Fermi-LAT Observation of Quiescent Solar Emission
Abstract
The Large Area Telescope (LAT), one of two instruments on the Fermi Gamma-ray Space Telescope is a pair-conversion detector designed to study the gamma-ray sky in the energy range 30 MeV to 300 GeV. Fermi has detected high-energy gamma rays from the quiet Sun produced by interactions of cosmic-ray nucleons with the solar surface, and cosmic-ray electrons with solar photons in the heliosphere. While the Sun was detected by EGRET on CGRO with low statistics, Fermi provides high-quality detections on a daily basis allowing variability to be addressed. Such observations will provide a probe of the extreme conditions near the solar surface and a monitor the modulation of cosmic rays over the inner heliosphere. We discuss the study of the quiescent solar emission including spectral analysis of its two components, disk and inverse Compton.
Keywords
Cite
@article{arxiv.0907.0557,
title = {Fermi-LAT Observation of Quiescent Solar Emission},
author = {Elena Orlando},
journal= {arXiv preprint arXiv:0907.0557},
year = {2019}
}
Comments
Contribution to the 31st ICRC, Lodz, Poland, July 2009; 3 pages, 1 figure