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Created 6 GOES-18/SUVI NumericalData Descriptions
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<?xml version="1.0" encoding="UTF-8"?>
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<Spase xmlns="http://www.spase-group.org/data/schema" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.spase-group.org/data/schema http://www.spase-group.org/data/schema/spase-2_7_0.xsd">
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<Version>2.7.0</Version>
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<NumericalData>
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<ResourceID>spase://NOAA/NumericalData/GOES/18/SUVI/FE094/PT120S</ResourceID>
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<NamingAuthority>NOAA</NamingAuthority>
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<ResourceType>NumericalData</ResourceType>
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<ResourceHeader>
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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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<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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<Contact>
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<PersonID>spase://SMWG/Person/Christian.Bethge</PersonID>
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<Role>Scientist</Role>
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</Contact>
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<Contact>
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<PersonID>spase://SMWG/Person/Jonathan.Darnel</PersonID>
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<Role>Scientist</Role>
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</Contact>
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<Contact>
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<PersonID>spase://SMWG/Person/Josh.Riley</PersonID>
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<Role>GeneralContact</Role>
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</Contact>
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<Contact>
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<PersonID>spase://SMWG/Person/Alessandra.Pacini</PersonID>
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<Role>ArchiveSpecialist</Role>
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</Contact>
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<InformationURL>
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<Name>GOES-R Satellite Series SUVI Information</Name>
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<URL>https://www.goes-r.gov/spacesegment/suvi.html</URL>
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</InformationURL>
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</ResourceHeader>
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<AccessInformation>
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<RepositoryID>spase://SMWG/Repository/NOAA/NGDC</RepositoryID>
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<Availability>Online</Availability>
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<AccessRights>Open</AccessRights>
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<AccessURL>
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<URL>https://data.ngdc.noaa.gov/platforms/solar-space-observing-satellites/goes/goes18/l1b/suvi-l1b-fe094/</URL>
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<Style>File</Style>
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</AccessURL>
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<Format>FITS</Format>
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<Encoding>GZIP</Encoding>
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</AccessInformation>
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<InstrumentID>spase://NOAA/Instrument/GOES/18/SUVI</InstrumentID>
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<MeasurementType>ImageIntensity</MeasurementType>
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<TemporalDescription>
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<TimeSpan>
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<StartDate>2022-11-02T00:01:19</StartDate>
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<RelativeStopDate>-PT10M</RelativeStopDate>
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</TimeSpan>
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</TemporalDescription>
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<ObservedRegion>Sun</ObservedRegion>
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<ObservedRegion>Sun.Corona</ObservedRegion>
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<Parameter>
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<Name>FITS Data Array</Name>
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<Description>GOES/SUVI 94 Å Image Intensity Array</Description>
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<Units>W m^-2 sr^-1</Units>
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<Wave>
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<WaveType>Photon</WaveType>
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<WaveQuantity>Intensity</WaveQuantity>
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<WavelengthRange>
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<Low>94</Low>
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<High>94</High>
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<Units>angstrom</Units>
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</WavelengthRange>
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</Wave>
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<SpatialCoverage>
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<CoordinateSystem>
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<CoordinateRepresentation>Cartesian</CoordinateRepresentation>
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<CoordinateSystemName>HPC</CoordinateSystemName>
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</CoordinateSystem>
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<Description>Array size: 1280x1280
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Pixel Resolution: 2.5 arcsec
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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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</NumericalData>
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</Spase>
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<?xml version="1.0" encoding="UTF-8"?>
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<Spase xmlns="http://www.spase-group.org/data/schema" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.spase-group.org/data/schema http://www.spase-group.org/data/schema/spase-2_7_0.xsd">
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<Version>2.7.0</Version>
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<NumericalData>
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<ResourceID>spase://NOAA/NumericalData/GOES/18/SUVI/FE131/PT120S</ResourceID>
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<NamingAuthority>NOAA</NamingAuthority>
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<ResourceType>NumericalData</ResourceType>
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<ResourceHeader>
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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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<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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<Contact>
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<PersonID>spase://SMWG/Person/Christian.Bethge</PersonID>
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<Role>Scientist</Role>
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</Contact>
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<Contact>
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<PersonID>spase://SMWG/Person/Jonathan.Darnel</PersonID>
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<Role>Scientist</Role>
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</Contact>
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<Contact>
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<PersonID>spase://SMWG/Person/Josh.Riley</PersonID>
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<Role>GeneralContact</Role>
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</Contact>
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<Contact>
