Energization of Charged Test Particles in Magnetohydrodynamic Fields: Waves versus Turbulence Picture

被引:1
作者
Pugliese, F. [1 ,2 ]
Brodiano, M. [1 ,2 ]
Andres, N. [2 ,3 ]
Dmitruk, P. [1 ,2 ]
机构
[1] Univ Buenos Aires, CONICET, Inst Fis Interdisciplinaria & Aplicada INFINA, Ciudad Univ, RA-1428 Buenos Aires, Argentina
[2] Univ Buenos Aires, Fac Ciencias Exactas & Nat, Dept Fis, Ciudad Univ, RA-1428 Buenos Aires, Argentina
[3] Univ Buenos Aires, CONICET, Inst Astron & Fis Espacio IAFE, Ciudad Univ, RA-1428 Buenos Aires, Argentina
关键词
SOLAR-WIND TURBULENCE; MAGNETIC RECONNECTION; ACCELERATION; TRANSPORT; MECHANISM; ENERGY;
D O I
10.3847/1538-4357/ad055b
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Direct numerical simulations of three-dimensional compressible magnetohydrodynamic (MHD) turbulence have been performed in order to study the relation between wave modes and coherent structures and the consequent energization of test particles. Moreover, the question of which is the main mechanism of this particle energization is rigorously discussed. In particular, using the same initial conditions, we analyzed the nonlinear and linear evolution of a turbulent state along with the case of randomized phases. Then, the behaviors of the linear and nonlinear simulations were compared through the study of the time evolution of particle kinetic energy and preferential concentration. Also, spatiotemporal spectra were used to identify the presence of wave modes and quantify the fraction of energy around the MHD modes in linear and nonlinear simulations. Finally, the variation of the correlation time of the external forcing is studied in detail along with the effect on the particle energization (and clustering) and the presence of wave modes. More specifically, particle energization tends to decrease when the fraction of linear energy increases, supporting the idea that energization by structures is the dominant mechanism for particle energization instead of resonance with wave modes as suggested by Fermi energization theory.
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页数:13
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共 65 条
  • [1] Turbulent cascades, transfer, and scale interactions in magnetohydrodynamics
    Alexakis, A.
    Mininni, P. D.
    Pouquet, A.
    [J]. NEW JOURNAL OF PHYSICS, 2007, 9
  • [2] The incompressible energy cascade rate in anisotropic solar wind turbulence
    Andres, N.
    Sahraoui, F.
    Huang, S.
    Hadid, L. Z.
    Galtier, S.
    [J]. ASTRONOMY & ASTROPHYSICS, 2022, 661
  • [3] The Evolution of Compressible Solar Wind Turbulence in the Inner Heliosphere: PSP, THEMIS, and MAVEN Observations
    Andres, N.
    Sahraoui, F.
    Hadid, L. Z.
    Huang, S. Y.
    Romanelli, N.
    Galtier, S.
    DiBraccio, G.
    Halekas, J.
    [J]. ASTROPHYSICAL JOURNAL, 2021, 919 (01)
  • [4] Interplay between Alfven and magnetosonic waves in compressible magnetohydrodynamics turbulence
    Andres, N.
    Clark di Leoni, P.
    Mininni, P. D.
    Dmitruk, P.
    Sahraoui, F.
    Matthaeus, W. H.
    [J]. PHYSICS OF PLASMAS, 2017, 24 (10)
  • [5] Effect of the electronic pressure on the energy and magnetic moment of charged test particles in turbulent electromagnetic fields
    Balzarini, B.
    Pugliese, F.
    Dmitruk, P.
    [J]. PHYSICS OF PLASMAS, 2022, 29 (12)
  • [6] Barnes A., 1979, SPACE PLASMA PHYS ST, V2, P257
  • [7] Dominant two-dimensional solar wind turbulence with implications for cosmic ray transport
    Bieber, JW
    Wanner, W
    Matthaeus, WH
    [J]. JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1996, 101 (A2) : 2511 - 2522
  • [8] A statistical study of the compressible energy cascade rate in solar wind turbulence: Parker solar probe observations
    Brodiano, M.
    Dmitruk, P.
    Andres, N.
    [J]. PHYSICS OF PLASMAS, 2023, 30 (03)
  • [9] Spatiotemporal Analysis of Waves in Compressively Driven Magnetohydrodynamics Turbulence
    Brodiano, M.
    Andres, N.
    Dmitruk, P.
    [J]. ASTROPHYSICAL JOURNAL, 2021, 922 (02)
  • [10] The Solar Wind as a Turbulence Laboratory
    Bruno, Roberto
    Carbone, Vincenzo
    [J]. LIVING REVIEWS IN SOLAR PHYSICS, 2013, 10 (02) : 7 - +