Fermi-LAT Observation of Impulsive Solar Flares

TL;DR

The Fermi-LAT has observed high-energy gamma-ray emissions from solar flares, including impulsive phases and sustained emissions, providing new insights into solar energetic processes and particle acceleration.

Contribution

This study presents new observations of gamma-ray emissions during solar flares, highlighting the LAT's capability to detect high-energy phenomena during impulsive and extended phases.

Findings

Detection of gamma rays up to GeV energies during impulsive phases.

Observation of sustained gamma-ray emission hours after flare onset.

Correlation of gamma-ray emissions with X-ray flare classes.

Abstract

The Fermi Large Area Telescope (LAT) is the most sensitive instrument ever deployed in space for observing gamma-ray emission >100 MeV. This sensitivity has enabled the LAT to detect gamma-ray emission from the Sun during quiescent periods from pions produced by cosmic-ray protons interacting in the solar atmosphere and from cosmic-ray electrons interacting with solar optical photons. The LAT has detected high-energy gamma-ray emission associated with GOES M-class and X-class X-ray flares accompanied by coronal mass ejections and solar energetic particle events. In a number of cases, LAT has detected gamma rays with energies up to several hundreds of MeV during the impulsive phase and gamma rays up to GeV energies sustained for several hours after the impulsive phase. This presentation focuses on observations in the impulsive emission phase in solar flares, including the modest GOES M2-class flare at SOL2010-06-12T0057 and more recent detections, such as the bright X-class flares of March 2012.