The Center for Earth and Planetary Studies (CEPS) data repository provides public access to data from CEPS publications. Contact the corresponding author with questions regarding individual datasets. If you use any of these datasets in research that results in a publication, please include a citation to that dataset and its associated publication.

  1. Evolution of escarpments, pediments, and plains in the Noachian highlands of Mars
    Cawley, J. C., & Irwin, R. P., III (2018). Evolution of escarpments, pediments, and plains in the Noachian highlands of Mars. Journal of Geophysical Research: Planets, 123, 3167–3187. https://doi.org/10.1029/2018JE005681. | Associated Data Files
     
  2. Constraints on the Noachian Paleoclimate of the Martian Highlands From Landscape Evolution Modeling
    Matsubara, Y., Howard, A. D., & Irwin, R. P., III (2018). Constraints on the Noachian paleoclimate of the Martian highlands from landscape evolution modeling. Journal of Geophysical Research: Planets, 123, 2958–2979. https://doi.org/10.1029/2018JE005572. | Associated Data Files​​
     
  3. Incoherently summed SHARAD radargrams of the south polar layered deposits, Mars
    Whitten, J. L., Campbell, B. A. (2018). Lateral continuity of layering in the Mars South Polar Layered Deposits from SHARAD data. Journal of Geophysical Research: Planets, 123. https://doi.org/10.1029/2018JE005578. | Associated Data Files​​
     
  4. Geologic map of wind-eroded crater floors and intercrater plains, Terra Sabaea, Mars
    Irwin, R. P., III, Wray, J. J., Mest, S. C., & Maxwell, T. A. (2018). Wind-eroded crater floors and intercrater plains, Terra Sabaea, Mars. Journal of Geophysical Research: Planets, 123. https://doi.org/10.1002/2017JE005270. | Associated Data Files​​
     
  5. Pyroclastic Flow Deposits on Venus as Indicators of Renewed Mantle Plume Activity
    Campbell, B. A., Morgan, G. A., Whitten, J. L., Carter, L. M., Glaze, L. S., & Campbell, D. B. (2017). Pyroclastic flow deposits on Venus as indicators of renewed magmatic activity. Journal of Geophysical Research: Planets, 122, 1580–1596, doi:10.1002/2017JE005299. | Figure 2, Figure 13a, Figure 13b, Figure 15, Figure 16, Figure 17
     
  6. P-Band (70 cm) same sense circular polarized radar image of Mare Imbrium
    Download Image (41.2MB)
    The data was collected via a bistatic approach using Arecibo to transmit and the the Green Bank telescope to receive (see Campbell et al., 2014 for a detailed description on how high-resolution P-Band data is collected). The data is 7335 columns by 5896 rows and has a spatial resolution of 202 meters per pixel. The projection is simple cylindrical. The upper left corner pixel is 319.69 E, 53.12 N.
    The radar data has was cropped using shapefiles provided by the LROC team online at: http://lroc.sese.asu.edu/data/
     
  7. Improved discrimination of volcanic complexes, tectonic features, and regolith properties in Mare Serenitatis from Earth-based radar mapping
    Campbell, B. A., Ray Hawke, B., Morgan, G. A., Carter, L. M., Campbell, D. B., & Nolan, M. (2014). Improved discrimination of volcanic complexes, tectonic features, and regolith properties in Mare Serenitatis from Earth-based radar mapping. Journal of Geophysical Research: Planets, 119(2), 313–330. http://doi.org/10.1002/2013JE004486
     
  8. 3D Reconstruction of the Source and Scale of Buried Young Flood Channels on Mars
    Morgan, G. A., Campbell, B. A., Carter, L. M., Plaut, J. J., & Phillips R. J. (2013). 3D Reconstruction of the Source and Scale of Buried Young Flood Channels on Mars. Science, 340:6132, 607-610. 
    doi:10.1126/science.1234787. | Journal Supplemental Material