17 Mar 2026 - 22:41 EDT
18 Mar 2026 - 02:41 UTC
18 Mar 2026 - 02:41 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 - 0042 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0044 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0046 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0048 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0050 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0052 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0054 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0056 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0058 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0100 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0102 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0104 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0106 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0108 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0110 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0112 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0114 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0116 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0118 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0120 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0122 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0124 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0126 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0128 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0130 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0132 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0134 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0136 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0138 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0140 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0142 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0144 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0146 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0148 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0150 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0152 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0154 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0156 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0158 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0200 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0202 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0204 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0206 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0208 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0210 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0212 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0214 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0216 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0218 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0220 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0222 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0224 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0226 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0228 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0230 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0232 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0234 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0236 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0238 UTC
Fe094 - Flare Location and Morphology - 18 Mar 2026 - 0240 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