Using Third-Order Moments of Fluctuations in V and B to Determine Turbulent Heating Rates in the Solar Wind

被引：1

作者：

Forman, M. A. ^{[1
]}

Smith, C. W. ^{[2
]}

Vasquez, B. J. ^{[2
]}

MacBride, B. T. ^{[3
]}

Stawarz, J. E. ^{[2
]}

Podesta, J. J. ^{[4
]}

Elton, D. C. ^{[5
]}

Malecot, U. Y. ^{[6
]}

Gagne, Y. ^{[7
]}

机构：

[1] SUNY Stony Brook, Stony Brook, NY 11794 USA

[2] Univ New Hampshire, Space Sci Inst Earth Oceans & Atmospheres, Durham, NH 03824 USA

[3] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA

[4] Los Alamos Natl Lab, Space Sci & Applicat, Los Alamos, NM 87545 USA

[5] Rensselaer Polytech Inst, Dept Phys, Troy, NY 12180 USA

[6] Univ Grenoble 1, F-38041 Grenoble 9, France

[7] CNRS, Lab Ecoul Geophys Ind, UJF INPG, UMR 5519, F-338041 Grenoble, France

来源：

TWELFTH INTERNATIONAL SOLAR WIND CONFERENCE | 2010年 / 1216卷

关键词：

MHD; Turbulence; Theory; Solar Wind; 1; AU; CASCADE; MHD;

D O I：

10.1063/1.3395830

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The inertial range scaling of certain mixed third-order moments of velocity and magnetic field fluctuations in a turbulent MHD plasma such as the solar wind is related to the energy dissipation rate of the turbulence. We have used this relation to measure energy dissipation rates in the solar wind and other statistical methods to estimate the accuracy of these measurements. This paper reviews results we and others have recently published, and some new results.

引用

页码：176 / +

页数：2

共 7 条

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