Page 3: Research news on flare

In the context of physical phenomena, a flare is a transient, intense increase in electromagnetic radiation and often particle emission from an astrophysical object, typically associated with rapid energy release in a magnetized plasma. Solar and stellar flares arise from magnetic reconnection in the corona, converting stored magnetic energy into heating, particle acceleration, and broadband radiation from radio to gamma rays on timescales of seconds to hours. Flares are characterized by impulsive and gradual phases, nonthermal electron and ion populations, and can drive associated phenomena such as coronal mass ejections, shock waves, and disturbances in surrounding magnetized environments.

Solar Orbiter traces superfast electrons back to sun

The European Space Agency-led Solar Orbiter mission has split the flood of energetic particles flung out into space from the sun into two groups, tracing each back to a different kind of outburst from our star.

This star survived a black hole—and came back for more

Lightning might not strike twice, but black holes apparently do. An international group of researchers led by Tel Aviv University astronomers observed a flare caused when a star falls onto a black hole and is destroyed.

Flares from magnetized stars can forge planets' worth of gold

Astronomers have discovered a previously unknown birthplace of some of the universe's rarest elements: a giant flare unleashed by a supermagnetized star. The astronomers calculated that such flares could be responsible for ...

page 3 from 5