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Added HelioViewerID to 18 NOAA/GOES/16-19/SUVI descriptions
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‎NumericalData/GOES/16/SUVI/FE094/PT120S.xml‎

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<ResourceName>GOES-R Series Level 1b SUVI 94 Angstrom FITS Data</ResourceName>
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<DOI>https://doi.org/10.7289/V5FT8J93</DOI>
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<ReleaseDate>2025-04-29T00:08:46</ReleaseDate>
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<RevisionHistory>
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<RevisionEvent>
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<ReleaseDate>2025-08-04T00:08:46</ReleaseDate>
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<Note>Added HelioViewerID to Extension</Note>
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</RevisionEvent>
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</RevisionHistory>
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<Description>The GOES-R/SUVI 94 Å Level 1b FITS Data. The 94 Å channel observes the Fe XVIII line from 6.3 MK flaring plasma.
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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.</Description>
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Field of view: ~1.6 solar radii</Description>
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</SpatialCoverage>
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</Parameter>
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<Extension><HelioViewerID>2000</HelioViewerID></Extension>
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</NumericalData>
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</Spase>

‎NumericalData/GOES/16/SUVI/FE131/PT240S.xml‎

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<ResourceName>GOES-R Series Level 1b SUVI 131 Angstrom FITS Data</ResourceName>
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<DOI>https://doi.org/10.7289/V5FT8J93</DOI>
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<ReleaseDate>2025-04-29T00:08:46</ReleaseDate>
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<RevisionHistory>
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<RevisionEvent>
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<ReleaseDate>2025-08-04T00:08:46</ReleaseDate>
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<Note>Added HelioViewerID to Extension</Note>
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</RevisionEvent>
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</RevisionHistory>
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<Description>The GOES-R/SUVI 131 Å Level 1b FITS Data. The 131 Å channel observes the Fe xx and Fe xxiii lines from 10 MK and 16 MK flaring plasma, respectively.
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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.</Description>
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Field of view: ~1.6 solar radii</Description>
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</SpatialCoverage>
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</Parameter>
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<Extension><HelioViewerID>2001</HelioViewerID></Extension>
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</NumericalData>
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</Spase>

‎NumericalData/GOES/16/SUVI/FE171/PT240S.xml‎

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<ResourceName>GOES-R Series Level 1b SUVI 171 Angstrom FITS Data</ResourceName>
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<DOI>https://doi.org/10.7289/V5FT8J93</DOI>
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<ReleaseDate>2025-04-29T00:08:46</ReleaseDate>
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<RevisionHistory>
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<RevisionEvent>
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<ReleaseDate>2025-08-04T00:08:46</ReleaseDate>
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<Note>Added HelioViewerID to Extension</Note>
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</RevisionEvent>
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</RevisionHistory>
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<Description>The GOES-R/SUVI 171 Å Level 1b FITS Data. The 171 Å channel observes the Fe ix line from quiet corona and upper transition region (0.63 MK).
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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.</Description>
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Field of view: ~1.6 solar radii</Description>
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</SpatialCoverage>
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</Parameter>
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<Extension><HelioViewerID>2002</HelioViewerID></Extension>
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</NumericalData>
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</Spase>

‎NumericalData/GOES/16/SUVI/FE195/PT60S.xml‎

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<ResourceName>GOES-R Series Level 1b SUVI 195 Angstrom FITS Data</ResourceName>
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<DOI>https://doi.org/10.7289/V5FT8J93</DOI>
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<ReleaseDate>2025-04-29T00:08:46</ReleaseDate>
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<RevisionHistory>
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<RevisionEvent>
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<ReleaseDate>2025-08-04T00:08:46</ReleaseDate>
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<Note>Added HelioViewerID to Extension</Note>
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</RevisionEvent>
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</RevisionHistory>
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<Description>The GOES-R/SUVI 195 Å Level 1b FITS Data. The 195 Å channel observes the Fe XII line from 1.5 MK plasma.
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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.</Description>
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Field of view: ~1.6 solar radii</Description>
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</SpatialCoverage>
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</Parameter>
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<Extension><HelioViewerID>2003</HelioViewerID></Extension>
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</NumericalData>
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</Spase>

‎NumericalData/GOES/16/SUVI/FE284/PT240S.xml‎

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<ResourceName>GOES-R Series Level 1b SUVI 284 Angstrom FITS Data</ResourceName>
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<DOI>https://doi.org/10.7289/V5FT8J93</DOI>
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<ReleaseDate>2025-04-29T00:08:46</ReleaseDate>
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<RevisionHistory>
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<RevisionEvent>
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<ReleaseDate>2025-08-04T00:08:46</ReleaseDate>
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<Note>Added HelioViewerID to Extension</Note>
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</RevisionEvent>
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</RevisionHistory>
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<Description>The GOES-R/SUVI 284 Å Level 1b FITS Data. The 284 Å channel observes the Fe XV line from 2 MK plasma.
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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.</Description>
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Field of view: ~1.6 solar radii</Description>
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</SpatialCoverage>
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</Parameter>
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<Extension><HelioViewerID>2004</HelioViewerID></Extension>
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</NumericalData>
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</Spase>

