Image Details

Choose export citation format:

Magnetic Rayleigh–Taylor Interchange Shapes Chiral Barbs in Solar Prominences

  • Authors: Hongyang Luo, Yuhong Fan

Hongyang Luo and Yuhong Fan 2026 The Astrophysical Journal Letters 1010 .

  • Provider: AAS Journals

Caption: Figure 1.

Observed and simulated right-bearing filament barbs. (A) Hα observation of a dextral filament with right-bearing barbs extending from the filament spine, adapted from A. A. van Ballegooijen (2005). Red plus and green minus symbols mark the positive and negative photospheric magnetic polarities, respectively, and the white arrow indicates the inferred axial-field direction. (B) Top view of the synthetic AIA 304 Å emission. The simulated prominence develops similarly oriented right-bearing barbs along its spine, reproducing the characteristic morphology of a dextral filament. The polarity symbols and white arrow schematically indicate the corresponding polarity arrangement and axial-field direction.

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse