Image Details
Caption: Figure 7.
Temporal evolution of the WEF for the Alfvén wave packet at the different positions on the slit S3 (see Figure 5). Here the dotted line and the solid line respectively correspond to kinetic and total energy (kinetic+magnetic) associated with the WEF. At point “a” the packet has an energy flux of about 2140 W m−2, which then decreases gradually at the different points owing to the curved magnetic field. Thereafter it reaches a constant value of 860 W m−2 and propagates up to very far distance along the horizontal field line.
© 2026. The Author(s). Published by the American Astronomical Society.