Savvas Raptis

@savvasraptis.bsky.social

Researcher at Johns Hopkins University Applied Physics Laboratory (JHUAPL): https://savvasraptis.github.io

🙋‍If you are an AGU member who has attended an Annual Meeting in the last five years, you are eligible to volunteer for the OEP Program. Volunteers will give feedback on presenters’ draft presentations in November. You do not need to attend AGU26 yourself to volunteer. ️spklr.io/63328ET3hy

🌉 If you are an AGU member who has attended an Annual Meeting in the last five years, you are eligible to volunteer for the OEP Program. Volunteers will give feedback on presenters’ draft presentations in November. You do not need to attend AGU26 yourself to volunteer.

Great GEM workshop last week in Portland, Maine. Our focus group on Multiscale Dayside Transients (MDT) ran strong sessions on how transients interact with the bow shock and magnetosphere. Thanks to all who presented, and stay tuned for our GEM challenge. gemworkshop.org

BildBild

What is Smile set out to discover? This groundbreaking mission will observe Earth’s magnetosphere in X-rays while capturing the northern lights in ultraviolet, offering an entirely new way to see how our planet defends itself from solar storms. 🔭 🧪 ☀️

In the background of this infographic is an artist impression of the interaction between the Sun and Earth, in the sense that the Sun is sending out particles and the Earth is holding up a shield against them. Three pop-out boxes indicate the top three questions that Smile seeks to solve, with close-up images of the relevant part of the Sun-Earth connection.

New paper out in Science Advances addressing a long-standing open question: what is maximum energy of particles in radiation belts? A simple model shows a universal energy limit of 7 ± 2 TeV, with implications for cosmic rays. doi.org/10.1126/scia... #Heliophysics #Astrophysics #SpaceScience

Universal energy limits of radiation belts in planetary and brown dwarf magnetospheric systems

Exoplanetary and brown dwarf radiation belt systems may contribute significantly to observed cosmic ray spectra up to several TeV.

doi.org

Yesterday I joined remotely a space weather AI/ML panel at #ESWW2025 in Umeå as a giant face on a screen. Key takeaways: We need less hype, more rigor. Better validation, standardized benchmarks, and open access to models/data. Hope to join in-person next year😀!

BildBild