The Turbulent Cascade at 1 AU: Energy Transfer and the Third-Order Scaling for MHD

By B. T. MacBride, Charles W. Smith, M. Forman. 2007

188 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/7924df8ffded3e57f0bd2e971dd03400685daf67

How researchers see this paper

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In Astronomy and Astrophysics

1. S. Cranmer
2. E. Quataert
3. William H. Matthaeus
4. B. Chandran
5. Ben Breech
6. S. Oughton
7. S. Bale
8. T. Dennis

Citations in the corpus

• Electron and proton heating by solar wind turbulence (2009, background): “An active MHD turbulent cascade [MacBride et al., 2008; Marino et al., 2008] transfers energy from the large-scale fluctuations down to small scales where kinetic processes dissipate the energy as heat.”
• INCORPORATING KINETIC PHYSICS INTO A TWO-FLUID SOLAR-WIND MODEL WITH TEMPERATURE ANISOTROPY AND LOW-FREQUENCY ALFVÉN-WAVE TURBULENCE (2011, background): “Moreover, the amplitudes of these turbulent fluctuations are sufficient to explain the heating rates thathave been inferred from the proton and electron temperature profiles (Smith et al. 2001; MacBride et al. 2008; Cranmer et al. 2009; Stawarz et al. 2009).”
• EMPIRICAL CONSTRAINTS ON PROTON AND ELECTRON HEATING IN THE FAST SOLAR WIND (2009, background): “2001; Vasquez et al. 2007; MacBride et al. 2008; Marino et al. 2008; Breech et al. 2008).”