15 citations as recorded by crossref.

1. Modeling Ion Beams, Kinetic Instabilities, and Waves Observed by the Parker Solar Probe near Perihelia L. Ofman et al. 10.3847/1538-4357/ac402c
2. Kinetic cascade beyond magnetohydrodynamics of solar wind turbulence in two-dimensional hybrid simulations D. Verscharen et al. 10.1063/1.3682960
3. Ion acceleration by parallel propagating nonlinear Alfvén wave packets in a radially expanding plasma Y. Nariyuki et al. 10.5194/npg-21-339-2014
4. ION HEATING IN INHOMOGENEOUS EXPANDING SOLAR WIND PLASMA: THE ROLE OF PARALLEL AND OBLIQUE ION-CYCLOTRON WAVES N. Ozak et al. 10.1088/0004-637X/799/1/77
5. On nonlinear evolution of low-frequency Alfvén waves in weakly-expanding solar wind plasmas Y. Nariyuki 10.1063/1.4908544
6. The effects of inhomogeneous proton‐α drifts on the heating of the solar wind L. Ofman et al. 10.1002/2016JA023705
7. Computational and theoretical study of the wave-particle interaction of protons and waves P. Moya et al. 10.5194/angeo-30-1361-2012
8. Observations and Modeling of Unstable Proton and α Particle Velocity Distributions in Sub-Alfvénic Solar Wind at Parker Solar Probe Perihelia L. Ofman et al. 10.3847/1538-4357/acea7e
9. Current Sheets, Plasmoids and Flux Ropes in the Heliosphere O. Pezzi et al. 10.1007/s11214-021-00799-7
10. Relative drifts and temperature anisotropies of protons andαparticles in the expanding solar wind: 2.5D hybrid simulations Y. Maneva et al. 10.1051/0004-6361/201424401
11. WEAK TURBULENCE CASCADING EFFECTS IN THE ACCELERATION AND HEATING OF IONS IN THE SOLAR WIND P. Moya et al. 10.1088/0004-637X/781/2/76
12. Kinetic instabilities in the solar wind driven by temperature anisotropies P. Yoon 10.1007/s41614-017-0006-1
13. DISSIPATION OF PARALLEL AND OBLIQUE ALFVÉN-CYCLOTRON WAVES—IMPLICATIONS FOR HEATING OF ALPHA PARTICLES IN THE SOLAR WIND Y. Maneva et al. 10.1088/0004-637X/814/1/33
14. Nonlinear Evolution of Ion Kinetic Instabilities in the Solar Wind L. Ofman 10.1007/s11207-019-1440-8
15. First Principles Description of Plasma Expansion Using the Expanding Box Model S. Echeverría-Veas et al. 10.3390/universe9100448