# IRIS observations of magnetic interactions in the solar atmosphere   between pre-existing and emerging magnetic fields. II. UV emission properties

**Authors:** Salvo L. Guglielmino, Peter R. Young, Francesca Zuccarello

arXiv: 1812.07285 · 2018-12-19

## TL;DR

This study uses IRIS UV observations to analyze magnetic reconnection events in the solar atmosphere, revealing asymmetric emission profiles, plasma surges, and coronal counterparts to UV brightenings during flux emergence.

## Contribution

It provides a detailed characterization of UV emission and plasma dynamics associated with small-scale magnetic reconnection in active regions.

## Key findings

- Asymmetry in emission lines indicates complex plasma motions.
- Correlation between Doppler velocity and line skewness reveals dynamics.
- Detection of coronal emission confirms reconnection extends to higher layers.

## Abstract

Multi-wavelength ultraviolet (UV) observations by the IRIS satellite in active region NOAA 12529 have recently pointed out the presence of long-lasting brightenings, akin to UV bursts, and simultaneous plasma ejections occurring in the upper chromosphere and transition region during secondary flux emergence. These signatures have been interpreted as evidence of small-scale, recurrent magnetic reconnection episodes between the emerging flux region (EFR) and the pre-existing plage field. Here, we characterize the UV emission of these strong, intermittent brightenings and we study the surge activity above the chromospheric arch filament system (AFS) overlying the EFR. We analyze the surges and the cospatial brightenings observed at different wavelengths. We find an asymmetry in the emission between the blue and red wings of the Si IV 1402 \AA{} and Mg II k 2796.3 \AA{} lines, which clearly outlines the dynamics of the structures above the AFS that form during the small-scale eruptive phenomena. We also detect a correlation between the Doppler velocity and skewness of the Si IV 1394 \AA{} and 1402 \AA{} line profiles in the UV burst pixels. Finally, we show that genuine emission in the Fe XII 1349.4 \AA{} line is cospatial to the Si IV brightenings. This definitely reveals a pure coronal counterpart to the reconnection event.

## Full text

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## Figures

33 figures with captions in the complete paper: https://tomesphere.com/paper/1812.07285/full.md

## References

82 references — full list in the complete paper: https://tomesphere.com/paper/1812.07285/full.md

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Source: https://tomesphere.com/paper/1812.07285