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. 
			
			
| Debris Apron in Phlegra Montes: ESP_018431_2270 ESP_019077_2270 (Interval in Earth days: 51) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 46.4 | 162. | -18. | 4.633 | 46.6 | 50.0 | 
| Streamlined Form at the Confluence of Tiu Valles and Ares Vallis: ESP_018491_1975 ESP_018636_1975 (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 | 17.23 | 326. | -4.3 | 11.33 | 47.5 | 46.6 | 
| 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 | 
| Exposure of North Polar Layered Deposits: ESP_018237_2720 ESP_019053_2720 (Interval in Earth days: 64) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 87.90 | 293. | -9.5 | -21.3 | 65.1 | 73.4 | 
| Light-Toned Outcrops in Noctis Region: ESP_018480_1725 ESP_024994_1725 (Interval in Earth days: 508) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.30 | 268. | 7.71 | -7.73 | 58.0 | 46.2 | 
| Channel and Depression in Northeast Syrtis Major Planum: ESP_018210_1980 ESP_034772_1980 (Interval in Earth days: 1290) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.69 | 76.8 | 4.91 | -22.5 | 45.9 | 45.4 | 
| Lava Channel and Cataract in South-Central Elysium Planitia: ESP_018339_1820 ESP_018194_1820 (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 | 2.117 | 157. | -0.8 | -16.4 | 53.3 | 54.4 | 
| Noctis Labyrinthus Terrain: ESP_018441_1735 ESP_045579_1735 (Interval in Earth days: 2115) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.28 | 253. | -2.1 | -25.1 | 58.1 | 55.0 | 
| Relatively Young Crater Ejecta and Apron in Deuteronilus Mensae: ESP_018423_2230 ESP_019056_2230 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 42.74 | 18.1 | 3.74 | -12.5 | 44.0 | 50.4 | 
| North Polar Residual Cap: ESP_018289_2655 ESP_018593_2655 (Interval in Earth days: 24) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 85.19 | 34.7 | 5.01 | -9.35 | 61.3 | 63.9 | 
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