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- W2134333776 endingPage "L24" @default.
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- W2134333776 abstract "We investigate the radial dependence of the spectral break separating the inertial from the dissipation range in power density spectra of interplanetary magnetic field fluctuations, between $0.42$ and $5.3$ AU, during radial alignments between MESSENGER and WIND for the inner heliosphere and between WIND and ULYSSES for the outer heliosphere. We found that the spectral break moves to higher and higher frequencies as the heliocentric distance decreases. The radial dependence of the corresponding wavenumber is of the kind $kappa_bsim R^{-1.08}$ in good agreement with that of the wavenumber derived from the linear resonance condition for proton cyclotron damping. These results support conclusions from previous studies which suggest that a cyclotron-resonant dissipation mechanism must participate into the spectral cascade together with other possible kinetic noncyclotron-resonant mechanisms." @default.
- W2134333776 created "2016-06-24" @default.
- W2134333776 creator A5048169710 @default.
- W2134333776 creator A5077847387 @default.
- W2134333776 date "2014-05-14" @default.
- W2134333776 modified "2023-10-17" @default.
- W2134333776 title "RADIAL DEPENDENCE OF THE FREQUENCY BREAK BETWEEN FLUID AND KINETIC SCALES IN THE SOLAR WIND FLUCTUATIONS" @default.
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- W2134333776 doi "https://doi.org/10.1088/2041-8205/787/2/l24" @default.
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