Page 4: 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.

Could life at TRAPPIST-1 survive the star's superflares?

The TRAPPIST-1 system is a science-fiction writer's dream. Seven Earth-sized worlds orbit a red dwarf star just 40 light-years away. Three of those worlds are within the habitable zone of the star. The system spans a distance ...

Astronomers observe a strong superflare from giant star

Using the Neutron Star Interior Composition Explorer (NICER) and various ground-based telescopes, an international team of astronomers have performed observations of a strong X-ray superflare which occurred in 2022 on a giant ...

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