18 Mar 2026 - 02:25 EDT
18 Mar 2026 - 06:25 UTC
18 Mar 2026 - 06:25 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 - 18 Mar 2026 - 0306 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0308 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0310 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0312 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0314 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0316 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0318 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0320 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0322 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0324 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0326 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0328 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0330 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0332 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0334 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0336 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0338 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0340 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0342 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0344 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0346 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0348 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0350 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0352 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0354 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0356 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0358 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0400 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0402 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0404 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0406 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0408 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0410 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0412 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0414 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0416 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0418 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0420 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0422 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0424 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0426 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0428 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0550 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0552 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0554 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0556 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0558 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0600 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0602 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0604 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0606 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0608 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0610 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0612 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0614 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0616 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0618 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0620 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0622 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0624 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