Image Details
Caption: Figure B1.
Snapshots of temperature (left column), pressure (middle column), and field-aligned velocity (right column) along an emerged field line shown at four time instances: t = 3.87 hr (1st row), t = 4.36 hr (second row), t = 4.56 hr (3rd row), and t = 8.70 hr (4th row). The sequence captures the transition from a hot coronal state to rapid cooling at the field-line dip, followed by persistent field-aligned inflows toward the condensation.
© 2026. The Author(s). Published by the American Astronomical Society.