29 citations · 38 across the 3 of their papers we have counts for
3 papers
Quasilinear Consequences of Turbulent Ion Heating by Magnetic Moment Breaking
Philip A. Isenberg, Bernard J. Vasquez, Joseph V. Hollweg
The fast solar wind emerging from coronal holes is likely heated and accelerated by the dissipation of magnetohydrodynamic turbulence, but the specific kinetic mechanism resulting…
Ultraviolet Coronagraph Spectroscopy: A Key Capability for Understanding the Physics of Solar Wind Acceleration
S. R. Cranmer, J. L. Kohl, D. Alexander +21
Understanding the physical processes responsible for accelerating the solar wind requires detailed measurements of the collisionless plasma in the extended solar corona. Some key c…
The Turbulent Heating Rate in Strong MHD Turbulence with Nonzero Cross Helicity
Benjamin D. G. Chandran, Eliot Quataert, Gregory G. Howes +2
Different results for the cascade power in strong, incompressible MHD turbulence with nonzero cross helicity appear in the literature. In this paper, we discuss the conditions unde…