lifetime estimate for plasma turbulence
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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
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|---|---|
| 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
|
| URL | |
| Keywords |
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