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astro-ph.SR2026

On the Radial Evolution of the Solar Wind : The Source Alignment Method Applied to Parker Solar Probe and Solar Orbiter Observations

Jean-Baptiste Dakeyo, Tamar Ervin, Stuart Bale +10

The properties of the solar wind, as measured in situ throughout the heliosphere, depend both on the characteristics of its coronal source and on the intrinsic processes governing…

astro-ph.SR2025

Proton specific entropy as a proxy for the charge state ratio over heliocentric distance

Jack D. Collard, Tamar Ervin, Ryan M. Dewey +10

While the fast solar wind has well-established origins in coronal holes, the source of the slow solar wind remains uncertain. Compositional metrics, such as heavy ion charge state…

astro-ph.SR2025

On the Propagation and Damping of Alfvenic Fluctuations in the Outer Solar Corona and Solar Wind

Nikos Sioulas, Marco Velli, Chen Shi +17

We analyze \textit{Parker Solar Probe} and \textit{Solar Orbiter} observations to investigate the propagation and dissipation of Alfvénic fluctuations from the outer corona to 1~A…

astro-ph.SR2025

Generalized Two Thermal Regimes Approach : Bipoly Fluid Modeling

J-B. Dakeyo, P. Démoulin, A. P. Rouillard +3

The isopoly bi-fluid approach assumes an isothermal evolution of the solar wind near the Sun up to the radial distance riso, followed by a polytropic evolution constrained by the o…

astro-ph.SR2024

Testing the flux tube expansion factor -- solar wind speed relation with Solar Orbiter data

J-B. Dakeyo, A. P. Rouillard, V. Réville +5

The properties of the solar wind measured in-situ in the heliosphere are largely controlled by energy deposition in the solar. Previous studies have shown that long duration and la…