
Utilizing high-resolution knowledge from the one-meter New Vacuum Photo voltaic Telescope (NVST), a analysis workforce led by Prof. Yan Xiaoli from the Yunnan Observatories of the Chinese language Academy of Sciences (CAS) has performed an in-depth examine on the bodily properties and oscillations of chromospheric fibrils surrounding a quiescent filament.
The examine was revealed in Monthly Notices of the Royal Astronomical Society.
Specializing in a quiescent filament noticed by the NVST on November 1, 2023, the workforce analyzed 63 surrounding chromospheric fibrils.
By combining high-resolution Hα knowledge from the NVST with excessive ultraviolet (EUV) knowledge and line-of-sight magnetograms from the Photo voltaic Dynamics Observatory, in addition to full-disk photos from the Chinese language Hα Photo voltaic Explorer, the workforce found that whereas the orientations of the fibrils differed considerably on both facet of the filament, their different bodily properties have been related.
The evaluation revealed that the fibrils exhibited a variety of bodily properties, together with lifetimes of 150–650 seconds, widths of 0.32–0.85 megameters (Mm), most lengths of three–8.5 Mm, projection velocities of seven–29 km·s-1, and decelerations of 45–474 m·s-2.
To research the oscillatory properties of the fibrils, the workforce enhanced faint indicators utilizing a movement magnification algorithm. This system recognized transverse oscillations in some fibrils, with durations of 269–289 seconds and section speeds of 13.7–25.8 km·s-1, traits in step with magnetohydrodynamic kink waves.
Energy spectrum evaluation confirmed that the dominant oscillation durations have been concentrated within the vary of 4.8–6.6 minutes (288–396 seconds), comparable to a frequency vary of two.5–3.5 mHz. Moreover, the oscillation energy was considerably larger in fibril areas than in surrounding areas, peaking on the fibril roots.
Power estimates point out that the vitality flux carried by these waves ranges from 0.4 to six.5 W·m-2, which is inadequate to solely maintain chromospheric radiative loss.
The examine helps the idea that fibrils are pushed by magnetoacoustic shocks, offering new insights into vitality transport within the photo voltaic chromosphere. It additionally highlights the potential of the NVST’s excessive spatiotemporal decision for observing nice chromospheric buildings.
Extra info:
Qifan Dong et al, Properties of chromospheric fibrils round a quiescent filament, Month-to-month Notices of the Royal Astronomical Society (2025). DOI: 10.1093/mnras/staf1567
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Researchers use NVST high-resolution knowledge to check chromospheric fibrils round quiescent filament (2025, October 22)
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