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• W2785272930 endingPage "49" @default.
• W2785272930 startingPage "49" @default.
• W2785272930 abstract "We use magnetic field and ion moment data from the MFI and SWE instruments on board the Wind spacecraft to study the nature of solar wind turbulence at ion-kinetic scales. We analyze the spectral properties of magnetic field fluctuations between 0.1 and 5.4 Hz during 2012 using an automated routine, computing high-resolution 92 s power and magnetic helicity spectra. To ensure the spectral features are physical, we make the first in-flight measurement of the MFI noise-floor using tail-lobe crossings of the Earth's magnetosphere during early 2004. We utilize Taylor's hypothesis to Doppler-shift into the spacecraft frequency frame, finding that the spectral break observed at these frequencies is best associated with the proton cyclotron resonance scale, 1/kc, rather than the proton inertial length, di, or proton gyroscale, ρi. This agreement is strongest when we consider periods where , and is consistent with a spectral break at di for and at ρi for . We also find that the coherent magnetic helicity signature observed at these frequencies is bounded at low frequencies by 1/kc, and its absolute value reaches a maximum at ρi. These results hold in both slow and fast wind streams, but with a better correlation in the more Alfvénic fast wind where the helicity signature is strongest. We conclude that these findings are consistent with proton cyclotron resonance as an important mechanism for dissipation of turbulent energy in the solar wind, occurring at least half the time in our selected interval. However, we do not rule out additional mechanisms." @default.
• W2785272930 created "2018-02-02" @default.
• W2785272930 creator A5003940393 @default.
• W2785272930 creator A5041456476 @default.
• W2785272930 creator A5070199237 @default.
• W2785272930 creator A5075436034 @default.
• W2785272930 date "2018-03-23" @default.
• W2785272930 modified "2023-10-16" @default.
• W2785272930 title "The Role of Proton Cyclotron Resonance as a Dissipation Mechanism in Solar Wind Turbulence: A Statistical Study at Ion-kinetic Scales" @default.
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