29 Jan 2026 - 00:00 EST
29 Jan 2026 - 05:00 UTC
29 Jan 2026 - 05:00 UTC
GOES-19 Solar Ultraviolet Imager (SUVI) - Fe094 Å
4 hour loop - 60 images - 4 minute update
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Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0255 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0257 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0301 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0303 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0305 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0307 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0309 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0311 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0313 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0315 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0317 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0319 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0321 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0323 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0325 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0327 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0329 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0331 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0333 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0335 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0337 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0339 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0341 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0343 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0345 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0347 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0349 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0351 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0353 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0355 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0357 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0401 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0403 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0405 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0407 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0409 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0411 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0413 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0415 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0417 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0419 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0421 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0423 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0425 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0427 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0429 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0431 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0433 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0435 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0437 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0439 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0441 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0443 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0445 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0447 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0449 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0451 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0453 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0455 UTC
Fe094 - Flare Location and Morphology - 29 Jan 2026 - 0457 UTC
Wavelength: 094Å - Primarily used to observe the location and morphology of solar flares, particularly those associated with hot, flaring plasma at temperatures around 6.3 megakelvin (MK).
• Learn more about space weather and the SUVI instrument at the NOAA Space Weather Prediction Center, and the GOES Space Weather Fact Sheet.
• For more details, see the SUVI Documentation at NCEI