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It took some time to go from "in press" to "published", but the mega-review of solar energetic particle (SEP) models by Whitman et al. is out at last! 🎉 Lots of authors contributed by providing info on their prediction codes & validation efforts ✨ Link: sciencedirect.com/science/articl…

Love the how it started vs how it’s going comparison! ☀️ We have definitely come a long way since then studying our star (but there’s still so much to learn) ☺️

Yo the next total solar eclipse over Los Angeles is in 2472, party at my house afterwards 💃🏻

Final round of the #NAstroCoverComp! Give the Sun some love and vote for the February issue, featuring our MHD modeling of the elusive solar corona. From Chitta et al. (2023): nature.com/articles/s4155…

Check out this International Space Science Institute (ISSI) Science Highlight on our project "Tomographic inversion of synthetic white-light images: Advancing our understanding of CMEs in 3D", containing a brief update on our work in progress to unveil the structure of solar eruptions! ☀️

Our live prediction of the #TotalSolarEclipse of April 8, 2024 is out! Wanna see what the majestic solar corona will look like according to our time-dependent model? ☀️ Check out how our expectations evolve with time as we assimilate real-time data at predsci.com/eclipse2024

Some updates on our near-real-time prediction of the #TotalSolarEclipse of April 8, with new data products and data download—and even simulated views from existing coronagraphs in space 😉 Details in the quoted thread and at predsci.com/eclipse2024

Saw the Sun behind the Moon behind a cloud 🌞🌚☁️👀 #TotalEclipse2024

Still craving some Sun science after the magical #SolarEclipse2024? Worry not because AAS Nova has put together very nice write-ups of 3 recent solar physics research articles, including our work on exceptional observations of a CME at Mercury's orbit: aasnova.org/2024/04/08/mon… ☀️

Woah, G5 (extreme) geomagnetic storm conditions have been attained due to the recent CME(s) from AR 13664, with solar wind speeds at ~750 km/s and the north–south (Bz) magnetic field component almost reaching –50 nT. Enjoy the aurora show out there! 💫

What's brewin' in the solar wind—an update: Current storm conditions are: Radio R1, Radiation S1, Geomagnetic G4. Solar wind speeds are still high (~800 km/s), but the Bz field is close to zero, so G4 conditions are unlikely to hold. Will a following CME turn the lights back up?

We are nominated for "Best Use of HPC in Physical Sciences" re: our total solar eclipse 2024 continuously running prediction—Vote at this link by Friday, October 4! hpcwire.com/2024-hpcwire-r…