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Suprathermal Proton Spectra at Interplanetary Shocks in Hybrid Simulations
Matthew A. Young, Bernard J. Vasquez, Harald Kucharek +1
Interplanetary shocks are one of the proposed sources of suprathermal ion populations (i.e., ions with energies of a few times the solar wind energy). Here, we present results from…
Perpendicular Ion Heating by Cyclotron Resonant Dissipation of Turbulently Generated Kinetic Alfvén Waves in the Solar Wind
Philip A. Isenberg, Bernard J. Vasquez
Solar wind ions are observed to be heated in the directions perpendicular to the large-scale magnetic field, with preferential heating given to heavy ions. In the solar corona, thi…
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…