Planetary magnetospheric convection models: The Dungey cycle and the Vasyliūnas cycle

Key Points

• The Dungey cycle describes magnetosphere dynamics, demonstrating how magnetic fields interact with plasma.
• Key phenomena include the transport and mixing of plasma in magnetospheric convection, influencing space weather.
• Observational analysis across various planetary systems highlights features of the Vasyliūnas cycle in magnetospheric behavior.
• Findings suggest a better understanding of these cycles may enhance predictions of plasma interactions in space.