The JPL Open Repository (JOR) replaced the JPL Technical Report Server (TRS) in 2023. It is a repository for digital copies of technical publications authored by JPL employees. It includes journal articles (the Final Accepted Version), meeting papers, presentations, and other publications cleared for external distribution from 1992 to the present. It also includes research datasets from 2022 on.

Years covered: 1992 to the present.
  • 1992-2021 records were originally on the JPL Technical Report Server (TRS) on Dspace system; those records were migrated to Dataverse in 2022.
  • Records with publication date 2022 or later are native to the Dataverse.
  • Data sets: 2022 to present
  • There are a few pre-1992 records. Those were added to the system on a case-by-case request basis.

  • Persistent IDs (PIDs):
  • 1992-2021 records have Handles
  • 2022 and later records have Digital Object Identifiers (DOIs).
    • Featured Dataverses

    In order to use this feature you must have at least one published dataverse.

    Publish Dataverse

    Are you sure you want to publish your dataverse? Once you do so it must remain published.

    Publish Dataverse

    This dataverse cannot be published because the dataverse it is in has not been published.

    Delete Dataverse

    Are you sure you want to delete your dataverse? You cannot undelete this dataverse.

    Advanced Search

    1 to 10 of 48,338 Results
    Far horizons, dark backgrounds, adjacent mountains, and other considerations for producing more accurate snow and ice reflectance spectra from imaging spectroscopy measurements
    Nov 2, 2026
    Wilder, Brenton A.; Bohn, Niklas; Carmon, Nimrod; Bair, Edward H.; Griessbaum, Niklas; Et al., 2026, "Far horizons, dark backgrounds, adjacent mountains, and other considerations for producing more accurate snow and ice reflectance spectra from imaging spectroscopy measurements", https://doi.org/10.48577/jpl.EMXJYB, JPL Open Repository
    Far horizons, dark backgrounds, adjacent mountains, and other considerations for producing more accurate snow and ice reflectance spectra from imaging spectroscopy measurements
    Regional Geologic Mapping Surrounding the Marius Hills Pit as the Basis for Potential Future Lunar ExplorationEmbargoed
    Oct 29, 2026
    Jennifer E. C. Scully; Erin J. Leonard; Abigail A. Fraeman; Laura Kerber; Catherine M. Elder, 2026, "Regional Geologic Mapping Surrounding the Marius Hills Pit as the Basis for Potential Future Lunar Exploration", https://doi.org/10.48577/jpl.I4KGY4, The Planetary Science Journal, JPL Open Repository
    The Marius Hills pit (14.1 °N, 303.2 °E) is within the large Marius Hills volcanic plateau on the Moon and is often interpreted as a lava tube skylight, making it a feature of interest for future human exploration. It is a scientifically interesting site because its walls would p...
    The Combined ASTER and MODIS Emissivity over Land (CAMEL) Version 3 Dataset and its ApplicationsEmbargoed
    Oct 29, 2026
    M. L. Loveless; E. E. Borbas; R. O. Knuteson; K. Cawse-Nicholson; G. Hulley; et. al., 2026, "The Combined ASTER and MODIS Emissivity over Land (CAMEL) Version 3 Dataset and its Applications", https://doi.org/10.48577/jpl.OP5O5W, Earth and Space Science, JPL Open Repository
    The recently available Combined ASTER and MODIS Emissivity over Land (CAMEL) Version 3 infrared land surface emissivity dataset is described in this paper. This version uses the updated MODIS Collection 6.1 MxD11 and MxD21 emissivity products as inputs that are less affected by c...
    An intrusive origin for the Nili Fossae regional olivine-bearing unitEmbargoed
    Oct 29, 2026
    Michael S. Bramble; John F. Mustard; Kenneth A. Farley; Kenneth H. Williford; Eleni Ravanis; et. al., 2026, "An intrusive origin for the Nili Fossae regional olivine-bearing unit", https://doi.org/10.48577/jpl.MCDVHW, Nature Communications, JPL Open Repository
    The origin of the olivine-rich unit in Nili Fossae has been debated for over two decades, with leading hypotheses ranging from pyroclastic falls to aeolian deposits. However, recent in situ data from the Perseverance rover favor an igneous cumulate origin, creating a paradox with...
    An insider's look at the Nancy Grace Roman Space TelescopeEmbargoed
    Oct 29, 2026
    Jason Rhodes; Bruce Betts, 2026, "An insider's look at the Nancy Grace Roman Space Telescope", https://doi.org/10.48577/jpl.YXFHKI, Planetary Report, JPL Open Repository
    NA
    Depositional history of the Otis Peak formation, Western fan, Jezero crater, MarsEmbargoed
    Oct 29, 2026
    Samantha Gwizd; Kathryn M. Stack; Michael P. Lamb; Libby R.W. Ives; Sanjeev Gupta; et. al., 2026, "Depositional history of the Otis Peak formation, Western fan, Jezero crater, Mars", https://doi.org/10.48577/jpl.MNUYJC, JGR-Planets, JPL Open Repository
    No abstract available.
    Reading the Future of Space Science
    Oct 29, 2026
    Jonathan I Lunine, 2026, "Reading the Future of Space Science", https://doi.org/10.48577/jpl.2SHYQB, Space Horizons Forum https://research.arizona.edu/events/space-horizons-forum, JPL Open Repository
    No abstract available.
    EMIT Integration Activities
    Oct 29, 2026
    K. Dana Chadwick, 2026, "EMIT Integration Activities", https://doi.org/10.48577/jpl.IZA7TE, Committee on Earth Science and Applications from Space (CESAS) Fall 2026 Meeting, JPL Open Repository
    No abstract available.
    Quantum Advantages
    Oct 28, 2026
    Jason Hyon; Sheng-Wey Chiow; Spencer Johnson; Paul Lundgren; Darmin Arumugam, 2026, "Quantum Advantages", https://doi.org/10.48577/jpl.OBTAE6, ARPA-E Quantum Sensor Network Workshop, JPL Open Repository
    No abstract available.
    Distinguishing N2-Dominated from O2-Dominated Atmospheres on Terrestrial Exoplanets with Reflected-Light SpectroscopyEmbargoed
    Oct 28, 2026
    Nick Burri; Mario Damiano; Renyu Hu, 2026, "Distinguishing N2-Dominated from O2-Dominated Atmospheres on Terrestrial Exoplanets with Reflected-Light Spectroscopy", https://doi.org/10.48577/jpl.8I5PKH, Astronomical Journal, JPL Open Repository
    Reflected-light spectra of Earth-sized exoplanets promise to probe habitability and biosignatures, but interpreting atmospheric oxygen can be challenging because O2 can arise from both biological and abiotic processes. In addition, reflected-light retrievals exhibit degeneracies...
    Add Data

    Log in to create a dataverse or add a dataset.

    Log In
    Share Dataverse

    Share this dataverse on your favorite social media networks.

    Link Dataverse
    Reset Modifications

    Are you sure you want to reset the selected metadata fields? If you do this, any customizations (hidden, required, optional) you have done will no longer appear.