30 Sep 2026 - 02:08 EDT
30 Sep 2026 - 06:08 UTC
30 Sep 2026 - 06:08 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 - 30 Sep 2026 - 0245 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0247 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0249 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0251 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0253 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0255 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0257 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0301 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0303 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0305 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0307 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0309 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0311 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0313 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0315 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0317 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0319 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0321 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0323 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0325 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0327 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0329 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0331 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0333 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0335 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0337 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0339 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0341 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0343 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0345 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0347 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0349 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0351 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0353 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0355 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0357 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0401 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0403 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0405 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0407 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0409 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0411 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0529 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0531 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0533 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0535 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0537 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0539 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0541 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0543 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0545 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0547 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0549 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0551 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0553 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0555 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0557 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0601 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0603 UTC
Fe094 - Flare Location and Morphology - 30 Sep 2026 - 0605 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