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Lunar Orbiter UVVIS and NIR Warp Mosaics - USGS Lunar Updates (October 2008)

Explore the latest updates from the USGS regarding the Lunar Orbiter's UVVIS and NIR warp mosaics. This resource contains high-resolution images and detailed analysis for lunar topography utilizing Clementine data. It features optimized server processing for raster graphics and real-time handling of discrete images, ensuring efficient access to geological and topographic information. The data is available for download, leveraging existing funding and supporting integrated surface visualization for lunar research and exploration.

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Lunar Orbiter UVVIS and NIR Warp Mosaics - USGS Lunar Updates (October 2008)

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  1. USGS Lunar UpdatesOct. 2008 UVVIS and NIR Warp Mosaics Lunar Orbiter (jpeg2000 mosaic) NASM1KM Topography JPL’s onMoon GIS Server LO UVVIS Basemap Merge

  2. Lunar GIS • For More: • Hare 2007 • Cohen 2008 • Thaisen 2008

  3. Clementine Warp (6th order polynomial warp) • 30x30 degree tiles • mean RMS errors X, Y (181.94, 178.90) meters

  4. UVVIS Warp / LO Blink

  5. Clementine Warp http://webgis.wr.usgs.gov/pigwad/maps  Moon  Apollo Viewer

  6. Clementine Warp (6th order polynomial warp) • M3 Targeting in REACT • LROC Targeting in REACT (JMoon?) • http://www.google.com/moon • LMMP Infrastructure (OnMoon) • Available for download on PIGWAD

  7. OnMoon (JPL) Integrated Surface VisualizationExamples of Possible LMMP Products Description: • Optimized OGC/KML support • Focus on quick response and server processing for rasters • Handles high-resolution discrete images in real-time Rationale: • Leverages existing funding • Cached servers can be housed locally for non-public data layers.

  8. NASM1KM Topography http://webgis.wr.usgs.gov/pigwad/down/moon_dl.htm

  9. LAC mosaics (geology and topography)

  10. Clementine Mineral Ratio over LO

  11. LO and UVVIS Basemap Merge

  12. LO and UVVIS Basemap Merge 100 km

  13. Questions

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