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Wednesday, June 18, 2025

The Flare-ometer is at X-level again

Solar flares are classified using the X-ray brightness (see an explanation here), and "X class" flares are the strongest.  The sunspot and magnetic active region complex that produced many M-class and X-class flares last month is back, and the EVE "flare-ometer" is hitting the red zone again.  

EVE measures irradiance in the extreme ultraviolet (EUV), which are wavelengths slightly less energetic than X-rays. EUV variations in flux have a direct impact on the Earth's atmosphere and ionosphere, so EVE's measurements are essential for space weather forecasts.  

An image of a plot of the EVE EUV irradiance during an X-flare, along with GOES X-ray flux.

EVE has a special flare observation mode that is triggered autonomously onboard SDO.  EVE had 7 flare campaigns triggered in April, 8 in May, and so far there have been 8 in June. When combined with HMI and AIA, SDO is able to capture the magnetic structure and dynamics of space weather processes. 


HMI (magnetic field) and AIA (EUV brightness) images from 18 June 2025 showing the sunspot regions responsible for the flares.