29–31 May 2019
Sykia, Peloponnese, Greece
Europe/Athens timezone

The VESPER model, a presentation, updates, and future work

30 May 2019, 09:40
15m
Sykia, Peloponnese, Greece

Sykia, Peloponnese, Greece

Χylokastro, Corinthia, Greece 20400

Speaker

Dr Sigiava Aminalragia-Giamini (SPARC)

Description

The Virtual Enhancements – Solar Proton Event Radiation (VESPER) model is one of the latest efforts in the probabilistic modelling of solar particle radiation. VESPER produces differential proton flux time-series of virtual Solar Proton Events (SPEs) for arbitrary mission durations. These virtual SPEs are constructed by rescaling historical SPEs in a spectrally coherent way. A presentation on the VESPER methodology is made and the approach on current and future improvements and updates is shown and discussed.

Primary authors

Dr Sigiava Aminalragia-Giamini (SPARC) Dr Piers Jiggens Dr Ingmar Sandberg (SPARC) Mr Constantinos Papadimitriou (SPARC) Prof. Ioannis Daglis

Presentation materials

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