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Researchers find potential mechanism of solar light bridge formation and penumbra disappearance

Researchers find potential mechanism of solar light bridge formation and penumbra disappearance
Horizontal velocity around the sunspot derived by DAVE4VM. The background image shows the vertical magnetic field (the positive field is shown in white and the negative field is shown in black). The arrows represent horizontal velocity. Blue (red) arrows indicate that the vertical magnetic fields in the pixels are positive (negative). The green contours show the outer boundary of the sunspot (I = 0.9Iqs). Credit: The Astrophysical Journal (2023). DOI: 10.3847/1538-4357/aca667

Sunspots are the most noticeable manifestation of solar magnetic field concentrations in the photosphere. A typical mature sunspot has an umbra and a penumbra. Light bridges (LBs) are the strip-like bright features, two ends of which connect the penumbra and span the umbra of a sunspot.

Commonly, the appearance of light bridges is an indication of decay or fragmentation. The evolution of is closely related to solar eruptions, e.g., , , and filament eruptions. However, up to now, the formation and decay mechanisms of sunspots were poorly understood.

Researchers led by Prof. Yan Xiaoli from Yunnan Observatories of the Chinese Academy of Sciences (CAS) and Li Qiaoling from Yunnan University analyzed the decay process of a sunspot in active region NOAA 12680 on the sun by using the calibrated data from the Solar Dynamics Observatory/Helioseismic and Magnetic Imaging (SDO/HMI), and discussed the influence of the light bridge on a decaying sunspot.

The results were published in The Astrophysical Journal on Jan. 11.

The researchers found that at the beginning of sunspot decay, some elongated dark structures were gradually separated from the umbra. The intensity, vertical field strength and magnetic inclination of these dark structures were between those of the umbra and penumbra. With the formation of a light bridge, the total magnetic flux of the whole penumbra region gradually decreased, and part of the penumbra located on one side of the light bridge rapidly disappeared.

In addition, after the appearance of an outward motion of magnetic flux along the light bridge, the decay rate of the area and magnetic flux of the penumbral sector rapidly deceased. These results suggested that the rapid decay of the penumbral sector was correlated with the light bridge.

"The dark structure in the penumbra and the formation of light bridge may be the result of magnetic flux spreading out from the umbra, which may accelerate the decay of the sunspot," said Prof. Yan.

More information: Qiaoling Li et al, Rapid Decay of a Penumbral Sector Associated with a Strong Light Bridge in Active Region NOAA 12680, The Astrophysical Journal (2023). DOI: 10.3847/1538-4357/aca667

Journal information: Astrophysical Journal

Citation: Researchers find potential mechanism of solar light bridge formation and penumbra disappearance (2023, January 18) retrieved 21 May 2024 from
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