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We extend the kinetic guiding-center model of collisionless coronal hole protons presented in Isenberg \& Vasquez to consider driving by imbalanced spectra of obliquely propagating ion-cyclotron waves. These waves are assumed to be a small by-product of the imbalanced turbulent cascade to high perpendicular wavenumber, and their total intensity is taken to be 1\% of the total fluctuation energy. We also extend the kinetic solutions for the proton distribution function in the resulting fast solar wind to heliocentric d ...
Published by: The Astrophysical Journal Published on: 08/2015
YEAR: 2015   DOI: 10.1088/0004-637X/808/2/119
Published by: \apj Published on: 10/2013
YEAR: 2013   DOI: 10.1088/0004-637X/776/1/45