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<PersonID>spase://SMWG/Person/Alessandra.Pacini</PersonID>
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<Role>ArchiveSpecialist</Role>
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</Contact>
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<InformationURL>
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<Name>GOES-R Satellite Series SUVI Information</Name>
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<URL>https://www.goes-r.gov/spacesegment/suvi.html</URL>
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</InformationURL>
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</ResourceHeader>
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<AccessInformation>
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<RepositoryID>spase://SMWG/Repository/NOAA/NGDC</RepositoryID>
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<Availability>Online</Availability>
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<AccessRights>Open</AccessRights>
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<AccessURL>
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<URL>https://data.ngdc.noaa.gov/platforms/solar-space-observing-satellites/goes/goes18/l1b/suvi-l1b-fe131/</URL>
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<Style>File</Style>
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</AccessURL>
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<Format>FITS</Format>
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<Encoding>GZIP</Encoding>
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</AccessInformation>
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<InstrumentID>spase://NOAA/Instrument/GOES/18/SUVI</InstrumentID>
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<MeasurementType>ImageIntensity</MeasurementType>
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<TemporalDescription>
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<TimeSpan>
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<StartDate>2022-11-02T00:00:29</StartDate>
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<RelativeStopDate>-PT10M</RelativeStopDate>
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</TimeSpan>
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</TemporalDescription>
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<ObservedRegion>Sun</ObservedRegion>
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<ObservedRegion>Sun.Corona</ObservedRegion>
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<Parameter>
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<Name>FITS Data Array</Name>
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<Description>GOES/SUVI 131 Å Image Intensity Array</Description>
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<Units>W m^-2 sr^-1</Units>
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<Wave>
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<WaveType>Photon</WaveType>
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<WaveQuantity>Intensity</WaveQuantity>
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<WavelengthRange>
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<Low>131</Low>
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<High>131</High>
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<Units>angstrom</Units>
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</WavelengthRange>
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</Wave>
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<SpatialCoverage>
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<CoordinateSystem>
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<CoordinateRepresentation>Cartesian</CoordinateRepresentation>
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<CoordinateSystemName>HPC</CoordinateSystemName>
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</CoordinateSystem>
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<Description>Array size: 1280x1280
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Pixel Resolution: 2.5 arcsec
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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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</NumericalData>
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</Spase>
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<?xml version="1.0" encoding="UTF-8"?>
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<Spase xmlns="http://www.spase-group.org/data/schema" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.spase-group.org/data/schema http://www.spase-group.org/data/schema/spase-2_7_0.xsd">
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<Version>2.7.0</Version>
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<NumericalData>
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<ResourceID>spase://NOAA/NumericalData/GOES/18/SUVI/FE171/PT240S</ResourceID>
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<NamingAuthority>NOAA</NamingAuthority>
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<ResourceType>NumericalData</ResourceType>
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<ResourceHeader>
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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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<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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<Contact>
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<PersonID>spase://SMWG/Person/Christian.Bethge</PersonID>
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<Role>Scientist</Role>
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</Contact>
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<Contact>
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<PersonID>spase://SMWG/Person/Jonathan.Darnel</PersonID>
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<Role>Scientist</Role>
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</Contact>
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<Contact>
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<PersonID>spase://SMWG/Person/Josh.Riley</PersonID>
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<Role>GeneralContact</Role>
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</Contact>
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<Contact>
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<PersonID>spase://SMWG/Person/Alessandra.Pacini</PersonID>
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<Role>ArchiveSpecialist</Role>
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</Contact>
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<InformationURL>
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<Name>GOES-R Satellite Series SUVI Information</Name>
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<URL>https://www.goes-r.gov/spacesegment/suvi.html</URL>
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</InformationURL>
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</ResourceHeader>
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<AccessInformation>
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<RepositoryID>spase://SMWG/Repository/NOAA/NGDC</RepositoryID>
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<Availability>Online</Availability>
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<AccessRights>Open</AccessRights>
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<AccessURL>
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<URL>https://data.ngdc.noaa.gov/platforms/solar-space-observing-satellites/goes/goes18/l1b/suvi-l1b-fe171/</URL>
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<Style>File</Style>
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</AccessURL>
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<Format>FITS</Format>
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<Encoding>GZIP</Encoding>
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</AccessInformation>
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<InstrumentID>spase://NOAA/Instrument/GOES/18/SUVI</InstrumentID>
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<MeasurementType>ImageIntensity</MeasurementType>
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<TemporalDescription>
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<TimeSpan>
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<StartDate>2022-11-02T00:01:49</StartDate>
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<RelativeStopDate>-PT10M</RelativeStopDate>
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</TimeSpan>
