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. 
			
			
| Valley Attached to Northern Mid-Latitude Crater: ESP_089316_2135 ESP_089461_2135 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 33.34 | 7.71 | 5.13 | 17.17 | 47.2 | 47.2 | 
| Megadunes in Hyperborei Cavi: ESP_089212_2620 ESP_089238_2620 (Interval in Earth days: 2) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 82.03 | 312. | -8.3 | 5.626 | 62.8 | 62.2 | 
| Features around Crater in Terra Sabaea: ESP_089319_2205 ESP_089385_2205 (Interval in Earth days: 5) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 39.93 | 284. | 8.56 | -7.88 | 47.1 | 49.1 | 
| Dune Interaction with Residual Polar Ice: ESP_089273_2595 ESP_089365_2595 (Interval in Earth days: 7) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 79.28 | 88.0 | -3.9 | 11.81 | 61.5 | 61.4 | 
| Thermal Anomaly in Young Lava Flows of Elysium Region: ESP_089284_1970 ESP_089429_1970 (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 | 17.03 | 163. | 2.69 | 16.88 | 49.6 | 48.9 | 
| Light-Toned Mesas in Arcadia Planitia: ESP_089560_2260 ESP_089336_2260 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 45.44 | 183. | 12.9 | -21.3 | 49.9 | 50.8 | 
| Avalanche Scarp: ESP_089280_2640 ESP_089386_2640 (Interval in Earth days: 8) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 83.76 | 236. | 6.42 | -8.01 | 63.6 | 65.4 | 
| Dune Interaction with Residual Polar Ice: ESP_089286_2595 ESP_089405_2595 (Interval in Earth days: 9) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 79.46 | 89.3 | 3.05 | -13.8 | 61.3 | 63.6 | 
| Light-Toned Exposures in Capri Chasma: ESP_089582_1665 ESP_089437_1665 (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 | -13.1 | 312. | -0.7 | -17.4 | 62.4 | 64.0 | 
| Layering in Lucus Planum: ESP_089244_1710 ESP_089521_1710 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -9.00 | 178. | 8.29 | -21.2 | 60.3 | 61.9 | 
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