VALIDITY TESTS OF THE MIXING-LENGTH THEORY OF DEEP CONVECTION

被引:51
|
作者
CHAN, KL [1 ]
SOFIA, S [1 ]
机构
[1] YALE UNIV,CTR SOLAR & SPACE RES,NEW HAVEN,CT 06511
关键词
D O I
10.1126/science.235.4787.465
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
引用
收藏
页码:465 / 467
页数:3
相关论文
共 50 条
  • [41] Double-diffusive mixing-length theory, semiconvection and massive star evolution
    Grossman, SA
    Taam, RE
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1996, 283 (04) : 1165 - 1178
  • [42] A STUDY OF CONVECTIVE MODEL STELLAR ATMOSPHERES USING A MODIFIED MIXING-LENGTH THEORY
    LESTER, JB
    LANE, MC
    KURUCZ, RL
    ASTROPHYSICAL JOURNAL, 1982, 260 (01): : 272 - 285
  • [43] A non-local mixing-length theory able to compute core overshooting
    Gabriel, M.
    Belkacem, K.
    ASTRONOMY & ASTROPHYSICS, 2018, 612
  • [44] DIFFERENCE-QUOTIENT TURBULENCE MODEL - A GENERALIZATION OF PRANDT MIXING-LENGTH THEORY
    EGOLF, PW
    PHYSICAL REVIEW E, 1994, 49 (02): : 1260 - 1268
  • [45] INSTABILITY DUE TO LOCAL MIXING-LENGTH APPROXIMATION
    KRUSKAL, M
    SCHWARZSCHILD, M
    HARM, R
    ASTROPHYSICAL JOURNAL, 1977, 214 (02): : 498 - 501
  • [46] A mixing-length model for shallow turbulent wakes
    Stansby, PK
    JOURNAL OF FLUID MECHANICS, 2003, 495 : 369 - 384
  • [47] Stellar evolution with a variable mixing-length parameter
    Trampedach, R
    Stein, RF
    Christensen-Dalsgaard, J
    Nordlund, Å
    THEORY AND TESTS OF CONVECTION IN STELLAR STRUCTURE: FIRST GRANADA WORKSHOP, 1999, 173 : 233 - 236
  • [48] Beyond the mixing-length treatment: Why and how?
    Zahn, JP
    THEORY AND TESTS OF CONVECTION IN STELLAR STRUCTURE: FIRST GRANADA WORKSHOP, 1999, 173 : 121 - 132
  • [49] Mixing-length parameter from binaries and clusters
    Yildiz, Mutlu
    ART OF MODELLING STARS IN THE 21ST CENTURY, 2008, (252): : 183 - 187