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</TemporalDescription>
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<ObservedRegion>Sun</ObservedRegion>
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<ObservedRegion>Sun.Corona</ObservedRegion>
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<ObservedRegion>Sun.TransitionRegion</ObservedRegion>
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<Parameter>
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<Name>FITS Data Array</Name>
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<Description>GOES/SUVI 171 Å Image Intensity Array</Description>
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<Units>W m^-2 sr^-1</Units>
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<Wave>
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<WaveType>Photon</WaveType>
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<WaveQuantity>Intensity</WaveQuantity>
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<WavelengthRange>
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<Low>171</Low>
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<High>171</High>
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<Units>angstrom</Units>
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</WavelengthRange>
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</Wave>
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<SpatialCoverage>
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<CoordinateSystem>
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<CoordinateRepresentation>Cartesian</CoordinateRepresentation>
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<CoordinateSystemName>HPC</CoordinateSystemName>
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</CoordinateSystem>
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<Description>Array size: 1280x1280
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Pixel Resolution: 2.5 arcsec
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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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</NumericalData>
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</Spase>
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<?xml version="1.0" encoding="UTF-8"?>
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<Spase xmlns="http://www.spase-group.org/data/schema" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.spase-group.org/data/schema http://www.spase-group.org/data/schema/spase-2_7_0.xsd">
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<Version>2.7.0</Version>
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<NumericalData>
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<ResourceID>spase://NOAA/NumericalData/GOES/18/SUVI/FE195/PT60S</ResourceID>
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<NamingAuthority>NOAA</NamingAuthority>
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<ResourceType>NumericalData</ResourceType>
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<ResourceHeader>
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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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<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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<Contact>
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<PersonID>spase://SMWG/Person/Christian.Bethge</PersonID>
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<Role>Scientist</Role>
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</Contact>
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<Contact>
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<PersonID>spase://SMWG/Person/Jonathan.Darnel</PersonID>
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<Role>Scientist</Role>
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</Contact>
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<Contact>
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<PersonID>spase://SMWG/Person/Josh.Riley</PersonID>
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<Role>GeneralContact</Role>
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</Contact>
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<Contact>
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<PersonID>spase://SMWG/Person/Alessandra.Pacini</PersonID>
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<Role>ArchiveSpecialist</Role>
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</Contact>
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<InformationURL>
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<Name>GOES-R Satellite Series SUVI Information</Name>
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<URL>https://www.goes-r.gov/spacesegment/suvi.html</URL>
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</InformationURL>
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</ResourceHeader>
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<AccessInformation>
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<RepositoryID>spase://SMWG/Repository/NOAA/NGDC</RepositoryID>
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<Availability>Online</Availability>
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<AccessRights>Open</AccessRights>
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<AccessURL>
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<URL>https://data.ngdc.noaa.gov/platforms/solar-space-observing-satellites/goes/goes18/l1b/suvi-l1b-fe195/</URL>
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<Style>File</Style>
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</AccessURL>
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<Format>FITS</Format>
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<Encoding>GZIP</Encoding>
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</AccessInformation>
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<InstrumentID>spase://NOAA/Instrument/GOES/18/SUVI</InstrumentID>
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<MeasurementType>ImageIntensity</MeasurementType>
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<TemporalDescription>
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<TimeSpan>
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<StartDate>2022-11-02T00:00:59</StartDate>
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<RelativeStopDate>-PT10M</RelativeStopDate>
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</TimeSpan>
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</TemporalDescription>
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<ObservedRegion>Sun</ObservedRegion>
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<ObservedRegion>Sun.Corona</ObservedRegion>
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<Parameter>
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<Name>FITS Data Array</Name>
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<Description>GOES/SUVI 195 Å Image Intensity Array</Description>
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<Units>W m^-2 sr^-1</Units>
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<Wave>
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<WaveType>Photon</WaveType>
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<WaveQuantity>Intensity</WaveQuantity>
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<WavelengthRange>
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<Low>195</Low>
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<High>195</High>
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<Units>angstrom</Units>
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</WavelengthRange>
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</Wave>
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<SpatialCoverage>
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<CoordinateSystem>
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<CoordinateRepresentation>Cartesian</CoordinateRepresentation>
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<CoordinateSystemName>HPC</CoordinateSystemName>
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</CoordinateSystem>
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<Description>Array size: 1280x1280
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Pixel Resolution: 2.5 arcsec
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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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</NumericalData>
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</Spase>

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