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      <DOI>https://doi.org/10.48322/9fer-5m90</DOI>
      <ReleaseDate>2025-12-04T13:31:35Z</ReleaseDate>
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      <Description>The COR1 telescope is the inner coronagraph of the Sun Earth Connection Coronal and Heliospheric Investigation (SECCHI) instrument suite aboard the twin Solar Terrestrial Relations Observatory (STEREO) spacecraft. Like all coronagraphs, COR1 is designed to measure the weak light from the solar corona in the presence of scattered light from the much brighter solar photosphere. It designed to observe the white light corona from 1.4 to 4 solar radii.</Description>
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        <Authors>The SECCHI Consortium: Naval Research Laboratory (USA); Lockheed Martin Solar and Astrophysics Laboratory (USA); NASA Goddard Space Flight Center (USA); Johns Hopkins University Applied Physics Laboratory (USA); Rutherford Appleton Laboratory (UK); University of Birmingham (UK); Max-Planck-Institut für Sonnensystemforschung (Germany); Centre Spatiale de Liege (Belgium); Institut d'Optique Théorique et Appliqueé (France); Institut d'Astrophysique Spatiale (France)</Authors>
        <PublicationDate>2006-12-06T00:00:00</PublicationDate>
        <PublishedBy>Goddard Space Flight Center</PublishedBy>
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      <PriorID>spase://VSPO/NumericalData/P_STEREO_HDR_SECCHI</PriorID>
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    <InstrumentID>spase://NASA/Instrument/STEREO-A/SECCHI/Cor1</InstrumentID>
    <MeasurementType>ImageIntensity</MeasurementType>
    <TemporalDescription>
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    <SpectralRange>WhiteLight</SpectralRange>
    <ObservedRegion>Sun.Corona</ObservedRegion>
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