<Spase xmlns="http://www.spase-group.org/data/schema">
    <Version>2.2.2</Version>
    <NumericalData>
        <ResourceID>spase://NASA/NumericalData/Skylab/Spectroheliometer/RasterFITS/PT330S</ResourceID>
        <ResourceHeader>
            <ResourceName>Skylab UV Solar EUV Data in Original and FITS Format</ResourceName>
            <ReleaseDate>2020-07-07T21:15:23Z</ReleaseDate>
            <Description>This data set contains Skylab UV solar EUV data provided by the Principal Investigator. The data consist of both FITS data files and raw data files, contained in two subdirectories: /fits_data and /raw_data. The subdirectory /fits_data contains fits data files created in 2012 by copying from CDs (Compact Disks) which were in turn written by Mathieu Hirtzig at CfA in 2001 from SKYLAB-S055 data stored at the time on tape at CfA.  These data are stored in 22 subdirectories (/fits_data/CD01 through /fits_data/CD22), each of which is a copy of one of the 22 CD's. Each of the subdirectories contains an identical
sub-subdirectory named /README_S055, which contains a number of files some of which may be helpful in examining the data. It is recommended that those unfamiliar with the S055 experiment look at the file README_S055.txt for background, as well as other files in the README_S055 sub-subdirectory, some of which provide useful auxilliary information.  The subdirectory /raw_data contains the raw data from which the fits data files were created.  This is probably of limited use, but is included for archival purposes.</Description>
            <Contact>
                <PersonID>spase://SMWG/Person/Robert.W.Noyes</PersonID>
                <Role>PrincipalInvestigator</Role>
            </Contact>
            <PriorID>spase://VSPO/NumericalData/Skylab/Spectroheliometer/RasterFITS/PT330S</PriorID>
        </ResourceHeader>
        <AccessInformation>
            <RepositoryID>spase://SMWG/Repository/NASA/GSFC/SPDF</RepositoryID>
            <Availability>Online</Availability>
            <AccessRights>Open</AccessRights> 
            <AccessURL>
                <Name>FTP access to FITS data files at SPDF</Name>
                <URL>ftps://spdf.gsfc.nasa.gov/pub/data/skylab/uv_scanning_polychromator_spectroheliometer/fits_data/</URL>
                <Description>In FITS via FTP from SPDF</Description>
            </AccessURL>
            <AccessURL>
                <Name>HTTP access to FITS data files at SPDF</Name>
                <URL>https://spdf.gsfc.nasa.gov/pub/data/skylab/uv_scanning_polychromator_spectroheliometer/fits_data/</URL>
                <Description>In FITS via HTTP from SPDF</Description>
            </AccessURL>
            <Format>FITS</Format>
        </AccessInformation>
       <AccessInformation>
            <RepositoryID>spase://SMWG/Repository/NASA/GSFC/SPDF</RepositoryID>
            <Availability>Online</Availability>
            <AccessRights>Open</AccessRights> 
            <AccessURL>
                <Name>FTPS from SPDF (not with most browsers)</Name>
                <URL>ftps://spdf.gsfc.nasa.gov/pub/data/skylab/uv_scanning_polychromator_spectroheliometer/raw_data/</URL>
                <Description>In counts via FTP from SPDF</Description>
            </AccessURL>
            <AccessURL>
                <Name>HTTPS from SPDF</Name>
                <URL>https://spdf.gsfc.nasa.gov/pub/data/skylab/uv_scanning_polychromator_spectroheliometer/raw_data/</URL>
                <Description>In counts via HTTP from SPDF</Description>
            </AccessURL>
            <Format>Binary</Format>
        </AccessInformation>
        <InstrumentID>spase://SMWG/Instrument/Skylab/Spectroheliometer</InstrumentID>
        <MeasurementType>ImageIntensity</MeasurementType>
        <TemporalDescription>
            <TimeSpan>
                <StartDate>1973-05-28T00:00:00Z</StartDate>
                <StopDate>1974-02-08T23:59:59Z</StopDate>
            </TimeSpan>
            <Cadence>PT330S</Cadence>
        </TemporalDescription>
    </NumericalData>
</Spase>
