31 Oct 2026 - 14:26 EDT
31 Oct 2026 - 18:26 UTC
31 Oct 2026 - 18:26 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 - 1621 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1623 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1625 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1627 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1629 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1631 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1633 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1635 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1637 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1639 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1641 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1643 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1645 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1647 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1649 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1651 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1653 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1655 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1657 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1701 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1703 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1705 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1707 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1709 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1711 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1713 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1715 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1717 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1719 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1721 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1723 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1725 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1727 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1729 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1731 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1733 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1735 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1737 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1739 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1741 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1743 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1745 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1747 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1749 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1751 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1753 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1755 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1757 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1801 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1803 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1805 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1807 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1809 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1811 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1813 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1815 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1817 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1819 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1821 UTC
Fe094 - Flare Location and Morphology - 31 Oct 2026 - 1823 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