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The SolarIC project aims to enhance our understanding of cosmic-ray propagation in the solar system by using solar inverse-Compton emission as a remote measurement tool. This innovative approach seeks to provide insights into charged particle behavior in astrophysics.
How well do we understand charged particle propagation in the solar system?
This is an important topic for both astrophysics and space weather.
Unfortunately, we still lack a fully predictive theory to this problem; a major challenge to this is the lack of cosmic-ray (CR) measurement throughout the solar system, as most data are measured locally on Earth. I propose to overcome this hurdle in my SolarIC project by using the solar inverse-Compton (IC) emission—produced by CR electrons scattering w…
UNIVERSITEIT VAN AMSTERDAM
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