lifetime estimate for plasma turbulence

Clicks: 80
ID: 259092
2017
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Abstract
A method is proposed to experimentally determine the intrinsic timescale or a decay rate of turbulent fluctuations. The method is based on the assumption that the Breit–Wigner spectrum model with a non-Gaussian frequency broadening is valid in the data analysis. The decay rate estimate is applied to the multispacecraft magnetic field data in interplanetary space, yielding the decay rate on spatial scales of about 1000 km (about 10 times larger than the ion inertial length), which is higher than the theoretical predictions from the random sweeping timescale of the eddy turnover time. The faster decay of fluctuation components in interplanetary space is interpreted as a realization of plasma physical (and not fluid mechanical) processes.
Reference Key
narita2017nonlinearlifetime Use this key to autocite in the manuscript while using SciMatic Manuscript Manager or Thesis Manager
Authors ;Y. Narita;Y. Narita;Y. Narita;Z. Vörös;Z. Vörös;Z. Vörös
Journal BMC research notes
Year 2017
DOI
10.5194/npg-24-673-2017
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