Simulating Three-Wave Interactions and the Resulting Particle Transport Coefficients in a Magnetic Loop by Seve Nyberg, Rami Vainio

Subjects: “…Alfvén waves…”
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Nonlinear dynamics of phase space zonal structures and energetic particle physics in fusion plasmas by F Zonca, L Chen, S Briguglio, G Fogaccia, G Vlad, X Wang

Subjects: “…Alfvèn waves…”
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Generation of Vertical Flows by Torsional Alfvén Pulses in Zero-beta Tubes with a Transitional Layer by Joseph Scalisi, Michael S. Ruderman, Robertus Erdélyi

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Research progress on in-flight calibration of the magnetometer in deep space exploration by Guoqiang Wang

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Generation of auroral turbulence through the magnetosphere–ionosphere coupling by Tomo-Hiko Watanabe, Hiroaki Kurata, Shinya Maeyama

Subjects: “…Alfvén waves…”
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Review and comparison of MHD wave characteristics at the Sun and in Earth’s magnetosphere by Chelpanov M. A., Anfinogentov S. A., Kostarev D. V., Mikhailova O. S., Rubtsov A. V., Fedenev V. V., Chelpanov A. A.

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Clockwise and counter clockwise 6 & 9 year geostrophic MC (& Rossby) waves in centre of the mechanism of geomagnetic jerks and relevant LODs by Mohsen LUTEPHY, Botir Berdiyorovich ISMAILOV, Adnan Hashim ABDULKADHIM

Subjects: “…geological and geophysical evidences of deep processes, core dynamics, geodynamo, alfvén wave, hall-mhd model, numerical simulation, geomagnetic jerk, lod variation, perturbation theory, modulational instability, decay, rogue wave, nonlinear schrödinger equation, alfvénic turbulences…”
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Plasma Magnetohydrodynamics and Energy Conversion by Shapiro, A. H., Heiser, W. H., Heywood, J. B., Penhune, J. P., Jackson, W. D., Cooper, R. S., East, D. A., Barnett, G. O., Brown, G. A., Kerrebrock, J. L., Carabateas, E. N., Lewis, A. T., Kliman, G. B., Carson, J. F., Lee, K. S., Porter, R. P., Pruslin, D. H., Gadzuk, J. W.

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Coronal Holes by Steven R. Cranmer

Subjects: “…Alfven waves…”
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The Alfvén resonator revisited by A. M. Hamza, W. Lyatsky

“…In both models the instability arises because of the generation of an Alfvén wave from growing arc-like structures in the ionospheric conductivity. …”
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Anisotropy of solar wind turbulence between ion and electron scales. by Chen, C, Horbury, T, Schekochihin, A, Wicks, RT, Alexandrova, O, Mitchell, J

“…The spectral index of the perpendicular component is -2.6 at large angles and -3 at small angles, in broad agreement with critically balanced whistler and kinetic Alfvén wave predictions. For the parallel component, however, it is shallower than -1.9, which is considerably less steep than predicted for a kinetic Alfvén wave cascade.…”

Modeling the Solar Wind during Different Phases of the Last Solar Cycle by Zhenguang Huang, Gábor Tóth, Nishtha Sachdeva, Lulu Zhao, Bart van der Holst, Igor Sokolov, Ward B. Manchester, Tamas I. Gombosi

“…We describe our first attempt to systematically simulate the solar wind during different phases of the last solar cycle with the Alfvén Wave Solar atmosphere Model (AWSoM) developed at the University of Michigan. …”
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Multi-channel coupling of decay instability in three-dimensional low-beta plasma by H. Comişel, H. Comişel, Y. Narita, Y. Narita, U. Motschmann, U. Motschmann

“…<p>Three-dimensional hybrid simulations have been carried out to verify the hypothesis of simultaneous multi-channel decay of a large-amplitude Alfvén wave in a low-beta plasma, e.g., in the shock-upstream region or the solar corona. …”
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A Model of Turbulence in Magnetized Plasmas: Implications for the Dissipation Range in the Solar Wind by Howes, G, Cowley, S, Dorland, W, Hammett, G, Quataert, E, Schekochihin, A

“…Wave phase velocity measurements are consistent with a kinetic Alfven wave cascade and not the onset of ion cyclotron damping. …”

From small-scale dynamo to isotropic MHD turbulence by Schekochihin, A, Cowley, S, Taylor, S, Maron, J, McWilliams, J

“…There is no scale-by-scale equipartition between magnetic and kinetic energies as would be the case for the Alfvén-wave turbulence. The isotropic MHD turbulence is the end state of the turbulent dynamo which generates folded fields with small-scale direction reversals. …”

From Small-Scale Dynamo to Isotropic MHD Turbulence by Schekochihin, A, Cowley, S, Taylor, S, Maron, J, McWilliams, J

“…There is no scale-by-scale equipartition between magnetic and kinetic energies as would be the case for the Alfven-wave turbulence. The isotropic MHD turbulence is the end state of the turbulent dynamo which generates folded fields with small-scale direction reversals. …”

Gyrokinetic simulations of solar wind turbulence from ion to electron scales. by Howes, G, TenBarge, J, Dorland, W, Quataert, E, Schekochihin, A, Numata, R, Tatsuno, T

“…Despite the strongly nonlinear nature of the turbulence, the linear kinetic Alfvén wave mode quantitatively describes the polarization of the turbulent fluctuations. …”

A stringent limit on the amplitude of alfvénic perturbations in high-beta low-collisionality plasmas by Squire, J, Quataert, E, Schekochihin, A

“…Such a restrictive bound on shear-Alfvén-wave amplitudes has far-reaching implications for the physics of magnetized turbulence in the high-β conditions prevalent in many astrophysical plasmas, as well as for the solar wind at ∼1 au where β ≳ 1.…”

Dissipation-Scale Turbulence in the Solar Wind by Howes, G, Cowley, S, Dorland, W, Hammett, G, Quataert, E, Schekochihin, A

“…We present a cascade model for turbulence in weakly collisional plasmas that follows the nonlinear cascade of energy from the large scales of driving in the MHD regime to the small scales of the kinetic Alfven wave regime where the turbulence is dissipated by kinetic processes. …”

Dissipation-scale turbulence in the solar wind by Howes, G, Cowley, S, Dorland, W, Hammett, G, Quataert, E, Schekochihin, A

“…We present a cascade model for turbulence in weakly collisional plasmas that follows the nonlinear cascade of energy from the large scales of driving in the MHD regime to the small scales of the kinetic Alfvén wave regime where the turbulence is dissipated by kinetic processes. …”