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Alfvénic fluctuations in the expanding solar wind: Formation and radial evolution of spherical polarization
DOI: 10.1063/5.0177754 Bibcode: 2024PhPl...31c2901M

Hellinger, P.; Matteini, L.; Horbury, T. S. +7 more

We investigate properties of large-scale solar wind Alfvénic fluctuations and their evolution during radial expansion. We assume a strictly radial background magnetic field B ∥ R, and we use two-dimensional hybrid (fluid electrons, kinetic ions) simulations of balanced Alfvénic turbulence in the plane orthogonal to B; the simulated plasma evolves …

2024 Physics of Plasmas
Ulysses 11
Kinetic numerical scaling of Alfven cyclotron instability in non-thermal solar wind plasmas
DOI: 10.1063/5.0204224 Bibcode: 2024PhPl...31h2110S

Shahzad, Muhammad Ahsan; Aman-ur-Rehman; Bilal, Muhammad +3 more

Linear plasma kinetic theory for a non-thermal, magnetized, homogeneous, and collisionless plasma is incorporated to study Alfvén cyclotron instability (ACI) driven by the ion/proton perpendicular temperature anisotropy (T⊥p/T∥p>1) ( ⊥, ∥ symbols designate directions perpendicular and parallel to ambient magnetic field, respectively), and the w…

2024 Physics of Plasmas
Ulysses 1
Role of nonlinear structures and associated turbulence generation dayside magnetosphere reconnection sites
DOI: 10.1063/5.0172154 Bibcode: 2024PhPl...31b2104P

Sharma, R. P.; Pathak, Neha; Sharma, Suresh C. +1 more

A numerical simulation is implemented to investigate the role of whistler wave in the presence of the ponderomotive force-driven density modification and the magnetic field perturbation due to preexisting magnetic islands. The dynamical equation governing the whistler waves is derived and solved using numerical methods to assess their role. The si…

2024 Physics of Plasmas
Cluster 0