2 papers
astro-ph.SR2026
Global Multi-ion Solar Wind Model. I. Ion Temperatures
Bart van der Holst, Judit Szente, Enrico Landi
Over the past several decades, observations have shown that minor ions have a higher temperature and flow faster than protons in the solar wind. Theories based on turbulence have b…
astro-ph.SR2024
Mapping the Sun's coronal magnetic field using the Zeeman effect
Thomas A. Schad, Gordon J. D. Petrie, Jeffrey R. Kuhn +9
Regular remote sensing of the magnetic field embedded within the million-degree solar corona is severely lacking. This reality impedes fundamental investigations of the nature of c…