The Extreme UltraViolet Monitor (EUV) uses three stable photometers at key wavelengths (0.1-7, 17-22, and 121.6 nm) representing different temperature solar emissions from different sources: chromospheric, transition region and coronal regions. This data is interpreted to characterize the solar EUV solar radiance.

    Measurement Objectives
    EUV will measure solar EUV irradiance shortward of 122 nm, which can vary from a few percent to more than a thousand times depending on the state of solar flares, etc. EUV measurements will provide solar EUV energy input to understand photoionization, photodissociation, and heating rates due to solar variability.

    Useful Mission Documents
    Mission Description
    Spacecraft Description
    Software Interface Specification (SIS) - Description of the instrument and data structures
    Calibration Document - Description of calibration methods

    Archive Bundle Contents
    Documentation - Directory containing the document collection, which includes references to refereed journals using this instrument, and information about calibration and explanation of data structures.

    Raw Data - Directory containing the raw data files

    Calibrated Data - Directory containing the calibrated data files

    Derived Data - Directory containing advanced products


    Selecting and Requesting Data - The following index can be downloaded and edited to contain data that conform to your needs. This allows you to understand the scope of the data set and to tailor your request for specific products.

    As-flown Index - List of actual observations in order of acquisition

    Requesting Data You will need to upload your edited file


    Citing Data Sets for Publications (to be developed)

    Other Useful Products for Interpreting the Data

    References - Publications by team members

    Other Potential Relevant Data - Data that may be relevant from missions other than MAVEN

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