THEORY OF INCOMPRESSIBLE MAGNETOHYDRODYNAMIC TURBULENCE WITH SCALE-DEPENDENT ALIGNMENT AND CROSS-HELICITY

被引:44
作者
Podesta, J. J. [1 ]
Bhattacharjee, A. [1 ]
机构
[1] Univ New Hampshire, Ctr Integrated Computat & Anal Reconnect & Turbul, Durham, NH 03824 USA
关键词
solar wind; turbulence; waves; MAGNETO-HYDRODYNAMIC TURBULENCE; MHD TURBULENCE; HYDROMAGNETIC TURBULENCE; FLUCTUATIONS; SIMULATIONS; SPECTRUM; FIELD;
D O I
10.1088/0004-637X/718/2/1151
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A phenomenological anisotropic theory of MHD turbulence with nonvanishing cross-helicity is constructed based on Boldyrev's phenomenology and probabilities p and q for fluctuations delta v(perpendicular to). and delta b(perpendicular to) to be positively or negatively aligned. The positively aligned fluctuations occupy a fractional volume p and the negatively aligned fluctuations occupy a fractional volume q. Guided by observations suggesting that the normalized cross-helicity sigma(c) and the probabilities p and q are approximately scale invariant in the inertial range, a generalization of Boldyrev's theory is derived that depends on the three ratios w(+)/w(-), is an element of(+)/is an element of(-), and p/q. It is assumed that the cascade processes for positively and negatively aligned fluctuations are both in a state of critical balance and that the eddy geometries are scale invariant. The theory reduces to Boldyrev's original theory when sigma(c) = 0, is an element of(+) = is an element of(-), and p = q and extends the theory of Perez and Boldyrev when sigma(c) not equal 0. The theory is also an anisotropic generalization of the theory of Dobrowolny, Mangeney, and Veltri.
引用
收藏
页码:1151 / 1157
页数:7
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