G. Share

collaborators

3 papers

astro-ph.SR2026

Evidence that SOL2012-06-03 Late Phase $I^^{3}$ Rays are Produced by $>$ 300 MeV Protons from CME-Shock Acceleration of Suprathermals from the Flare

Gerald H. Share, Ronald J. Murphy

A recent paper on SOL2012-06-03 reported the detection for the first time of two distinct phases of $>$ 100 MeV $I^^{3}$ -radiation indicating separate acceleration processes. But such t…

astro-ph.HE2026

$I^^{3}$ -Ray Lines -- Signatures of Nucleosynthesis, Cosmic Rays, Positron Annihilation, and Fundamental Physics

Thomas Siegert, Francesca Calore, Pierre Jean +6

The nuclear $I^^{3}$ -ray lines in the MeV range of the electromagnetic spectrum hold a vast variety of astrophysical, particle-physical, and fundamental physical information that is ot…

astro-ph.SR2025

Solar Gamma-Ray Evidence for a Distinct Population of $>$ 1 MeV Flare-Accelerated Electrons

Gerald H. Share, Ronald J. Murphy, Brian R. Dennis +1

Significant improvements in our understanding of nuclear $I^^{3}$ -ray line production and instrument performance allow us to better characterize the continuum emission from electrons a…

Evidence that SOL2012-06-03 Late Phase I^3 Rays are Produced by >300 MeV Protons from CME-Shock Acceleration of Suprathermals from the Flare

I^3-Ray Lines -- Signatures of Nucleosynthesis, Cosmic Rays, Positron Annihilation, and Fundamental Physics

Solar Gamma-Ray Evidence for a Distinct Population of > 1 MeV Flare-Accelerated Electrons

Evidence that SOL2012-06-03 Late Phase $I^^{3}$ Rays are Produced by $>$ 300 MeV Protons from CME-Shock Acceleration of Suprathermals from the Flare

$I^^{3}$ -Ray Lines -- Signatures of Nucleosynthesis, Cosmic Rays, Positron Annihilation, and Fundamental Physics

Solar Gamma-Ray Evidence for a Distinct Population of $>$ 1 MeV Flare-Accelerated Electrons