# Large-amplitude longitudinal oscillations in a solar filament

**Authors:** Q. M. Zhang, T. Li, R. S. Zheng, Y. N. Su, and H. S. Ji

arXiv: 1705.04820 · 2017-06-21

## TL;DR

This study presents multiwavelength observations of large-amplitude longitudinal oscillations in a solar filament, revealing complex behaviors, spatial dependence, and the influence of mass drainage, with implications for understanding filament dynamics.

## Contribution

It provides detailed observational analysis of filament oscillations, including their spatial variation, damping, and growth, and introduces a schematic model for thread interactions.

## Key findings

- Oscillations had periods of 3100-4400 s with spatial dependence.
- Amplitudes ranged from a few to ten Mm, velocities up to 30 km/s.
- Mass drainage occurred without stopping the oscillations.

## Abstract

In this paper, we report our multiwavelength observations of the large-amplitude longitudinal oscillations of a filament on 2015 May 3. Located next to active region 12335, the sigmoidal filament was observed by the ground-based H$\alpha$ telescopes from GONG and by AIA aboard SDO. The filament oscillations were most probably triggered by the magnetic reconnection in the filament channel. The directions of oscillations have angles of 4$^\circ$-36$^\circ$ with respect to the filament axis. The whole filament did not oscillate in phase as a rigid body. Meanwhile, the periods (3100$-$4400 s) of oscillations have a spatial dependence. The values of $R$ are estimated to be 69.4$-$133.9 Mm, and the minimum transverse magnetic field of the dips is estimated to be 15 G. The amplitudes of S5-S8 grew with time, while the amplitudes of S9-S14 damped with time. The amplitudes of oscillations range from a few to ten Mm, and the maximal velocity can reach 30 km s$^{-1}$. Interestingly, the filament experienced mass drainage southwards at a speed of $\sim$27 km s$^{-1}$. The oscillations continued after the mass drainage and lasted for more than 11 hr. After the mass drainage, the phases of oscillations did not change a lot. The periods of S5-S8 decreased, while the periods of S9-S14 increased. The amplitudes of S5$-$S8 damped with time, while the amplitudes of S9-S14 grew. Most of the damping (growing) ratios are between -9 and 14. We propose a schematic cartoon to explain the complex behaviors of oscillations by introducing thread-thread interaction.

## Full text

_Full body text omitted from this summary view._ Fetch the complete paper as Markdown: https://tomesphere.com/paper/1705.04820/full.md

## Figures

16 figures with captions in the complete paper: https://tomesphere.com/paper/1705.04820/full.md

## References

78 references — full list in the complete paper: https://tomesphere.com/paper/1705.04820/full.md

---
Source: https://tomesphere.com/paper/1705.04820