30 Jan 2026 - 09:56 EST
30 Jan 2026 - 14:56 UTC
30 Jan 2026 - 14:56 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 Jan 2026 - 1251 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1253 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1255 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1257 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1301 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1303 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1305 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1307 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1309 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1311 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1313 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1315 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1317 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1319 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1321 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1323 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1325 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1327 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1329 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1331 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1333 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1335 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1337 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1339 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1341 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1343 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1345 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1347 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1349 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1351 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1353 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1355 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1357 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1401 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1403 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1405 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1407 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1409 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1411 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1413 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1415 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1417 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1419 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1421 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1423 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1425 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1427 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1429 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1431 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1433 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1435 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1437 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1439 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1441 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1443 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1445 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1447 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1449 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1451 UTC
Fe094 - Flare Location and Morphology - 30 Jan 2026 - 1453 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