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. 
			
			
| Gullies with Dark Channel or Deposit: ESP_022283_1420 ESP_022916_1420 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -37.7 | 126. | -6.8 | -24.4 | 36.9 | 37.7 | 
| Possible Source Region of Harris Crater Fan: ESP_022140_1585 ESP_021784_1585 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -21.4 | 67.2 | 3.34 | -9.00 | 37.3 | 42.6 | 
| Inverted Valleys near Juventae Chasma: PSP_007627_1765 PSP_008563_1765 (Interval in Earth days: 73) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -3.67 | 297. | -4.8 | 5.755 | 48.7 | 55.0 | 
| Possible Inverted Topography Landscape with Clay Minerals: ESP_022077_2000 ESP_022367_2000 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 19.80 | 342. | -1.5 | 22.08 | 59.3 | 54.9 | 
| Hematite in Eos Chasma: ESP_021775_1665 ESP_022408_1665 (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 | -13.3 | 311. | -3.6 | -23.2 | 44.4 | 38.4 | 
| Mounds North of Simud Valles Region Chaos: ESP_021880_1950 ESP_030359_1950 (Interval in Earth days: 661) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 14.75 | 320. | 4.40 | -21.0 | 57.2 | 60.9 | 
| Lava Flow Features in Marte Vallis: ESP_021964_2015 ESP_030232_2015 (Interval in Earth days: 645) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.01 | 186. | 4.43 | -13.0 | 60.8 | 64.2 | 
| Mesas and Buttes of Hydraotes Chaos: ESP_021893_1805 ESP_031163_1805 (Interval in Earth days: 722) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 0.634 | 327. | 3.40 | 22.57 | 48.7 | 42.4 | 
| Bedform Changes in Aureum Chaos: ESP_021906_1765 ESP_022183_1765 (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 | -3.64 | 333. | -1.9 | -28.1 | 46.7 | 45.5 | 
| Candidate New Gully Flow Formed between 15 May 2009 and 3 March 2011: ESP_021914_1475 ESP_022336_1475 (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 | -32.3 | 118. | 3.26 | -10.0 | 39.2 | 35.9 | 
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