MSU researcher’s breakthrough model sheds light on solar storms and space weather
Peer-Reviewed Publication
Updates every hour. Last Updated: 17-Jun-2025 18:10 ET (17-Jun-2025 22:10 GMT/UTC)
Our sun is essentially a searing hot sphere of gas. Its mix of primarily hydrogen and helium can reach temperatures between 10,000 and 3.6 million degrees Fahrenheit on its surface and its atmosphere’s outermost layer. Because of that heat, the blazing orb constantly oozes a stream of plasma, made up of charged subatomic particles — mainly protons and electrons. The sun’s gravity can’t contain them because they hold so much energy as heat, so they drift away into space as solar wind. Understanding how charged particles as solar wind interact with other transient eruptions of energy from the sun can help scientists study cosmic rays emitted in supernova explosions. Thomas Do, an astronomy graduate student at Michigan State University, published a paper predicting how particles accelerate under a wider net of circumstances than previous models. His model could be applied to solar storms that impact technology in space.
The team proposes a performance optimization framework of GVDS including the multitask-oriented data migration method and the request access-aware IO proxy resource allocation strategy.
A first-of-its-kind study found subtle, but distinct vowel pronunciations in Pacific Islanders attending more diverse schools compared to students in a predominately white high school. The findings support a long-held theory from cultural anthropology—there’s a stronger tendency for groups to differentiate along ethnic lines where more groups share the same social space.
In the years following the launch of NASA's Hubble Space Telescope, astronomers have tallied over 1 trillion galaxies in the universe. But only one galaxy stands out as the most important nearby stellar island to our Milky Way — the magnificent Andromeda galaxy (Messier 31). It can be seen with the naked eye on a very clear autumn night as a faint cigar-shaped object roughly the apparent angular diameter of our Moon.
A century ago, Edwin Hubble first established that this so-called "spiral nebula" was actually very far outside our own Milky Way galaxy — at a distance of approximately 2.5 million light-years or roughly 25 Milky Way diameters. Prior to that, astronomers had long thought that the Milky way encompassed the entire universe. Overnight, Hubble's discovery turned cosmology upside down by unveiling an infinitely grander universe.
Now, a century later, the space telescope named for Hubble has accomplished the most comprehensive survey of this enticing empire of stars. The Hubble telescope is yielding new clues to the evolutionary history of Andromeda, and it looks markedly different from the Milky Way's history.