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Detailed Reference Information |
Hartlep, T., Matthaeus, W.H., Padhye, N.S. and Smith, C.W. (2000). Magnetic field strength distribution in interplanetary turbulence. Journal of Geophysical Research 105: doi: 10.1029/1999JA000223. issn: 0148-0227. |
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The distribution of magnetic field magnitudes is derived for the special case of a constant mean field and uncorrelated components having Gaussian distributions. Of the three cases considered (isotropic, transverse, and axisymmetric) the latter most closely resembles a lognormal distribution when the parallel variance is less than the perpendicular variance. Thus a normally distributed, nonintermittent vector field can produce a magnitude distribution that closely resembles a functional form often associated with models of intermittency. This result is illustrated by comparison with a magnetic field magnitude distribution computed from the 1 AU Omni dataset. The parameters of the Gaussian component magnitude distribution can be chosen to compare with the data which is also well fit as a lognormal type. We conclude that the magnitude distribution may not be a sensitive indicator of intermittency and that further examination of the sensitivity of such indicators is warranted. ¿ 2000 American Geophysical Union |
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Abstract |
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Keywords
Interplanetary Physics, Interplanetary magnetic fields, Interplanetary Physics, Solar wind plasma, Space Plasma Physics, Turbulence |
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Publisher
American Geophysical Union 2000 Florida Avenue N.W. Washington, D.C. 20009-1277 USA 1-202-462-6900 1-202-328-0566 service@agu.org |
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