31 Oct 2026 - 09:00 EDT
31 Oct 2026 - 13:00 UTC
31 Oct 2026 - 13:00 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 - 31 Oct 2026 - 1055 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1057 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1101 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1103 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1105 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1107 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1109 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1111 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1113 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1115 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1117 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1119 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1121 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1123 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1125 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1127 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1129 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1131 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1133 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1135 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1137 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1139 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1141 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1143 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1145 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1147 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1149 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1151 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1153 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1155 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1157 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1201 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1203 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1205 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1207 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1209 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1211 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1213 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1215 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1217 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1219 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1221 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1223 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1225 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1227 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1229 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1231 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1233 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1235 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1237 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1239 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1241 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1243 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1245 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1247 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1249 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1251 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1253 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1255 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1257 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