Sudden, localised release of 10²²–10²⁵ J of magnetic energy in the solar atmosphere via reconnection, observed as bright multi-wavelength emission (soft X-ray, hard X-ray, EUV) and impulsive particle acceleration.
Sudden, localised release of 10²²–10²⁵ J of magnetic energy in the solar atmosphere via reconnection, observed as bright multi-wavelength emission (soft X-ray, hard X-ray, EUV) and impulsive particle acceleration.