Travis Metcalfe will present a reanalysis of stellar rotation using direct magnetic field measurements and X-ray mass-loss rates. Dr. Metcalfe will demonstrate how wind braking torque decreases abruptly as stars approach a critical Rossby number, suggesting the Sun is currently transitioning into a suppressed magnetic state.
This hybrid event is held in person at Center Green 1, room 3131, and
virtually via Google Meet. No registration is required for this session.
Dr. Metcalfe currently serves as a Senior Research Scientist and Executive Director at the Center for Solar-Stellar Connections at the White Dwarf Research Corporation (WDRC). This research provides a new physical basis for understanding the limitations of gyrochronology in older stars.