Monte Carlo simulations of nuclear de-excitation gamma-ray line spectra from solar flares

Szpigel, S., Thereza, R. M., Castro, C. G. G. d., MacKinnon, A. L. and Simões, P. J. d. A. (2022) Monte Carlo simulations of nuclear de-excitation gamma-ray line spectra from solar flares. Journal of Physics: Conference Series, 2340, 012031. (doi: 10.1088/1742-6596/2340/1/012031)

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Abstract

Recently, we have demonstrated that the Monte Carlo package FLUKA can be used as an effective tool for simulating nuclear processes which occur in solar flares and that it is capable to provide a self-consistent treatment of all typical components of the γ-ray spectra observed in those events. In this work, we have employed a new simulation strategy that allows to improve statistics and resolution in energy of the generated γ-ray spectra. Using this new strategy, we have calculated spectra of γ-ray nuclear de-excitation lines produced by solar flare primary accelerated ions with typical power-law energy distributions.

Item Type:Articles
Status:Published
Refereed:Yes
Glasgow Author(s) Enlighten ID:MacKinnon, Dr Alexander
Authors: Szpigel, S., Thereza, R. M., Castro, C. G. G. d., MacKinnon, A. L., and Simões, P. J. d. A.
College/School:College of Science and Engineering > School of Physics and Astronomy
Journal Name:Journal of Physics: Conference Series
Publisher:Institute of Physics Publishing Ltd.
ISSN:1742-6588
ISSN (Online):1742-6596
Published Online:01 September 2022
Published Online:11 November 2022
Copyright Holders:Copyright © The Author(s) 2022
First Published:First published in Journal of Physics: Conference Series 2340: 012031
Publisher Policy:Reproduced under a Creative Commons License

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