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Researchers Discover Solar Jets Come from Eruption of Mini-filaments

Sep 29, 2019

Solar jets are straight or bi-directional plasma flows, and they are ubiquitous in the solar atmosphere. Studying of solar jets are very important for understanding the enigmatic problems of coronal heating and the acceleration of solar wind. However, knowledge on the formation of solar jets is still scarce.

A jet often started from the eruption of a mini-filament due to magnetic cancellation or some instabilities, the confining magnetic fields first reconnect with the ambient open or horizontal field lines, and then, due to the rising of the filament, magnetic reconnection will occur underneath the filament resembling the eruption of large filaments.

In a recent study published in The Astrophysical Journal, a research group led by Dr. SHEN Yuandeng from Yunnan Observatories of the Chinese Academy of Sciences found that both straight and two-sided-loop jets are evolved from the eruption of mini-filaments located at the jet base, and experience two times magnetic reconnection process. The findings are new to the understanding of the formation of solar jets.

Based on high resolution multi-wavelength and stereoscopic observations taken by the Solar Dynamic Observatory and the Solar Terrestrial Relations Observatory, the researchers found that the basic formation mechanisms for the two kinds of solar jets are similar, and both of them include the eruption of a mini-filament and undergo two times of magnetic reconnection processes. However, due to different magnetic topologies, they result in different outcomes.

For a straight jet moving along open magnetic field lines, it often results in simultaneous jet-like and bubble-like coronal mass ejections. For a two-sided-loop jet along horizontal and closed loop, it cannot cause coronal mass ejections in the outer corona.

These findings not only indicated the similarity of small- and large-scale solar eruptions, but also advanced the understanding of the formation mechanism of solar jets.

 

The formation mechanism of the two types of solar jets. The top row is for straight jets, while the bottom row is for two-sided-loop jets. The red dashed lines indicate the reconnection positions, while the orange circle represents the mini-filament. The black and blue lines represent the magnetic field lines before and after the magnetic reconnections. Symbols ‘+' and ‘-' indicate the positive and negative magnetic polarities. (Image by SHEN Yuandeng) 

Contact

SHEN Yuandeng

Yunnan Observatories

E-mail:

Stereoscopic Observations of an Erupting Mini-filament-driven Two-sided-loop Jet and the Applications for Diagnosing a Filament Magnetic Field

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