13 citations as recorded by crossref.

1. Kinetic scale turbulence and dissipation in the solar wind: key observational results and future outlook M. Goldstein et al. https://doi.org/10.1098/rsta.2014.0147
2. The origin of reconnection-mediated transient brightenings in the solar transition region S. Bahauddin et al. https://doi.org/10.1038/s41550-020-01263-2
3. The Solar Orbiter Solar Wind Analyser (SWA) suite C. Owen et al. https://doi.org/10.1051/0004-6361/201937259
4. The Role of Proton Cyclotron Resonance as a Dissipation Mechanism in Solar Wind Turbulence: A Statistical Study at Ion-kinetic Scales L. Woodham et al. https://doi.org/10.3847/1538-4357/aab03d
5. Three-dimensional magnetic reconnection in particle-in-cell simulations of anisotropic plasma turbulence J. Agudelo Rueda et al. https://doi.org/10.1017/S0022377821000404
6. Energy Transport during 3D Small-scale Reconnection Driven by Anisotropic Plasma Turbulence J. Agudelo Rueda et al. https://doi.org/10.3847/1538-4357/ac8667
7. Alfvén Reflection and Reverberation in the Solar Atmosphere P. Cally https://doi.org/10.1007/s11207-012-0052-3
8. Modeling Transition Region Hot Loops on the Sun: The Necessity of Rapid, Complex Spatiotemporal Heating and Nonequilibrium Ionization S. Bahauddin & S. Bradshaw https://doi.org/10.3847/1538-4357/ad5a86
9. Reflection of Alfvén waves in the corona and solar wind: An impulse function approach J. Hollweg & P. Isenberg https://doi.org/10.1029/2007JA012253
10. The Damping and Instability of Ion-acoustic Waves in the Solar Wind: Solar Orbiter Observations H. Ran 冉 et al. https://doi.org/10.3847/1538-4357/ae60fb
11. The need to consider ion Bernstein waves as a dissipation channel of solar wind turbulence J. Podesta https://doi.org/10.1029/2012JA017770
12. Dependence of Solar Wind Proton Temperature on the Polarization Properties of Alfvénic Fluctuations at Ion-kinetic Scales L. Woodham et al. https://doi.org/10.3847/1538-4357/abed51
13. Preferential Heating of Particles by H-Cyclotron Waves Generated by a Global Magnetohydrodynamic Mode in Solar Coronal Holes T. Zhang https://doi.org/10.1086/379798