2 papers
astro-ph.SR2026
Magnetic Connectivity in the Time-Dependent Corona and Heliosphere
Roberto Lionello, Cooper Downs, Emily I. Mason +3
Magnetic flux fills the heliosphere, expands outward from the solar corona, and is fundamentally related to the structure and dynamics of the solar corona and solar wind. Open magn…
astro-ph.SR2024
Near subsonic solar wind outflow from an active region
Tamar Ervin, Stuart D. Bale, Samuel T. Badman +10
During Parker Solar Probe (Parker) Encounter 15 (E15), we observe an 18-hour period of near subsonic ( 1) and sub-Alfvénic (SA), <<< 1, slow speed…