Constraints on Models of Ion Cyclotron Resonance Heating in the Polar Solar Corona and High-Speed Solar Wind , 1998 .
[48] M. Porkolab. Kinetic theory of plasma waves, homogeneous plasmas , 1998 .
[49] J. Chae,et al. SUMER Measurements of Nonthermal Motions: Constraints on Coronal Heating Mechanisms , 1998 .
[50] S. Bale,et al. Bipolar electrostatic structures in the shock transition region: Evidence of electron phase space holes , 1998 .
[51] F. Mozer,et al. DEBYE-SCALE PLASMA STRUCTURES ASSOCIATED WITH MAGNETIC-FIELD-ALIGNED ELECTRIC FIELDS , 1998 .
[52] Giampiero Naletto,et al. UVCS/SOHO Empirical Determinations of Anisotropic Velocity Distributions in the Solar Corona , 1998 .
[53] Marco Brambilla,et al. Kinetic Theory of Plasma Waves: Homogeneous Plasmas , 1998 .
[54] H. K. Wong,et al. Observational constraints on the dynamics of the interplanetary magnetic field dissipation range , 1998 .
[55] S. Fineschi,et al. Plasma Properties in Coronal Holes Derived from Measurements of Minor Ion Spectral Lines and Polarized White Light Intensity , 1998 .
[56] S. Fineschi,et al. EUV Spectral Line Profiles in Polar Coronal Holes from 1.3 to 3.0 R☉ , 1998 .
[57] E. Quataert. Particle Heating by Alfvénic Turbulence in Hot Accretion Flows , 1997, astro-ph/9710127.
[58] Giampiero Naletto,et al. First Results from the Soho Ultraviolet Coronagraph Spectrometer , 1997 .
[59] P. Goldreich,et al. Magnetohydrodynamic Turbulence Revisited , 1997 .
[60] E. Marsch,et al. TWO-FLUID MODEL FOR HEATING OF THE SOLAR CORONA AND ACCELERATION OF THE SOLAR WIND BY HIGH-FREQUENCY ALFVÉN WAVES , 1997 .
[61] S. Fineschi,et al. First results from UVCS/SOHO , 1997 .
[62] J. Harmon,et al. Observations of field-aligned density microstructure near the Sun , 1997 .
[63] Hiroshi Matsumoto,et al. Nonlinear waves and chaos in space plasmas , 1997 .
[64] W. Matthaeus,et al. Evolution of turbulent magnetic fluctuation power with heliospheric distance , 1996 .
[65] J. Kohl,et al. Measurement of Hydrogen Velocity Distributions in the Extended Solar Corona , 1996 .
[66] F. Gratton,et al. Acceleration and heating of heavy ions by circularly polarized Alfvén waves , 1996 .
[67] E. Olsen,et al. Thermally Driven One-Fluid Electron-Proton Solar Wind: Eight-Moment Approximation , 1996 .
[68] Liting Song. Turbulence spectrum of kinetic Alfvén wave in the solar wind. (a) Landau damping , 1996 .
[69] W. Matthaeus,et al. Anisotropic three-dimensional MHD turbulence , 1996 .
[70] James A. Miller,et al. Stochastic Electron Acceleration by Cascading Fast Mode Waves in Impulsive Solar Flares , 1996 .
[71] H. Rosenbauer,et al. An extended structure-function model and its application to the analysis of solar wind intermittency properties , 1996 .
[72] Multifractal scaling of the kinetic energy flux in solar wind turbulence , 1996 .
[73] R. Lysak,et al. On the kinetic dispersion relation for shear Alfvén waves , 1996 .
[74] R. Esser,et al. Coronal heating and plasma parameters at 1 AU , 1995 .
[75] John W. Belcher,et al. Radial evolution of the solar wind from IMP 8 to Voyager 2 , 1995 .
[76] W. Feldman,et al. Solar wind plasma electron parameters based on aligned observations by ICE and Ulysses , 1995 .
[77] Minoru Tsutsui,et al. Electrostatic solitary waves (ESW) in the magnetotail: BEN wave forms observed by GEOTAIL , 1994 .
