17 Oct 2026 - 23:22 EDT
18 Oct 2026 - 03:22 UTC
18 Oct 2026 - 03:22 UTC
GOES-19 Solar Ultraviolet Imager (SUVI) - Fe094 Å
GOES-East - Full Disk - Fe094 - We are working to restore image production as quickly as possible. Please refer to the other GOES imagery sites listed on our resources page. Thank you for your patience.
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Fe094 - Flare Location and Morphology - 18 Oct 2026 - 0002 UTC
Fe094 - Flare Location and Morphology - 18 Oct 2026 - 0004 UTC
Fe094 - Flare Location and Morphology - 18 Oct 2026 - 0006 UTC
Fe094 - Flare Location and Morphology - 18 Oct 2026 - 0008 UTC
Fe094 - Flare Location and Morphology - 18 Oct 2026 - 0010 UTC
Fe094 - Flare Location and Morphology - 18 Oct 2026 - 0012 UTC
Fe094 - Flare Location and Morphology - 18 Oct 2026 - 0014 UTC
Fe094 - Flare Location and Morphology - 18 Oct 2026 - 0016 UTC
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Fe094 - Flare Location and Morphology - 18 Oct 2026 - 0020 UTC
Fe094 - Flare Location and Morphology - 18 Oct 2026 - 0022 UTC
Fe094 - Flare Location and Morphology - 18 Oct 2026 - 0024 UTC
Fe094 - Flare Location and Morphology - 18 Oct 2026 - 0026 UTC
Fe094 - Flare Location and Morphology - 18 Oct 2026 - 0028 UTC
Fe094 - Flare Location and Morphology - 18 Oct 2026 - 0030 UTC
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Fe094 - Flare Location and Morphology - 18 Oct 2026 - 0100 UTC
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Fe094 - Flare Location and Morphology - 18 Oct 2026 - 0114 UTC
Fe094 - Flare Location and Morphology - 18 Oct 2026 - 0116 UTC
Fe094 - Flare Location and Morphology - 18 Oct 2026 - 0118 UTC
Fe094 - Flare Location and Morphology - 18 Oct 2026 - 0120 UTC
Fe094 - Flare Location and Morphology - 18 Oct 2026 - 0122 UTC
Fe094 - Flare Location and Morphology - 18 Oct 2026 - 0124 UTC
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Fe094 - Flare Location and Morphology - 18 Oct 2026 - 0148 UTC
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Fe094 - Flare Location and Morphology - 18 Oct 2026 - 0152 UTC
Fe094 - Flare Location and Morphology - 18 Oct 2026 - 0154 UTC
Fe094 - Flare Location and Morphology - 18 Oct 2026 - 0156 UTC
Fe094 - Flare Location and Morphology - 18 Oct 2026 - 0158 UTC
Fe094 - Flare Location and Morphology - 18 Oct 2026 - 0200 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