Characterize the 3D magnetic structure of the Sun and Heliosphere during the current solar activity minimum.
Follow the evolution and effects of the Sun’s radiative output, magnetic field and outflowing solar wind plasma
as they interact with the background heliosphere and with the magnetospheres and atmospheres of the Earth and other Planets.
Compare the current minimum with previous solar minima and investigate how periods of extremely low solar activity
affect the geospace and other planetary space environments.
Embrace latest advances in data collection, management, analysis, and communication and set the stage for the next
generation of collaborative Heliophysics System Observatory research.