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Data Content Related Terms Terms related to user choices of the content of…

- - - - RangeInDarkDunes
      - RangeInImpactEjecta
      - RangeInSlopeStreaks
      - RangeInSpiders
      - RangeInSwissCheese
      - RangeInCraters
      - RangeInBrightDunes
    - - Image class
        There are 34 image classes which appear to be a mix of a variety of kinds of targets including:
        
        parts of the rover or instrument
        
        images of objects and geologic features on Mars
        
        images of the Martian landscaoe
        
        images of the night sky
        
        calibration images
        
        images of the sun and eclipses of the sun by a Martian moon
        
        images containing some sort of imaging artifact (e.g., all blue, all green, wierd lines, etc.)
      - ConfidenceLevel
        Pick a range from .9 to 1.0. It should be noted that AI is used to determine the image classes
    - - Mapped Image
        An image that has been geometrically corrected so that it can be used for mapping.
      - Unmapped Image
        An image that has not been geometrically corrected.
  - - - Mosaic Projection
        In the Perseverance Notebook mosaics can be created in several different projections. Options are:
        
        Cylindrical
        
        Cylindrical Perspective
        
        Perspective
        
        Polar
        
        Vertical Perspective
      - Mosaic Source Image Count
        In the Perseverance Notebook this field searches against the number of single frame images that comprise a mosaic. Options are:
        
        2 to 5
        
        6 to 10
        
        11 to 20
        
        21 to 50
        
        51 to 100
        
        101 +
    - - OutPut Options
        Tools here generally have lots of options, including:
        
        Do you want exact counts only?
        
        ASCII vs CSV output
        
        Shapefile output in various ways
        
        Binned image output?
        
        Formats (1 or all of 6 posssible formats)
        
        Zip the results (Y/N)
        
        Should the outputs be tiled and if so what size tiles
        
        Do you want the results emailed to you (as they may take a while to generate)
    - - Keyword
        Free text search against the Specimen name, Product Id, Specimen Classification, and description fields.
      - Specimen Provenance
        Indicates where the specimen came from. Options are:
        
        Earth
        
        Meteorite
        
        Moon
        
        Synthetic
        
        All
      - Textural State
        Options are:
        
        Consolidated
        
        Unconsolidated
        
        All
      - Composition
        Options are:
        
        Mixture
        
        Mineral
        
        Organic
        
        All
      - Mineral Type
        If a composition of mineral is selected then the user may further filter by one or mineral types, the list includes:
        
        carbonate
        
        hydroxide
        
        inosilicate
        
        native element
        
        nesosilicate
        
        nitrate
        
        oxide
        
        phosphate
        
        phyllosilicate
        
        silicate
        
        sorosilicate
        
        sulfate
        
        sulfide
        
        tectosilicate
        
        unclassified
      - Measurement Type
        
        Reflectance
        
        Emission
        
        Raman
        
        X-Ray Flourescence
        
        X-Ray Diffraction
        
        LIBS
        
        Microprobe
      - Data Supplier
        Options are:
        
        JBISHOP, SETI Institute/NASA/AMES Research Center
        
        JMUSTARD, Brown University
        
        RVMORRIS, Johnson Space Center
        
        TLROUSH, NASA/AMES Research Center
    - - Clear Atmosphere
        Indicates whether you only want data from periods/places where the atmosphere was clear (no dust, no clouds, etc.)
      - Time of Day
        Options are:
        
        Day
        
        Night
        
        None
      - Highest Spectral Quality
        Indicates whether only the very highest quality data is returned or not.
      - Highest Bolometric Quality
        Indicates whether only the highest quality bolometric data is returned
      - Field Selection
        Indicates which of the myriad of TES data fields will be returned.
  - - - Spectral Information Flag
        A flag indicating whether an observation contains separable information about multiple wavelengths. Options are Yes or No
      - PolarizationType
        The type of polarization detected by the instrument. Depending on the instrument this may be programmable (i.e., swap a polarization filter in or out). Values are
        