[78] S. Sridhar,et al. Toward a theory of interstellar turbulence. 2. Strong Alfvenic turbulence , 1994 .
[79] N. Omidi,et al. Mode properties of low‐frequency waves: Kinetic theory versus Hall‐MHD , 1994 .
[80] Claude Brezinski,et al. Numerical recipes in Fortran (The art of scientific computing) : W.H. Press, S.A. Teukolsky, W.T. Vetterling and B.P. Flannery, Cambridge Univ. Press, Cambridge, 2nd ed., 1992. 963 pp., US$49.95, ISBN 0-521-43064-X.☆ , 1993 .
[81] Joseph P. Dougherty,et al. Waves in plasmas. , 1993 .
[82] D. Aaron Roberts,et al. Velocity shear generation of solar wind turbulence , 1992 .
[83] J. Scudder. Why all stars should possess circumstellar temperature inversions , 1992 .
[84] William H. Press,et al. Numerical recipes in FORTRAN (2nd ed.): the art of scientific computing , 1992 .
[85] T. H. Stix. Waves in plasmas , 1992 .
[86] J. F. Mckenzie,et al. The origin of high speed solar wind streams , 1992 .
[87] S. Spangler. The Dissipation of Magnetohydrodynamic Turbulence Responsible for Interstellar Scintillation and the Heating of the Interstellar Medium , 1991 .
[88] Eugene N. Parker,et al. Heating solar coronal holes , 1991 .
[89] Eckart Marsch,et al. Kinetic Physics of the Solar Wind Plasma , 1991 .
[90] W. Matthaeus,et al. Models of inertial range spectra of interplanetary magnetohydrodynamic turbulence , 1990 .
[91] C. T. Dum. Simulation studies of plasma waves in the electron foreshock: The generation of Langmuir waves by a gentle bump‐on‐tail electron distribution , 1990 .
[92] G. P. M. Poppe,et al. More efficient computation of the complex error function , 1990, TOMS.
[93] P. Diamond,et al. Clouds and holes: self-organization in compressible fluid and collisionless plasma turbulence , 1989 .
[94] A. Hasegawa,et al. Excitation of kinetic Alfven waves by resonant mode conversion and longitudinal heating of magnetized plasmas , 1989 .
[95] William H. Press,et al. Book-Review - Numerical Recipes in Pascal - the Art of Scientific Computing , 1989 .
[96] John Ambrosiano,et al. Test particle acceleration in turbulent reconnecting magnetic fields , 1988 .
[97] C. Tu. The damping of interplanetary Alfvénic fluctuations and the heating of the solar wind , 1988 .
[98] S. Gary,et al. Instabilities in Space and Laboratory Plasmas , 1987 .
[99] A. Hasegawa,et al. MACROSCALE PARTICLE SIMULATION OF KINETIC ALFVEN WAVES , 1987 .
[100] I. Cairns. The electron distribution function upstream from the Earth's bow shock , 1987 .
[101] C. Tu. A solar wind model with the power spectrum of Alfvénic fluctuations , 1987 .
[102] M. Goldman,et al. Microstructures in type III events in the solar wind , 1987 .
[103] W. Matthaeus,et al. Turbulent magnetic reconnection , 1986 .
[104] J. V. Hollweg. Transition region, corona, and solar wind in coronal holes , 1986 .
[105] D. Melrose. Instabilities in Space and Laboratory Plasmas: MHD instabilities , 1986 .
[106] A. V. Ballegooijen,et al. Cascade of magnetic energy as a mechanism of coronal heating , 1985 .
[107] 若谷 誠宏. A. A. Galeev and R. N. Sudan 編: Handbook of Plasma Physics, Vol. 1; Basic Plasma Physics, 1 and 2, North-Holland, Amsterdam and New York, 1983, 1984, 2vols., 24.5×17.5cm, 1: 51,000円, 2: 43,560円. , 1985 .
[108] Z. Pu,et al. The power spectrum of interplanetary Alfvénic fluctuations: Derivation of the governing equation and its solution , 1984 .
[109] V. A. Turikov. Electron Phase Space Holes as Localized BGK Solutions , 1984 .
[110] P. Isenberg. The ion cyclotron dispersion relation in a proton‐alpha solar wind , 1984 .
