Continuous outflow of magnetised plasma from the solar corona — slow component (~400 km/s, dense) from streamers, fast component (~750 km/s) from coronal holes. Carries the heliospheric magnetic field outward to the heliopause.
Continuous outflow of magnetised plasma from the solar corona — slow component (~400 km/s, dense) from streamers, fast component (~750 km/s) from coronal holes. Carries the heliospheric magnetic field outward to the heliopause.