‎NumericalData/GOES/16/SUVI/HE304/PT120S.xml‎

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<ResourceName>GOES-R Series Level 1b SUVI 304 Angstrom FITS Data</ResourceName>
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<DOI>https://doi.org/10.7289/V5FT8J93</DOI>
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<ReleaseDate>2025-04-29T00:08:46</ReleaseDate>
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<RevisionHistory>
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<RevisionEvent>
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<ReleaseDate>2025-08-04T00:08:46</ReleaseDate>
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<Note>Added HelioViewerID to Extension</Note>
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</RevisionEvent>
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</RevisionHistory>
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<Description>The GOES-R/SUVI 304 Å Level 1b FITS Data. The 304 Å channel observes the He ii line from chromosphere and transition region (0.50 MK).
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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.</Description>
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Field of view: ~1.6 solar radii</Description>
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</SpatialCoverage>
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</Parameter>
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<Extension><HelioViewerID>2005</HelioViewerID></Extension>
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</NumericalData>
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</Spase>

‎NumericalData/GOES/17/SUVI/FE094/PT120S.xml‎

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<ResourceName>GOES-R Series Level 1b SUVI 94 Angstrom FITS Data</ResourceName>
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<DOI>https://doi.org/10.7289/V5FT8J93</DOI>
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<ReleaseDate>2025-05-07T00:08:46</ReleaseDate>
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<RevisionHistory>
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<RevisionEvent>
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<ReleaseDate>2025-08-04T00:08:46</ReleaseDate>
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<Note>Added HelioViewerID to Extension</Note>
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</RevisionEvent>
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</RevisionHistory>
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<Description>The GOES-R/SUVI 94 Å Level 1b FITS Data. The 94 Å channel observes the Fe XVIII line from 6.3 MK flaring plasma.
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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.</Description>
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Field of view: ~1.6 solar radii</Description>
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</SpatialCoverage>
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</Parameter>
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<Extension><HelioViewerID>2000</HelioViewerID></Extension>
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</NumericalData>
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</Spase>

‎NumericalData/GOES/17/SUVI/FE131/PT240S.xml‎

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<ResourceName>GOES-R Series Level 1b SUVI 131 Angstrom FITS Data</ResourceName>
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<DOI>https://doi.org/10.7289/V5FT8J93</DOI>
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<ReleaseDate>2025-05-07T00:08:46</ReleaseDate>
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<RevisionHistory>
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<RevisionEvent>
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<ReleaseDate>2025-08-04T00:08:46</ReleaseDate>
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<Note>Added HelioViewerID to Extension</Note>
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</RevisionEvent>
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</RevisionHistory>
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<Description>The GOES-R/SUVI 131 Å Level 1b FITS Data. The 131 Å channel observes the Fe xx and Fe xxiii lines from 10 MK and 16 MK flaring plasma, respectively.
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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.</Description>
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Field of view: ~1.6 solar radii</Description>
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</SpatialCoverage>
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</Parameter>
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<Extension><HelioViewerID>2001</HelioViewerID></Extension>
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</NumericalData>
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</Spase>

‎NumericalData/GOES/17/SUVI/FE171/PT240S.xml‎

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<ResourceName>GOES-R Series Level 1b SUVI 171 Angstrom FITS Data</ResourceName>
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<DOI>https://doi.org/10.7289/V5FT8J93</DOI>
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<ReleaseDate>2025-05-07T00:08:46</ReleaseDate>
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<RevisionHistory>
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<RevisionEvent>
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<ReleaseDate>2025-08-04T00:08:46</ReleaseDate>
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<Note>Added HelioViewerID to Extension</Note>
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</RevisionEvent>
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</RevisionHistory>
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<Description>The GOES-R/SUVI 171 Å Level 1b FITS Data. The 171 Å channel observes the Fe IX line from quiet corona and upper transition region (0.63 MK).
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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.</Description>
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Field of view: ~1.6 solar radii</Description>
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</SpatialCoverage>
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</Parameter>
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<Extension><HelioViewerID>2002</HelioViewerID></Extension>
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</NumericalData>
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</Spase>

‎NumericalData/GOES/17/SUVI/FE195/PT60S.xml‎

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<ResourceName>GOES-R Series Level 1b SUVI 195 Angstrom FITS Data</ResourceName>
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<DOI>https://doi.org/10.7289/V5FT8J93</DOI>
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<ReleaseDate>2025-05-07T00:08:46</ReleaseDate>
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<RevisionHistory>
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<RevisionEvent>
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<ReleaseDate>2025-08-04T00:08:46</ReleaseDate>
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<Note>Added HelioViewerID to Extension</Note>
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</RevisionEvent>
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</RevisionHistory>
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<Description>The GOES-R/SUVI 195 Å Level 1b FITS Data. The 195 Å channel observes the Fe XII line from 1.5 MK plasma.
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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.</Description>
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Field of view: ~1.6 solar radii</Description>
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</SpatialCoverage>
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</Parameter>
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<Extension><HelioViewerID>2003</HelioViewerID></Extension>
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</NumericalData>
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</Spase>

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