Statistical Analysis of Field-Aligned Alfvenic Turbulence and Intermittency in Fast Solar Wind

被引：4
作者：
Carbone, Francesco [1 ]
Telloni, Daniele [2 ]
Sorriso-Valvo, Luca [3 ,4 ]
Zank, Gary [5 ,6 ]
Zhao, Lingling [5 ]
Adhikari, Laxman [5 ]
Bruno, Roberto [7 ]
机构：
[1] Univ Calabria, Natl Res Council, Inst Atmospher Pollut Res, I-87036 Arcavacata Di Rende, Italy
[2] Astrophys Observ Torino, Natl Inst Astrophys, Via Osservatorio 20, I-10025 Pino Torinese, Italy
[3] Escuela Politec Nacl, Dept Fis, Ladron De Guevera E11-253, Quito 170517, Ecuador
[4] CNR, Ist Sci & Tecnol Plasmi, Via Amendola 122-D, I-70126 Bari, Italy
[5] Univ Alabama Huntsville, Ctr Space Plasma & Aeron Res CSPAR, Huntsville, AL 35899 USA
[6] Univ Alabama Huntsville, Dept Space Sci, Huntsville, AL 35899 USA
[7] Natl Inst Astrophys, Inst Space Astrophys & Planetol, Via Fosso Cavaliere 100, I-00133 Rome, Italy
来源：
UNIVERSE | 2020年 / 6卷 / 08期
关键词：
solar wind; turbulence; scaling laws; EMPIRICAL MODE DECOMPOSITION; INTERSTELLAR TURBULENCE; INERTIAL-RANGE; ANISOTROPY; FLUCTUATIONS; SPECTRUM; WAVES; POWER;
D O I：
10.3390/universe6080116
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The statistical properties of fast Alfvenic solar wind turbulence have been analyzed by means of empirical mode decomposition and the associated Hilbert spectral analysis. The stringent criteria employed for the data selection in the Wind spacecraft database, has made possible to sample multiple k(parallel to) field-aligned intervals of the three magnetic field components. The results suggest that the spectral anisotropy predicted by the critical balance theory is not observed in the selected database, whereas a Kolmogorov-like scaling (E(k(parallel to)) similar to k(-5/3)) and a weak or absent level of intermittency are robust characteristics of the Alfvenic slab component of solar wind turbulence.
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页数：14
相关论文
共 64 条
  • [1] [Anonymous], 2004, Int. J. of Wavelets, DOI [10.1142/S0219691304000561, DOI 10.1142/S0219691304000561]
  • [2] Structure functions in turbulence, in various flow configurations, at Reynolds number between 30 and 5000, using extended self-similarity
    Arneodo, A
    Baudet, C
    Belin, F
    Benzi, R
    Castaing, B
    Chabaud, B
    Chavarria, R
    Ciliberto, S
    Camussi, R
    Chilla, F
    Dubrulle, B
    Gagne, Y
    Hebral, B
    Herweijer, J
    Marchand, M
    Maurer, J
    Muzy, JF
    Naert, A
    Noullez, A
    Peinke, J
    Roux, F
    Tabeling, P
    vandeWater, W
    Willaime, H
    [J]. EUROPHYSICS LETTERS, 1996, 34 (06): : 411 - 416
  • [3] STATISTICAL PROPERTIES OF MHD FLUCTUATIONS ASSOCIATED WITH HIGH-SPEED STREAMS FROM HELIOS-2 OBSERVATIONS
    BAVASSANO, B
    DOBROWOLNY, M
    FANFONI, G
    MARIANI, F
    NESS, NF
    [J]. SOLAR PHYSICS, 1982, 78 (02) : 373 - 384
  • [4] EXTENDED SELF-SIMILARITY IN TURBULENT FLOWS
    BENZI, R
    CILIBERTO, S
    TRIPICCIONE, R
    BAUDET, C
    MASSAIOLI, F
    SUCCI, S
    [J]. PHYSICAL REVIEW E, 1993, 48 (01): : R29 - R32
  • [5] Spectrum of magnetohydrodynamic turbulence
    Boldyrev, S
    [J]. PHYSICAL REVIEW LETTERS, 2006, 96 (11)
  • [6] Boos D., 2010, Significance, V7, P186, DOI DOI 10.1111/J.1740-9713.2010.00463.X
  • [7] The Solar Wind as a Turbulence Laboratory
    Bruno, Roberto
    Carbone, Vincenzo
    [J]. LIVING REVIEWS IN SOLAR PHYSICS, 2013, 10 (02) : 7 - +
  • [8] Sea surface temperature variation linked to elemental mercury concentrations measured on Mauna Loa
    Carbone, F.
    Landis, M. S.
    Gencarelli, C. N.
    Naccarato, A.
    Sprovieri, F.
    De Simone, F.
    Hedgecock, I. M.
    Pirrone, N.
    [J]. GEOPHYSICAL RESEARCH LETTERS, 2016, 43 (14) : 7751 - 7757
  • [9] Clustering of elastic energy due to electrohydrodynamics instabilities in nematic liquid crystals
    Carbone, F.
    Yoshida, H.
    Suzuki, S.
    Fujii, A.
    Strangi, G.
    Versace, C.
    Ozaki, M.
    [J]. EPL, 2010, 89 (04)
  • [10] CARBONE F, 2019, ATMOSPHERE-BASEL, V10, DOI DOI 10.3390/atmos10100611
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