most citedMagnetized winds of M-type stars and star-planet magnetic interactions: uncertainties and modeling strategy

10 citations · 30 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.SR2025★ 1 cited

A parametric study of solar wind properties and composition using fluid and kinetic solar wind models

Paul Lomazzi, Alexis P. Rouillard, Michael A. Lavarra +7

The physical processes in the solar corona that shape the solar wind remain an active research topic. Modeling efforts have shown that energy and plasma exchanges near the transiti…

astro-ph.SR2025★ 3 cited

On stellar hotspots due to star-planet magnetic interactions: How much power can actually be transmitted to the chromosphere?

Arghyadeep Paul, Antoine Strugarek, Victor Réville

Star-Planet Magnetic Interactions (SPMI) have been proposed as a mechanism for generating stellar hot-spots with energy outputs on the order of watts. This interaction…

astro-ph.SR2024★ 10 cited

Magnetized winds of M-type stars and star-planet magnetic interactions: uncertainties and modeling strategy

Victor Réville, Jamie M. Jasinski, Marco Velli +6

M-type stars are the most common stars in the universe. They are ideal hosts for the search of exoplanets in the habitable zone (HZ), as their small size and low temperature make t…

astro-ph.SR2024★ 7 cited

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…

astro-ph.SR2024★ 9 cited

Dominance of 2-Minute Oscillations near the Alfvén Surface

Zesen Huang, Marco Velli, Chen Shi +11

Alfvén waves, considered one of the primary candidates for heating and accelerating the fast solar wind, are ubiquitous in spacecraft observations, yet their origin remains elusive…