Scientists reveal magnetic reconnection details triggering filament eruption

Eruption of a solar filament produces a coronal mass ejection, which is a major driver of space weather. Understanding how filaments erupt is thus essential for space weather forecasting.

Both observations and simulations suggest that filament eruption is closely related to magnetic flux emergence. It is thought that eruption is triggered by magnetic reconnection between a filament and an emerging flux. However, details of such a reconnection have rarely been presented.

Recently, a research team led by Dr. LI Leping from the National Astronomical Observatories of the Chinese Academy of Sciences (NAOC) has revealed the details of reconnection between a filament and its nearby emerging fields, which led to the reconfiguration and subsequent partial eruption of the filament.

The study was published in The Astrophysical Journal on Aug. 18.

In the active region NOAA 12816, a filament was located over the polarity inversion lines on April 21, 2021. Near the northwestern endpoints of the filament, magnetic fields emerged and reconnected with the filament, forming a newly reconnected filament and loops.

A current sheet repeatedly occurred at the interface of the filament and its nearby emerging fields. "In order to understand the detailed reconnection, we measured some parameters of the current sheets, such as the length, width, reconnection rate, temperature, emission measure, and electron number density," said Dr. LI, first author of the study.

Bright plasmoids formed in the current sheet, propagating along it bidirectionally, and further along the newly reconnected filament and loops. "This result indicates the presence of plasmoid instabilities during the reconnection process," said Prof. Hardi Peter from the Max-Planck Institute for Solar System Research, a co-author of the study.

The newly reconnected filament then erupted, while the unreconnected filament remained stable. The filament thus only partially erupted. "These results suggest that the reconnection-favored orientation of the emerging fields near the filament alone cannot result in the eruption of the whole filament," said Dr. LI. "Some other parameters, such as the position, distance, strength, and area, are also crucial for triggering the filament eruption."

Research Report:Reconfiguration and Eruption of a Solar Filament by Magnetic Reconnection with an Emerging Magnetic Field

Related Links
National Astronomical Observatories, Chinese Academy of Sciences
Solar Science News at SpaceDaily

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