Yet Another Sunshine Mystery: Unexpected Asymmetry in GeV Emission from the Solar Disk

Abstract

The Sun is one of the most luminous $\gamma$-ray sources in the sky and continues to challenge our understanding of its high-energy emission mechanisms. This study provides an in-depth investigation of the solar disk $\gamma$-ray emission, using data from the Fermi Large Area Telescope spanning 2008 August to 2022 January. We focus on $\gamma$-ray events with energies exceeding 5 GeV, originating from 0.5${}^{\circ }$ angular aperture centered on the Sun, and implement stringent time cuts to minimize potential sample contaminants. We use a helioprojection method to resolve the $\gamma$-ray events relative to the solar rotation axes and combine statistical tests to investigate the distribution of events over the solar disk. We found that integrating observations over large time windows may overlook relevant asymmetrical features, which we reveal in this work through a refined time-dependent morphological analysis. We describe significant anisotropic trends and confirm compelling evidence of energy-dependent asymmetry in the solar disk $\gamma$-ray emission. Intriguingly, the asymmetric signature coincides with the Sun's polar field flip during the cycle 24 solar maximum, around 2014 June. Our findings suggest that the Sun's magnetic configuration plays a significant role in shaping the resulting $\gamma$-ray signature, highlighting a potential link between the observed anisotropies, solar cycle, and the solar magnetic fields. These insights pose substantial challenges to established emission models, prompting fresh perspectives on high-energy solar astrophysics.

21 pages, 8 figures, 2 animated data visualizations

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Cited by in corpus (4)

• Role of magnetic arcades in explaining the puzzle of the gamma-ray emission from the solar disk
• Puzzling Variation of Gamma Rays from the Sun over the Solar Cycle Revealed with Fermi-LAT
• First Observations of Solar Halo Gamma Rays Over a Full Solar Cycle
• Angular Distribution of Gamma Rays Produced in Proton-Proton Collisions