Extended solar emission - an analysis of the EGRET data

TL;DR

This paper analyzes EGRET gamma-ray data to detect and characterize extended solar emission caused by inverse-Compton scattering, accounting for interfering sources, and compares observations with theoretical models.

Contribution

It provides the first detailed analysis of EGRET data for extended solar gamma-ray emission, incorporating time-dependent methods and source interference corrections.

Findings

Detected clear solar gamma-ray emission in EGRET data

Validated analysis technique with moon signal

Results consistent with inverse-Compton emission models

Abstract

The Sun was recently predicted to be an extended source of gamma-ray emission, produced by inverse-Compton scattering of cosmic-ray electrons with the solar radiation. The emission was predicted to contribute to the diffuse extragalactic background even at large angular distances from the Sun. While this emission is expected to be readily detectable in future by GLAST, the situation for available EGRET data is more challenging. We present a detailed study of the EGRET database, using a time dependent analysis, accounting for the effect of the emission from 3C 279, the moon, and other sources, which interfere with the solar signal. The technique has been tested on the moon signal, with results consistent with previous work. We find clear evidence for emission from the Sun and its vicinity. The observations are compared with our model for the extended emission.