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20242026
most citedEvolution of an Alfvén Wave-Driven Proton Beam in the Expanding Solar Wind

3 citations · 3 across the 8 of their papers we have counts for

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physics.plasm-ph2026

Nonlinear Tearing Modes in Current-Vortex Sheets

D. Urbanski, F. L. Waelbroeck, A. Tenerani

The linear and nonlinear development of instabilities and Alfvén resonances in a plane current-vortex sheet is presented here for sheared equilibrium profiles $\boldsymbol{B_{y0}}…

physics.plasm-ph2026

Three dimensional, spherically polarized magnetic fields

Anna Tenerani, Marco Velli

Turbulence in the solar wind is characterized by Alfvénic fluctuations that exhibit spherical polarization, a geometric condition resulting in the nearly constant magnitude of the…

physics.plasm-ph2026

Characterization of compressible fluctuations in solar wind streams dominated by balanced and imbalanced turbulence: Parker Solar Probe, Solar Orbiter and Wind observations

C. A. Gonzalez, C. Gonzalez, A. Tenerani

Characterizing compressible fluctuations in the solar wind is essential for understanding their role in solar wind acceleration and heating, yet their origin and evolution across d…

physics.plasm-ph2026

Resistive instabilities of current sheets in stratified plasmas with a gravitational field

Faisal Sayed, Anna Tenerani, Richard Fitzpatrick

Magnetic reconnection can develop spontaneously via the tearing instability, often invoked to explain disruptive instabilities in fusion devices, solar flares, the generation of pe…

physics.plasm-ph2024

Unified Framework of Forced Magnetic Reconnection and Alfven Resonance

D. Urbanski, A. Tenerani, F. L. Waelbroeck

A unified linear theory that includes forced reconnection as a particular case of Alfvén resonance is presented. We consider a generalized Taylor problem in which a sheared magnet…