Observations of the Formation and Disappearance of a Funnel Prominence
Bo Yang, Jiayan Yang, Yi Bi, and Junchao Hong

TL;DR
This observational study details the dynamic formation and disappearance processes of a funnel prominence, highlighting the roles of coronal loop evolution, plasma flows, and magnetic reconnection in prominence lifecycle.
Contribution
It provides new insights into the formation and disappearance mechanisms of funnel prominences through detailed observational analysis.
Findings
Cool plasma flows along coronal loops contribute to prominence formation.
Magnetic reconnection may drive vertical downflows leading to prominence disappearance.
U-shaped coronal loops and coronal cavity dynamics are key to prominence evolution.
Abstract
We present an observational study of the formation and disappearance of a funnel prominence. Before the funnel prominence formed, cool materials from the top of a preexisting polar crown prominence flowed along saddle-shaped coronal loops to their base, forming a smaller prominence. Meanwhile, the saddle-shaped coronal loops gradually rose, and U-shaped coronal loops, termed prominence horns, began to appear along with a coronal cavity. Afterwards, a cool column emerged from the chromosphere, rose vertically into the corona, and then moved laterally to be transported into the U-shaped coronal loops. The formed prominence slid into the chromosphere, while the U-shaped coronal loops and the coronal cavity became more pronounced. As cool materials accumulated at the base of the U-shaped coronal loops, these loops underwent a significant descent and a V-shaped structure appeared at the base…
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Taxonomy
TopicsGeophysics and Gravity Measurements
