Turbulence spectrum of interplanetary magnetic fluctuations and the rate of energy cascade

Charles W. Smith, Bernard J. Vasquez, Kathleen Hamilton, Benjamin T. MacBride, Jeffrey A. Tessein, Miriam A. Forman, Robert J. Leamon

Research output: Chapter in Book/Report/Conference proceedingConference contributionpeer-review

3 Scopus citations

Abstract

There is growing evidence that a turbulent cascade of energy from large to small scales accounts for the dissipation of fluid energy (magnetic and velocity fluctuations) that heats the background plasma. However, much remains to be done to understand the dynamics of that cascade. We apply a structure function formalism originally derived for hydrodynamic turbulence and recently extended to include magnetohydrodynamics (MHD) to map the cascade of energy in the inertial range at 1 AU. We also examine the anisotropies associated with inertial range magnetic fluctuations in the hope of better understanding inertial- and dissipation-range dynamics.

Original languageEnglish
Title of host publicationTURBULENCE AND NONLINEAR PROCESSES IN ASTROPHYSICAL PLASMAS
Subtitle of host publication6th Annual International Astrophysics Conference
Pages96-101
Number of pages6
DOIs
StatePublished - 2007
Externally publishedYes
EventTURBULENCE AND NONLINEAR PROCESSES IN ASTROPHYSICAL PLASMAS: 6th Annual International Astrophysics Conference - Oahu, HI, United States
Duration: Mar 16 2007Mar 22 2007

Publication series

NameAIP Conference Proceedings
Volume932
ISSN (Print)0094-243X
ISSN (Electronic)1551-7616

Conference

ConferenceTURBULENCE AND NONLINEAR PROCESSES IN ASTROPHYSICAL PLASMAS: 6th Annual International Astrophysics Conference
Country/TerritoryUnited States
CityOahu, HI
Period03/16/0703/22/07

Keywords

  • Anisotropy
  • Cascade
  • Interplanetary turbulence
  • Magnetic field
  • Solar wind

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