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Abstract: Modeling strong perpendicular anisotropies in proton beams in the young solar wind: linear and quasilinear approaches (AGU25)

Modeling strong perpendicular anisotropies in proton beams in the young solar wind: linear and quasilinear approaches

Shaaban M. S. Hamd, Qatar University, Doha, Qatar, Marian Lazar, Katholieke Universiteit Leuven, Department of Mathematics, Leuven, Belgium, Peter H Yoon, Univ Maryland, College Park, MD, United States, Rodrigo Lopez, Comision Chilena de Energia Nuclear, Santiago, Chile and Stefaan Poedts, KU Leuven, Centre for mathematical Plasma-Astrophysics, Leuven, Belgium
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