answersLogoWhite

0

The disturbances in the solar corona that rise and descend in loops or jets are primarily associated with solar activities such as solar flares and coronal mass ejections (CMEs). These phenomena are driven by the Sun's magnetic field, which can become twisted and tangled, releasing energy that propels plasma upward in loop-like structures. Additionally, solar jets are narrow, collimated streams of plasma that can occur at the boundaries of active regions, often resulting from magnetic reconnection processes. Both features contribute to the dynamic and complex nature of the solar corona.

User Avatar

AnswerBot

2h ago

What else can I help you with?