9 citations · 34 across the 9 of their papers we have counts for
9 papers
Quasilinear Wave "Reflection" Due to Proton Heating by an Imbalanced Turbulent Cascade
Philip A. Isenberg, Bernard J. Vasquez, Benjamin D. G. Chandran +1
We investigate the quasilinear effects of the resonant wave-particle interaction under conditions of imbalanced turbulent heating in the collisionless coronal hole. We find that ve…
A Kinetic Model of Solar Wind Generation and Heating by Kinetic Alfvén Wave Turbulence
Philip A. Isenberg, Bernard J. Vasquez
We present results from a kinetic model of collisionless gyrotropic coronal hole protons heated by cyclotron and Landau resonant dissipation of critically balanced kinetic Alfvén w…
HelioSwarm: A Multipoint, Multiscale Mission to Characterize Turbulence
Kristopher G. Klein, Harlan Spence, Olga Alexandrova +47
HelioSwarm (HS) is a NASA Medium-Class Explorer mission of the Heliophysics Division designed to explore the dynamic three-dimensional mechanisms controlling the physics of plasma…
Turbulence Driving by Interstellar Pickup Ions in the Outer Solar Wind
Philip A. Isenberg, Bernard J. Vasquez, Charles W. Smith
We revisit the question of how the unstable scattering of interstellar pickup ions (PUIs) may drive turbulence in the outer solar wind, and why the energy released into fluctuation…
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…