Open Access
Research Article
Issue
J. Space Weather Space Clim.
Volume 11, 2021
Article Number 59
Number of page(s) 15
DOI https://doi.org/10.1051/swsc/2021043
Published online 24 December 2021

Supplementary materials

Table S1. The 26 parameters derived from the heliolongitude and the SXR time-series of each flare used as input in the neural network model.Figure S1. One of the more typical NP Events with a minor enhancement in lower proton energies and mainly background noise in higher energies.Figure S2. Similarly to S1, another typical NP Event with slightly higher intensities at low energies.Figure S3. A medium intensity NP Event which exhibits enhancement up to the 166 MeV channel.Figure S4. The most intense NP Event with the highest Peak Flux reaching ~300 p/(cm2·s·sr·MeV) for the 6 MeV channel. However, higher energies are again mostly if not entirely background.

(Access here)


© S. Aminalragia-Giamini et al., Published by EDP Sciences 2021

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.