Combining observations to better visualize a superflare

A team of Japanese astronomers used simultaneous ground-based and space-based observations to capture a more complete picture of a superflare on a star. The observed flare started with a very massive, high-velocity prominence ...

How the Sun's magnetic forces arrange gas particles

Solar prominences hover above the visible solar disk like giant clouds, held there by a supporting framework of magnetic forces, originating from layers deep within the Sun. The magnetic lines of force are moved by ever-present ...

Researchers provide new clue to solar coronal heating problem

Coronal heating is a topic dedicated to explaining how the corona may be heated up to a temperature of millions of degrees, far above that of the photosphere. To transport magnetic energy into the corona, Alfvén-wave turbulence ...

Race at the edge of the sun: Ions are faster than atoms

Scientists at the University of Göttingen, the Institut d'Astrophysique in Paris and the Istituto Ricerche Solari Locarno have observed that ions move faster than atoms in the gas streams of a solar prominence. The results ...

Bringing medieval literature into the digital age

William Langland likely wouldn't know what to make of the latest way people are reading his poetry. In part, that's because Langland died in 1386. But it's also because his most famous work, Piers Plowman, is the subject ...

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