20 Mar 2026 - 16:47 EDT
20 Mar 2026 - 20:47 UTC
20 Mar 2026 - 20:47 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 - 20 Mar 2026 - 1848 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 1850 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 1852 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 1854 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 1856 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 1858 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 1900 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 1902 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 1904 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 1906 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 1908 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 1910 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 1912 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 1914 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 1916 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 1918 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 1920 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 1922 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 1924 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 1926 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 1928 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 1930 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 1932 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 1934 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 1936 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 1938 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 1940 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 1942 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 1944 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 1946 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 1948 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 1950 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 1952 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 1954 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 1956 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 1958 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 2000 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 2002 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 2004 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 2006 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 2008 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 2010 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 2012 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 2014 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 2016 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 2018 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 2020 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 2022 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 2024 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 2026 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 2028 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 2030 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 2032 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 2034 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 2036 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 2038 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 2040 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 2042 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 2044 UTC
Fe094 - Flare Location and Morphology - 20 Mar 2026 - 2046 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