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Shaaban M. S. Hamd
Qatar UniversityMeeting roles in:
Cumulative effects of drift, temperature anisotropies, and suprathermal populations on the right-hand proton instabilities in the young solar wind
Multiscale Description of Solar Wind Dynamics: Quasilinear Theory, Simulations, and Observations Poster
Boundaries of the “Brazil Plots” for Solar Wind Protons, Core-and-halo Electrons, and Alpha Particles
Modeling strong perpendicular anisotropies in proton beams in the young solar wind: linear and quasilinear approaches
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