WAC Percentage-Based South Pole Illumination Map

The Lunar Reconnaissance Orbiter Camera (LROC) provides multi-temporal images of the polar regions, with repeat imaging with the Wide-Angle Camera approximately every 2 hours with a ground sampling distance of 100 meters enabling production of an illumination map from 88 to 90° south. WAC images (n=3807) acquired over one lunar year from 15 February 2010 to 5 February 2011 form the basis of the map. Temporal gaps were filled with 229 observations acquired with virtually identical lighting at other times during the mission. Each image was first map-projected at 100 meters/pixel in polar stereographic projection onto a 30 m LOLA DEM (Smith et al., 2010) using an improved WAC distortion model (Speyerer et al., 2016) and improved spacecraft ephemeris (Mazarico et al., 2011). Binary images indicating the illumination state of each image were created by applying a series of spatial filters and a conservative global threshold. Then the illumination map was derived by taking the number of times a mapped pixel was illuminated over the number of instances the mapped pixel was imaged. This map may contain some biases due to non-uniform timing between observations (Example- WAC images were not acquired on orbits when Mini-RF acquired polar observations). To limit this non-linear effect, an additional time-weighted illumination map is provided that linearly interpolated missed observations (see WAC_POLE_ILL_TWI_NORTH and WAC_POLE_ILL_TWI_SOUTH). For more information on the derivation of these products and for a map of image counts per pixel, see Speyerer and Robinson (2013). Due to a small amount of image noise and scattered light, some regions that are permanently shadowed from direct solar illumination have percentage values that are close to, but not equal to zero. These artifacts in the middle of permanently shadowed regions should be ignored when analyzing the extent.

Low-resolution 8-bit browse products in PNG format for this product, along with full-resolution 8-bit GeoTIFFs, are available at the following location, with names matching those of the full-resolution IMG files: http://lroc.sese.asu.edu/data/LRO-L-LROC-5-RDR-V1.0/LROLRC_2001/EXTRAS/BROWSE/WAC_POLE/WAC_POLE_ILL_PCT_SOUTH/

When citing this product, use the following reference: Speyerer, E. J., & Robinson, M. S. (2013). Persistently illuminated regions at the lunar poles: Ideal sites for future exploration. Icarus, 222(1), 122-136. doi:10.1016/j.icarus.2012.10.010.

References:

Mazarico, E., Rowlands, D. D., Neumann, G. A., Smith, D. E., Torrence, M. H., Lemoine, F. G., & Zuber, M. T. (2012). Orbit determination of the Lunar Reconnaissance Orbiter. Journal of Geodesy, 86(3), 193-207. doi:10.1007/s00190-011-0509-4

Smith, D. E., Zuber, M. T., Neumann, G. A., Lemoine, F. G., Mazarico, E., Torrence, M. H., McGarry, J. F., Rowlands, D. D, Head III, J. W., Duxbury, T. H., Aharonson, O., Lucey, P. G., Robinson, M. S., Barnouin, O. S., Cavanaugh, J. F., Sun, X., Liiva, P., Mao, D., Smith, J. C., & Bartels A. E. (2010). Initial observations from the Lunar Orbiter Laser Altimeter (LOLA). Geophysical Research Letters, 37(18). doi:10.1029/2010GL043751

Speyerer, E. J., Wagner, R. V., Robinson, M. S., Licht, A., Thomas, P. C., Becker, K., Anderson, J., Brylow, S. M., Humm, D. C., & Tschimmel, M. (2014). Pre-flight and on-orbit geometric calibration of the Lunar Reconnaissance Orbiter Camera, Space Science Reviews, 200, 357–392. doi:10.1007/s11214-014-0073-3

Speyerer, E. J., & Robinson, M. S. (2013). Persistently illuminated regions at the lunar poles: Ideal sites for future exploration. Icarus, 222(1), 122-136. doi:10.1016/j.icarus.2012.10.010

For more information on LROC Reduced Data Records (RDRs), please refer to the LROC RDR Software Interface Specification (SIS).

WAC Percentage-Based South Pole Illumination Map