# Double Coronal X-ray and Microwave Sources Associated With A Magnetic Breakout Solar Eruption

## TL;DR

This study reports on double coronal X-ray and microwave sources during a solar eruption, revealing new characteristics and linking the upper source to rapid magnetic arcade motions, advancing understanding of magnetic reconnection in solar flares.

## Contribution

It provides new observational insights into double coronal sources in both X-ray and microwave regimes, highlighting their association with magnetic breakout processes and fast arcade motions.

## Key findings

- Upper source extends up to 70-100 keV energies.
- Microwave spectra support gyro-synchrotron emission from non-thermal electrons.
- Upper source linked to rapid side lobe squeezing-in motion.

## Abstract

Double coronal hard X-ray (HXR) sources are believed to be critical observational evidence of bi-directional energy release through magnetic reconnection in a large-scale current sheet in solar ares. Here we present a study on double coronal sources observed in both HXR and microwave regimes, revealing new characteristics distinct from earlier reports. This event is associated with a footpoint-occulted X1.3-class flare (25 April 2014, starting at 00:17 UT) and a coronal mass ejection that are likely triggered by the magnetic breakout process, with the lower source extending upward from the top of the partially-occulted flare loops and the upper source co-incident with rapidly squeezing-in side lobes (at a speed of ~250 km/s on both sides). The upper source can be identified at energies as high as 70-100 keV. The X-ray upper source is characterized by flux curves different from the lower source, a weak energy dependence of projected centroid altitude above 20 keV, a shorter duration and a HXR photon spectrum slightly-harder than those of the lower source. In addition, the microwave emission at 34 GHz also exhibits a similar double source structure and the microwave spectra at both sources are in line with gyro-synchrotron emission given by non- thermal energetic electrons. These observations, especially the co-incidence of the very-fast squeezing-in motion of side lobes and the upper source, indicate that the upper source is associated with (possibly caused by) this fast motion of arcades. This sheds new lights on the origin of the corona double-source structure observed in both HXRs and microwaves.