The two Narrow Angle Cameras (NACs) provide high-resolution (0.5 to 2.0 m/pixel) panchromatic images over a combined 5 km swath. NAC images acquired on consecutive orbits, or occasionally over non-consecutive orbits under very similar lighting conditions (e.g. less than 5° difference in incidence angle and the same sun direction), can be combined to create controlled mosaics. A control network is generated to tie the images to the most accurate ground truth available and a bundle adjustment is performed to correct for pointing errors and image alignment. The images are then map-projected using the GLD100 (WAC derived 100 m/pixel DTM) and LOLA derived crossover corrected ephemeris and mosaicked together into an almost seamless mosaic of the region.

When citing this product, use the following reference:

Klem, S. M., Henriksen, M. R., Stopar, J., Boyd, A., & Robinson, M. S. (2014). Controlled LROC Narrow Angle Camera High Resolution Mosaics. In Lunar and Planetary Science Conference (Vol. 45, abstract #2885).

Site Name Serenitatis Lobate Flow
Center Lat 27.3
Center Lon 14.2
Pixel Scale 1.10 m/px
# Images 8
Incidence Low Sun

Images used, in order of layering from front to back:
Image ID Center Lat Center Lon Incidence Pixel Scale
M1245925137R 27.26 14.32 77° 1.12 m/px
M1245925137L 27.25 14.52 76° 1.12 m/px
M1245918104R 27.25 14.74 77° 1.15 m/px
M1245918104L 27.24 14.95 77° 1.14 m/px
M1245932170R 27.27 13.92 76° 1.12 m/px
M1245932170L 27.26 14.12 76° 1.12 m/px
M1245939203R 27.29 13.51 76° 1.15 m/px
M1245939203L 27.28 13.72 75° 1.16 m/px

Serenitatis Lobate Flow low-Sun controlled NAC mosaic (B)

Mosaic (1.10 m/px) (click for more information)