        Linear
        
        None
      - Intensity Levels
        Indicates how many bits are reserved for intensity data (e.g. 4-bit, 8-bit, 12-bit, etc.). Depending on the instrument this may be fixed or programmable.
      - Lesser Size in Pixels
        The length in pixels of the shortest edge of an image. Depending on the instrument this may either be fixed or programmable.
      - Greater Size in Pixels
        The length in pixels of the longest edge of the image. Depending on the instrument this may either be fixed or programmable.
      - Exposure Duration
        The time interval between the opening and closing of an instrument aperture. May be fixed or programmable.
      - Spectrum Size
        Indicates how many distinct wavelength or wavelength bins are in the spectrum. Users may specify a range in sizes.
      - Wavelength Range
        Allows users to restrict their search based on the wavelengths available in the respective instrument, instrument mode, and filter combination. For example, for an imaging instrument the wavelength range is based on the filter bandpass. For a spectroscopic instrument, the wavelength range is based on the limits of the spectrum collected. Wavelength ranges can be entered in microns, angstroms, nm, or cm.
      - Wavelength Resolution
        The range in widths of spectral lines that can be reliably detected in an observation, given in wavelengths. Ranges can be entered in microns, angstroms, nm, or cm.
      - Wavenumber Range
        Allows users to restrict their search based on the wavenumbers available in the respective instrument, instrument mode, and filter combination. Wavenumber ranges can be entered in inverse cm or inverse m.
      - Wavenumber Resolution
        The range in widths of spectral lines that can be reliably detected in an observation, given in wavenumbers. Ranges can be entered in inverse cm/pixel or inverse m/pixel.
- - - - Co-AlignedDataCubes
        These are data products where the data from multiple instruments has been combined into a single product (e.g., IRIS, Hinode and SDO data). Choices are:
        
        AIA
        
        SOT-SP
        
        SOT-FG
        
        Cruiser
- - - - TESS TCE
        A Transiting Exoplanet Survey Satellite (TESS) Threshold Crossing Event TCE) is identified by the processing pipeline. A Threshold Crossing Event (TCE) is a sequence of transit-like features in the flux time series of a given target that resembles the signature of a transiting planet to a sufficient degree that the target is passed on for further analysis.
      - TESS TOI
        TESS Objects Of Interest are TCE's that have been vetted and determined to be sufficiently consistent with a transit or eclipse. The TOI list contains both planet candidates and false positives, but these are the signals that are worthy of follow-up observations.
      - Planet
        By planet they mean the name of an exoplanet - not one in our solar system.
    - - Object
        The name of the object you are searching for information about
  - - - Classified Extragalactic
        Options are:
        
        Galaxy Pairs
        
        Galaxy Triples
        
        Galaxy Groups
        
        Galaxy Clusters
        
        QSOs
        
        QSO Groups
        
        Gravitational Lenses
        
        Absorption Line Systems
        
        Emission Line Systems
      - Components of Galaxies
        Options are:
        
        Supernovae
        
        HII Regions
        
        Planetary Nebulae
        
        Supernova Remnants
        
        Stellar Associations
        
        Star Clusters
        
        Molecular Clouds
        
        Novae
        
        Variable Stars
        
        Wolf-Rayet Stars
        
        Carbon Stars
        
        Parts of Galaxies
        
        Others
      - Source Types
        Options are:
        
        Radio Sources
        
        Submillimeter Sources
        
        Infrared Sources
        
        Visual Sources
        
        UV Sources
        
        UV Excess Sources
        
        X-Ray Sources
        
        Gamma-ray Sources
    - - Hubble Parameter (Ho)
      - Energy Density of Matter (Omega matter)
      - Energy Density of Vacuum (Omega vacuum)
    - - Flux
      - Flux Unit
        Options are:
        
        Jy
        
        mJy
        
        Magnitude
        
        W m^-2 Hz^-1
      - Spectral region
        Options are:
        
        Radio
        
        Millimeter
        
        Submillimeter
        
        Infrared
        
        Optical
        
        Ultrviolet
        
        X-ray
        
        Gamma Ray
      - Spectral Band
        The options vary based on the spectral region selected. Each list is rather long and seems to be instrument configuration specific.
- - - - EPSG:4326
        Lat-lon / Geographic / WGS 84
      - EPSG:3857
        Web Mercator / Spherical Mercator / "Google Projection"
      - EPSG:3413
        NSIDC Sea Ice Polar Stereographic North
      - EPSG:3031
        Antarctic Polar Stereographic / WGS 84