We are excited to announce that the Planetary Data System (PDS) will be hosting talks, demos, and drop-in consulting hours at LPSC in Houston from Monday, March 10th through Thursday, March 13th. Whether you're a seasoned researcher or a curious newcomer, our team is here to help you navigate the cosmos of planetary data. Full schedule: https://wufs.wustl.edu/lpsc-web/lpsc2025.htm

Release 72 from the Mars Reconnaissance Orbiter mission includes new SHARAD and gravity data. The data are online at https://pds-geosciences.wustl.edu/missions/mro.

Hello Sehaj, What I mentioned is about the spatial reconciliation between S and L data. And before that, there are multiple corrections to conduct. For the detailed processing, you may follow the below processing flowchart: Thanks, Feng

Thanks again @Feng in replying to my query. What do you mean by "the same base"? While mapping the S and L data of the same observation using CAT, won't the base be already same? Or Do I need to do adjust something manually? And by "combining the registered output", do you mean combining the generated plot values of both together (after getting the spectra of ROI of the geographically linked pixels)?

Hello Sehaj, If you want to get the full spectral profile from the L and S products, you can follow the similar procedure like MTRDR.  Map project the S and L data, register the projected results on the same base, finally combine the registered output together. Directly combine S and L products is not correct.  Please let me know if you have any questions. Thanks, Feng