Turbulent transport in stellar radiative zones

被引:0
|
作者
Lignières, F [1 ]
Toqué, N [1 ]
Vincent, A [1 ]
机构
[1] Observ Midi Pyrenees, Lab Astrophys Toulouse & Tarbes, F-31400 Toulouse, France
关键词
D O I
10.1051/eas:2005116
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Abundances anomalies and helioseismology provide constraints on the turbulent transport of chemical species in stellar radiative zone. We use these constraints to derive upper bounds oil the velocity and lengthscale of the vertical turbulent motions. We also present numerical simulations showing that a strong anisotropy between horizontal and vertical motions could help understand the observed transport.
引用
收藏
页码:209 / 214
页数:6
相关论文
共 50 条
  • [31] Effect of Gravity Waves on Transport Process in Stellar Radiative Region
    E. Schatzman
    Astrophysics and Space Science, 1999, 265 : 97 - 97
  • [32] Effect of gravity waves on transport process in stellar radiative region
    Schatzman, E
    ASTROPHYSICS AND SPACE SCIENCE, 1999, 265 (1-4) : 97 - 97
  • [33] Modeling turbulent stellar convection zones: Sub-grid scales effects
    Strugarek, A.
    Beaudoin, P.
    Brun, A. S.
    Charbonneau, P.
    Mathis, S.
    Smolarkiewicz, P. K.
    ADVANCES IN SPACE RESEARCH, 2016, 58 (08) : 1538 - 1553
  • [34] Some properties of the kinetic energy flux and dissipation in turbulent stellar convection zones
    Meakin, Casey A.
    Arnett, W. David
    ASTROPHYSICS AND SPACE SCIENCE, 2010, 328 (1-2) : 221 - 225
  • [35] Some properties of the kinetic energy flux and dissipation in turbulent stellar convection zones
    Casey A. Meakin
    W. David Arnett
    Astrophysics and Space Science, 2010, 328 : 221 - 225
  • [36] The diffusion-circulation coupling in stellar radiative zones:: 2D simulation
    Théado, S
    Vauclair, S
    STELLAR ROTATION, 2004, (215): : 354 - 355
  • [37] LOW MACH AND PECLET NUMBER LIMIT FOR A MODEL OF STELLAR TACHOCLINE AND UPPER RADIATIVE ZONES
    Donatelli, Donatella
    Ducomet, Bernard
    Kobera, Marek
    Necasova, Sarka
    ELECTRONIC JOURNAL OF DIFFERENTIAL EQUATIONS, 2016,
  • [38] STRESS TRANSPORT IN THE ROTATIONAL AND IRROTATIONAL ZONES OF TURBULENT SHEAR FLOWS
    BYGGSTOYL, S
    KOLLMANN, W
    PHYSICS OF FLUIDS, 1986, 29 (05) : 1423 - 1429
  • [39] Stellar Energetic Particle Transport in the Turbulent and CME-disrupted Stellar Wind of AU Microscopii
    Fraschetti, Federico
    Alvarado-Gomez, Julian D.
    Drake, Jeremy J.
    Cohen, Ofer
    Garraffo, Cecilia
    ASTROPHYSICAL JOURNAL, 2022, 937 (02):
  • [40] RADIATIVE TRANSPORT MODEL FOR MICROWAVE SCATTERING FROM TURBULENT PLASMA
    FEINSTEI.DL
    GRANATST.VL
    BULLETIN OF THE AMERICAN PHYSICAL SOCIETY, 1968, 13 (11): : 1566 - &