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• W2557030818 abstract "We report on the amplitude of the density turbulence spectrum ($C_{N}^{2}$) and the density modulation index ($delta N/N$) in the solar wind between $10$ and $45 R_{odot}$. We derive these quantities using a structure function that is observationally constrained by occultation observations of the Crab nebula made in 2011 and 2013 and similar observations published earlier. We use the most general form of the structure function, together with currently used prescriptions for the inner/dissipation scale of the turbulence spectrum. Our work yields a comprehensive picture of a) the manner in which $C_{N}^{2}$ and $delta N/N$ vary with heliocentric distance in the solar wind and b) of the solar cycle dependence of these quantities." @default.
• W2557030818 created "2016-11-30" @default.
• W2557030818 creator A5048322690 @default.
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• W2557030818 creator A5088193310 @default.
• W2557030818 date "2016-12-01" @default.
• W2557030818 modified "2023-10-15" @default.
• W2557030818 title "Amplitude of solar wind density turbulence from 10 to 45 <i>R</i>_⊙" @default.
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• W2557030818 doi "https://doi.org/10.1002/2016ja023254" @default.
• W2557030818 hasPublicationYear "2016" @default.
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