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Title: Spatial Correlation of Solar-Wind Turbulence from Two-Point Measurements

Abstract

Interplanetary turbulence, the best studied case of low frequency plasma turbulence, is the only directly quantified instance of astrophysical turbulence. Here, magnetic field correlation analysis, using for the first time only proper two-point, single time measurements, provides a key step in unraveling the space-time structure of interplanetary turbulence. Simultaneous magnetic field data from the Wind, ACE, and Cluster spacecraft are analyzed to determine the correlation (outer) scale, and the Taylor microscale near Earth's orbit.

Authors:
;  [1];  [2]; ;  [3];  [4]
  1. Bartol Research Institute, Department of Physics and Astronomy, University of Delaware, Newark, Delaware 19716 (United States)
  2. Instituto de Astronomia y Fisica del Espacio (IAFE) and Departamento de Fisica, Facultad de Ciencias Exactas y Naturales, Universidad de Buenos Aires, 1428 Buenos Aires (Argentina)
  3. IGPP, UCLA, Los Angeles, California 90095 (United States)
  4. Institute for Earth, Oceans and Space, University of New Hampshire, Durham, New Hampshire 03824 (United States)
Publication Date:
OSTI Identifier:
20699636
Resource Type:
Journal Article
Resource Relation:
Journal Name: Physical Review Letters; Journal Volume: 95; Journal Issue: 23; Other Information: DOI: 10.1103/PhysRevLett.95.231101; (c) 2005 The American Physical Society; Country of input: International Atomic Energy Agency (IAEA)
Country of Publication:
United States
Language:
English
Subject:
71 CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; 70 PLASMA PHYSICS AND FUSION TECHNOLOGY; ASTRONOMY; CORRELATIONS; INTERPLANETARY MAGNETIC FIELDS; PLASMA; SOLAR WIND; SPACE-TIME; TIME MEASUREMENT; TURBULENCE

Citation Formats

Matthaeus, W.H., Milano, L.J., Dasso, S., Weygand, J.M., Kivelson, M.G., and Smith, C.W. Spatial Correlation of Solar-Wind Turbulence from Two-Point Measurements. United States: N. p., 2005. Web. doi:10.1103/PhysRevLett.95.231101.
Matthaeus, W.H., Milano, L.J., Dasso, S., Weygand, J.M., Kivelson, M.G., & Smith, C.W. Spatial Correlation of Solar-Wind Turbulence from Two-Point Measurements. United States. doi:10.1103/PhysRevLett.95.231101.
Matthaeus, W.H., Milano, L.J., Dasso, S., Weygand, J.M., Kivelson, M.G., and Smith, C.W. Fri . "Spatial Correlation of Solar-Wind Turbulence from Two-Point Measurements". United States. doi:10.1103/PhysRevLett.95.231101.
@article{osti_20699636,
title = {Spatial Correlation of Solar-Wind Turbulence from Two-Point Measurements},
author = {Matthaeus, W.H. and Milano, L.J. and Dasso, S. and Weygand, J.M. and Kivelson, M.G. and Smith, C.W.},
abstractNote = {Interplanetary turbulence, the best studied case of low frequency plasma turbulence, is the only directly quantified instance of astrophysical turbulence. Here, magnetic field correlation analysis, using for the first time only proper two-point, single time measurements, provides a key step in unraveling the space-time structure of interplanetary turbulence. Simultaneous magnetic field data from the Wind, ACE, and Cluster spacecraft are analyzed to determine the correlation (outer) scale, and the Taylor microscale near Earth's orbit.},
doi = {10.1103/PhysRevLett.95.231101},
journal = {Physical Review Letters},
number = 23,
volume = 95,
place = {United States},
year = {Fri Dec 02 00:00:00 EST 2005},
month = {Fri Dec 02 00:00:00 EST 2005}
}
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