J. Space Weather Space Clim.
Volume 8, 2018
Measurement, Specification and Forecasting of the Solar Energetic Particle Environment and GLEs
|Number of page(s)||10|
|Published online||06 February 2018|
The virtual enhancements − solar proton event radiation (VESPER) model
Institute of Accelerating Systems and Applications,
P.O. Box 17214,
2 Space Applications & Research Consultancy (SPARC), Kleissovis 8, GR-10677 Athens, Greece
3 Department of Physics, National and Kapodistrian University of Athens, Athens, Greece
4 European Research and Technology Centre, European Space Agency, Noordwijk, Netherlands
Accepted: 4 December 2017
A new probabilistic model introducing a novel paradigm for the modelling of the solar proton environment at 1 AU is presented. The virtual enhancements − solar proton event radiation model (VESPER) uses the European space agency's solar energetic particle environment modelling (SEPEM) Reference Dataset and produces virtual time-series of proton differential fluxes. In this regard it fundamentally diverges from the approach of existing SPE models that are based on probabilistic descriptions of SPE macroscopic characteristics such as peak flux and cumulative fluence. It is shown that VESPER reproduces well the dataset characteristics it uses, and further comparisons with existing models are made with respect to their results. The production of time-series as the main output of the model opens a straightforward way for the calculation of solar proton radiation effects in terms of time-series and the pairing with effects caused by trapped radiation and galactic cosmic rays.
Key words: Radiation environment / SEP / modelling / radiation / missions
© S. Aminalragia-Giamini et al., Published by EDP Sciences 2018
This is an Open Access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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