Archival image depicting a solar flare.
For several days, the background X-ray radiation emanating from the Sun has persistently exceeded the C-level flare threshold, indicating a prolonged and uninterrupted solar flare event. This significant astronomical observation was reported by the Laboratory of Solar Astronomy at the Space Research Institute (IKI) of the Russian Academy of Sciences.
Scientists from the institute elaborate that the Sun is currently exhibiting an exceptionally large number of prominent sunspots. These sunspots are crucial indicators, directly reflecting the presence of substantial reserves of flare energy within our star, which fuel such powerful phenomena.
A statement released via the laboratory`s official Telegram channel further clarified the situation: “Furthermore, the background X-ray radiation from the Sun has been surpassing the C-level flare threshold for several days, meaning, in a certain sense, a single continuous flare has been active on the Sun throughout this entire period.”
The researchers at IKI RAS emphasized that solar X-ray emissions are exclusively generated as a result of dynamic and active processes occurring on the star. Consequently, such a consistently high level of X-ray radiation serves as additional, compelling confirmation that something continues to “burn” intensely and actively on the solar surface.
Rupert Blackwood 
Clement Ashworth