PDS4 Certified
















    The Ultraviolet/Visible Spectrometer (UVS) includes the UV-VIS Spectrometer designed for limb observations to achieve limb and occultation measurements and also measure limb dust by measuring backscattered or forward scattered sunlight. In Limb mode measures atmospheric species including: K, Na, Al, Si, Ca, Li, OH, H2O can be detected. UVS Observations are in Limb Mode or Occultation Mode.

    Useful Mission Documents

    Archive Bundle Contents
    Document - Directory containing the document collection, which includes references to refereed journals using this instrument, and information about calibration and explanation of data structures.
    Download Document Collection Zip file (6 MB)

    Raw Data - Directory containing the raw data files.
    Download Raw Collection Zip file (3 GB)

    Calibrated Data - Directory containing the calibrated data files.
    Calibration Document - Description of the calibration methods
    Download Calibrated Collection Zip file (5.2 GB)

    Derived Data – (Certified with liens - final version coming soon).


    Citing Data Sets for Publications

    Colaprete, A. et al., LADEE Ultraviolet-Visible Spectrometer, urn:nasa:pds:ladee_uvs_bundle, (2014).

    Other Useful Products for Interpreting the Data

    Publications - A listing of team members to facilitate literature searches

    Other potentially relevant data
    Acceleration, Reconnection, Turbulence and Electrodynamics of the
          Moon's Interaction with the Sun (ARTEMIS) (available soon from
          PPI Node)
    Lunar Elevation Map
    Solar Activity
    Meteoroid Environment

    SPICE - Archived LADEE SPICE ancillary data providing observation geometry (positions, orientations, instrument pointing, time conversions, etc.) are available from the PDS NAIF Node


    For assistance in understanding PDS4 contact lhuber"at"nmsu"dot"edu at the PDS Atmospheric Discipline Node.




















    Spectrum 554 in activity 1981 (Backward limb). Start of observation = 2014-04-17T07:42:53.324Z. Flux is in watts per nm per m^2 per steradian. Wavelengths corresponding to each pixel are found in the calibration collection.