The Solar Ultraviolet Imager (SUVI) aboard NOAA's GOES-19 geostationary satellite captures 24-hour timelapses of the Sun in extreme ultraviolet wavelengths, revealing different temperature layers of the solar atmosphere including the corona and chromosphere, with each wavelength channel (such as 284 Å for Fe XV at 2.0 MK) highlighting specific solar features like coronal loops, active regions, and coronal holes.
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Sun 24 Hour Timelapse | Iron XV / 284 Å | Extreme UV (May 06, 2026) #shortsAñadido:
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