[111] S. Schwartz,et al. The radial evolution of a single solar wind plasma parcel , 1983 .
[112] W. Matthaeus,et al. Magnetohydrodynamic turbulence in the solar wind , 1999 .
[113] John V. Shebalin,et al. Anisotropy in MHD turbulence due to a mean magnetic field , 1983, Journal of Plasma Physics.
[114] E. Marsch,et al. Wave heating and acceleration of solar wind ions by cyclotron resonance , 1982 .
[115] P. Isenberg,et al. On the preferential acceleration and heating of solar wind heavy ions , 1982 .
[116] T. H. Dupree. Theory of phase‐space density holes , 1982 .
[117] George L. Withbroe,et al. Probing the solar wind acceleration region using spectroscopic techniques , 1982 .
[118] D. Montgomery. Major disruptions, inverse cascades, and the Strauss equations. [Current-carrying plasmas] , 1982 .
[119] S. Schwartz,et al. The source of proton anisotropy in the high‐speed solar wind , 1981 .
[120] J. Hollweg,et al. Ion-cyclotron heating and acceleration of solar wind minor ions , 1981 .
[121] T. Tatsumi. Theory of Homogeneous Turbulence , 1980 .
[122] D. Eichler. Particle acceleration in solar flares by cyclotron damping of cascading turbulence , 1979 .
[123] U. Feldman,et al. Measurements of extreme-ultraviolet emission-line profiles near the solar limb. , 1978 .
[124] J. Hollweg,et al. Some physical processes in the solar wind , 1978 .
[125] J. Hollweg,et al. Acceleration of solar wind He++3. Effects of resonant and nonresonant interactions with transverse waves , 1978 .
[126] S. A. Jacques. Momentum and energy transport by waves in the solar atmosphere and solar wind. , 1977 .
[127] W. Feldman,et al. Nonlinear alfven waves in high speed solar wind streams , 1977 .
[128] A. Hasegawa. Particle acceleration by MHD surface wave and formation of aurora , 1976 .
[129] M. Brereton. Classical Electrodynamics (2nd edn) , 1976 .
[130] H. R. Strauss,et al. Nonlinear, three‐dimensional magnetohydrodynamics of noncircular tokamaks , 1976 .
[131] J. Hollweg,et al. Alfven waves in a two-fluid model of the solar wind , 1973 .
[132] J. Thompson. Nonlinear Evolution of Collisionless Electron Beam‐Plasma Systems , 1971 .
[133] T. Toichi. Thermal properties of the solar wind plasma , 1971 .
[134] R. Stéfant. Alfven wave damping from finite gyroradius coupling to the ion acoustic mode , 1970 .
[135] D. A. Dunnett. Classical Electrodynamics , 2020, Nature.
[136] A. Barnes. COLLISIONLESS HEATING OF THE SOLAR-WIND PLASMA. I. THEORY OF THE HEATING OF COLLISIONLESS PLASMA BY HYDROMAGNETIC WAVES. , 1968 .
[137] Robert L. Carovillano,et al. Physics of the magnetosphere , 1968 .
[138] C. E. Leith,et al. Diffusion Approximation to Inertial Energy Transfer in Isotropic Turbulence , 1967 .
[139] Robert H. Kraichnan,et al. Inertial‐Range Spectrum of Hydromagnetic Turbulence , 1965 .
[140] Y. Pao. Structure of Turbulent Velocity and Scalar Fields at Large Wavenumbers , 1965 .
[141] Burton D. Fried,et al. The Plasma Dispersion Function , 1961 .
[142] I. Bernstein,et al. Waves in a Plasma in a Magnetic Field , 1958 .
[143] M. Kruskal,et al. Exact Nonlinear Plasma Oscillations , 1957 .
[144] D. E. Kerr. Physics of Fully Ionized Gases. , 1956 .
[145] G. Batchelor,et al. The theory of homogeneous turbulence , 1954 .
[146] A. Townsend. On the fine-scale structure of turbulence , 1951, Proceedings of the Royal Society of London. Series A. Mathematical and Physical Sciences.
[147] S. Chandrasekhar. Stochastic problems in Physics and Astronomy , 1943 .