Planned stereo pairs have suitable stereo convergence angles and illumination by design. 
			In addition to planned stereo pairs, the Pairendipity software can identify overlapping 
			HiRISE images that are serendipitously suitable for stereo processing and find stereo 
			pairs within the CTX dataset.
			
			
			Planned HiRISE stereo pairs are listed in the “Stereo Pair List (CSV)” link below.
			Since this list is based on produced stereo anaglyphs it also contains a few serendipitous 
			pairs that underwent special processing. Most serendipitous HiRISE stereo pairs are listed 
			in the “Pairendipity Stereo” link, while CTX stereo pairs are listed 
			in  “Pairendipity CTX Stereo”.
			
			
			
			Images taken close together in time minimize illumination and frost differences and are 
			especially useful (see the Delta-Days column in the Pairendipity files or difference 
			the orbit numbers in the image IDs in the Stereo Pair List file). Stereo pairs 
			with both images planned within the same 14-day (168-orbit) operations cycle are known as SPORCs. 
			
			
| Well-Preserved 5-Kilometer Diameter Impact Crater: ESP_018478_2150 ESP_018979_2150 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 34.78 | 318. | -3.5 | 13.05 | 44.5 | 46.3 | 
| Exposure of North Polar Layered Deposits in Area Not Well Observed: ESP_018376_2685 ESP_019113_2685 (Interval in Earth days: 57) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 88.32 | 200. | -20. | -13.4 | 65.1 | 71.7 | 
| Well Developed Hollows and Ridges in Nilosyrtis Region Crater: ESP_018144_2185 ESP_018856_2185 (Interval in Earth days: 55) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 37.98 | 75.6 | 6.46 | 17.99 | 42.1 | 45.1 | 
| Rim and Ejecta of Very Fresh 7-Kilometer Diameter Impact Crater: ESP_018268_2335 ESP_033854_2335 (Interval in Earth days: 1215) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 53.34 | 289. | -4.9 | 20.21 | 46.1 | 47.4 | 
| Cones at Edge of North Polar Layered Deposits: ESP_018333_2605 ESP_018926_2605 (Interval in Earth days: 46) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 80.20 | 295. | 6.93 | 22.29 | 58.1 | 62.3 | 
| Protonilus Mensae Fretted Terrain: ESP_018448_2250 ESP_062913_2250 (Interval in Earth days: 3465) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 44.85 | 56.1 | -3.9 | 7.677 | 45.1 | 46.8 | 
| Erosional Surface Features in Arabia Terra: ESP_018488_2120 ESP_019345_2120 (Interval in Earth days: 66) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 31.70 | 46.1 | -5.1 | 17.79 | 44.8 | 48.9 | 
| Columbus Crater: ESP_018351_1510 ESP_018496_1510 (Interval in Earth days: 11) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -28.7 | 194. | -7.0 | 8.364 | 73.0 | 71.7 | 
| Layered Flow Ejecta in Terra Cimmeria: ESP_018379_1695 ESP_018880_1695 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -10.4 | 146. | 6.62 | 27.95 | 60.0 | 57.5 | 
| Steep North-Polar Boundary Scarp: ESP_018190_2640 ESP_018941_2640 (Interval in Earth days: 59) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 84.01 | 230. | 1.83 | 15.95 | 60.1 | 65.4 | 
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