2.7.0 spase://NOAA/NumericalData/GOES/18/SUVI/FE195/PT60S NOAA NumericalData GOES-R Series Level 1b SUVI 195 Angstrom FITS Data https://doi.org/10.7289/V5FT8J93 2025-05-07T00:08:46 2025-08-04T00:08:46 Added HelioViewerID to Extension The GOES-R/SUVI 195 Å Level 1b FITS Data. The 195 Å channel observes the Fe XII line from 1.5 MK plasma. The GOES-R Solar Ultraviolet Imagers (SUVI) data consist of solar images in six extreme-ultraviolet passbands — 94 Å, 131 Å, 171 Å, 195 Å, 284 Å, and 304 Å — with a variety of exposure times and filters in place to ensure each image set captures the full dynamic range of solar phenomena. SUVI images have a pixel resolution of 1280×1280 pixels, each with an angular resolution of 2.5 arcsec per pixel, for a total field of view of 53.3 arcmin square. Some corners of the CCD are obscured by instrumental vignetting. spase://SMWG/Person/Christian.Bethge Scientist spase://SMWG/Person/Jonathan.Darnel Scientist spase://SMWG/Person/Josh.Riley GeneralContact spase://SMWG/Person/Alessandra.Pacini ArchiveSpecialist GOES-R Satellite Series SUVI Information https://www.goes-r.gov/spacesegment/suvi.html spase://SMWG/Repository/NOAA/NGDC Online Open https://data.ngdc.noaa.gov/platforms/solar-space-observing-satellites/goes/goes18/l1b/suvi-l1b-fe195/ FITS GZIP spase://NOAA/Instrument/GOES/18/SUVI ImageIntensity 2022-11-02T00:00:59 -PT10M Sun Sun.Corona FITS Data Array GOES/SUVI 195 Å Image Intensity Array W m^-2 sr^-1 Photon Intensity 195 195 angstrom Cartesian HPC Array size: 1280x1280 Pixel Resolution: 2.5 arcsec Field of view: ~1.6 solar radii 2003