SOLAR-WIND TURBULENCE;
MAGNETIC RECONNECTION;
CASCADE;
D O I:
10.1063/1.5128376
中图分类号:
O35 [流体力学];
O53 [等离子体物理学];
学科分类号:
070204 ;
080103 ;
080704 ;
摘要:
The spectral properties associated with laminar, anti-parallel reconnection are examined using a 2.5D kinetic particle in cell simulation. Both the reconnection rate and the energy spectrum exhibit three distinct phases: an initiation phase where the reconnection rate grows, a quasi-steady phase, and a declining phase where both the reconnection rate and the energy spectrum decrease. During the steady phase, the energy spectrum exhibits approximately a double power law behavior, with a slope near -5/3 at wave numbers smaller than the inverse ion inertial length and a slope steeper than -8/3 for larger wave numbers up to the inverse electron inertial length. This behavior is consistent with a Kolmogorov energy cascade and implies that laminar reconnection may fundamentally be an energy cascade process. Consistent with this idea is the fact that the reconnection rate exhibits a rough correlation with the energy spectrum at wave numbers near the inverse ion inertial length. The 2D spectrum is strongly anisotropic with most energy associated with the wave vector direction normal to the current sheet. Reconnection acts to isotropize the energy spectrum, reducing the Shebalin angle from an initial value of 70 degrees to about 48 degrees (nearly isotropic) by the end of the simulation. The distribution of energy over length scales is further analyzed by dividing the domain into spatial subregions and employing structure functions.
机构:
Princeton Univ, Dept Astrophys Sci, Princeton, NJ 08544 USA
Princeton Univ, Princeton Plasma Phys Lab, Princeton, NJ 08540 USA
Columbia Univ, Dept Astron, New York, NY 10027 USA
Columbia Univ, Columbia Astrophys Lab, 538 W 120th St, New York, NY 10027 USAPrinceton Univ, Dept Astrophys Sci, Princeton, NJ 08544 USA
机构:
Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USAUniv Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA
Eastwood, J. P.
;
Phan, T. D.
论文数: 0引用数: 0
h-index: 0
机构:
Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USAUniv Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA
Phan, T. D.
;
Bale, S. D.
论文数: 0引用数: 0
h-index: 0
机构:
Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA
Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USAUniv Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA
Bale, S. D.
;
Tjulin, A.
论文数: 0引用数: 0
h-index: 0
机构:
Univ London Imperial Coll Sci Technol & Med, Blackett Lab, London SW7 2BW, EnglandUniv Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA
机构:
Princeton Univ, Dept Astrophys Sci, Princeton, NJ 08544 USA
Princeton Univ, Princeton Plasma Phys Lab, Princeton, NJ 08540 USA
Columbia Univ, Dept Astron, New York, NY 10027 USA
Columbia Univ, Columbia Astrophys Lab, 538 W 120th St, New York, NY 10027 USAPrinceton Univ, Dept Astrophys Sci, Princeton, NJ 08544 USA
机构:
Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USAUniv Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA
Eastwood, J. P.
;
Phan, T. D.
论文数: 0引用数: 0
h-index: 0
机构:
Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USAUniv Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA
Phan, T. D.
;
Bale, S. D.
论文数: 0引用数: 0
h-index: 0
机构:
Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA
Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USAUniv Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA
Bale, S. D.
;
Tjulin, A.
论文数: 0引用数: 0
h-index: 0
机构:
Univ London Imperial Coll Sci Technol & Med, Blackett Lab, London SW7 2BW, EnglandUniv Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA