Probability distribution function of self-organization of shear flows

被引:0
作者
Kim, Eun-jin [1 ]
Liu, Han-Li [2 ]
Anderson, Johan [1 ]
机构
[1] Univ Sheffield, Dept Appl Math, Sheffield, S Yorkshire, England
[2] Natl Ctr Atmospher Res, High Altitude Observ, POB 3000, Boulder, CO 80307 USA
来源
TWELFTH INTERNATIONAL SOLAR WIND CONFERENCE | 2010年 / 1216卷
基金
英国工程与自然科学研究理事会;
关键词
Shear flows; Self-organisation; Transport properties; PDFs; SOLAR TACHOCLINE; TURBULENCE; MODELS; EDGE;
D O I
暂无
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
we present a statistical theory of self-organisation of shear flows, modeled by a nonlinear diffusion equation driven by a stochastic forcing. A non-perturbative method based on a coherent structure is utilized for the prediction of the PDFs, showing strong intermittency with exponential tails. We confirm these results by numerical simulations. Furthermore, the results reveal a significant probability of supercritical states due to stochastic perturbation, which could have crucial implications in a variety of systems. To elucidate a crucial role of relative time scales of relaxation and disturbance in the determination of the PDFs, we present numerical simulation results obtained in a threshold model where the diffusion is given by discontinuous values. Our results highlight the importance of the statistical description of gradients, rather than their average value as has conventionally been done.
引用
收藏
页码:308 / +
页数:2
相关论文
共 25 条
  • [1] ANDERSON J, 2007, PLASMA PHYS CONTROL, V49, pS1
  • [2] The momentum flux probability distribution function for ion-temperature-gradient turbulence
    Anderson, Johan
    Kim, Eun-jin
    [J]. PHYSICS OF PLASMAS, 2008, 15 (05)
  • [3] Burgers turbulence
    Bec, Jeremie
    Khanin, Konstantin
    [J]. PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS, 2007, 447 (1-2): : 1 - 66
  • [4] Self-similarity properties of the probability distribution function of turbulence-induced particle fluxes at the plasma edge
    Carreras, BA
    van Milligen, B
    Hidalgo, C
    Balbin, R
    Sanchez, E
    Garcia-Cortes, I
    Pedrosa, MA
    Bleuel, J
    Endler, M
    [J]. PHYSICAL REVIEW LETTERS, 1999, 83 (18) : 3653 - 3656
  • [5] Avalanche models for solar flares
    Charbonneau, P
    McIntosh, SW
    Liu, HL
    Bogdan, TJ
    [J]. SOLAR PHYSICS, 2001, 203 (02) : 321 - 353
  • [6] Front propagation and critical gradient transport models
    Garbet, X.
    Sarazin, Y.
    Imbeaux, F.
    Ghendrih, P.
    Bourdelle, C.
    Guercan, Oe. D.
    Diamond, P. H.
    [J]. PHYSICS OF PLASMAS, 2007, 14 (12)
  • [7] HILDAGO C, 2002, NEW J PHYS, V4, P51, DOI DOI 10.1088/1367-2630/4/1/351
  • [8] Consistent theory of turbulent transport in two-dimensional magnetohydrodynamics
    Kim, EJ
    [J]. PHYSICAL REVIEW LETTERS, 2006, 96 (08)
  • [9] Gravity wave-driven flows in the solar tachocline. II. Stationary flows
    Kim, EJ
    MacGregor, KB
    [J]. ASTROPHYSICAL JOURNAL, 2003, 588 (01) : 645 - 654
  • [10] Self-consistent theory of turbulent transport in the solar tachocline - III. Gravity waves
    Kim, Eun-jin
    Leprovost, N.
    [J]. ASTRONOMY & ASTROPHYSICS, 2007, 468 (03) : 1025 - U129