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. 
			
			
| Deflected Ejecta of Arabia Region Crater: ESP_017356_2175 ESP_024872_2175 (Interval in Earth days: 586) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 37.02 | 350. | 0 | 20.49 | 41.2 | 39.9 | 
| Terraced Pedestal Crater in CTX Image: ESP_017497_2325 ESP_017774_2325 (Interval in Earth days: 22) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 52.23 | 97.6 | 3.87 | -14.3 | 43.3 | 45.0 | 
| Possible Clay Beds in West Ladon Valles Channels: ESP_017489_1610 ESP_035119_1610 (Interval in Earth days: 1374) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -18.9 | 326. | -5.8 | -19.4 | 65.4 | 66.3 | 
| Lava Delta in Eastern Tharsis Region: ESP_017307_2050 ESP_017729_2050 (Interval in Earth days: 32) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 24.97 | 249. | 4.76 | -11.9 | 41.7 | 44.1 | 
| Pits on Fan Surfaces in Mojave Crater: ESP_017568_1870 ESP_018069_1870 (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 | 7.120 | 326. | -6.1 | 13.95 | 49.9 | 49.5 | 
| Impact Crater Exposing Stratigraphy in Eos Chasma: ESP_017463_1630 ESP_018241_1630 (Interval in Earth days: 60) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -16.6 | 315. | 4.08 | -7.28 | 63.1 | 65.0 | 
| Crater Cut by Horst and Graben: ESP_017399_2185 ESP_017900_2185 (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 | 38.10 | 256. | -4.2 | 10.29 | 41.5 | 41.1 | 
| Circular Features in Far Northern Reaches of Arcadia Planitia: ESP_017632_2475 ESP_018634_2475 (Interval in Earth days: 78) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 67.05 | 9.22 | -2.5 | 13.14 | 49.8 | 52.6 | 
| Unnamed Crater on Rim of Valles Marineris: ESP_017556_1650 ESP_018268_1650 (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 | -14.7 | 297. | -12. | 0.635 | 63.2 | 63.2 | 
| Well-Preserved Impact Crater in Tempe Terra: ESP_017345_2200 ESP_017846_2200 (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 | 39.72 | 291. | -6.3 | 7.647 | 41.8 | 41.2 | 
| Page 663 of 866 (8,658 images) | |||||