HiRISE | Stereo Pairs

Stereo Pairs

An explanation of stereo pairs and their use (PDF)

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.

Stereo Pair List (csv) Pairendipity Stereo Pairendipity CTX Stereo SPORCs

Landslide Scarps in Large Crater: ESP_019955_1520 ESP_020100_1520 (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
-27.5	322.	-7.4	10.43	62.7	60.2
Well-Preserved 9-Kilometer Diameter Crater in Acidalia Planitia: ESP_019704_2195 ESP_020337_2195 (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
39.13	325.	1.8	-10.9	56.0	65.7
Layered Rock along Walls of South Ius Chasma: ESP_019785_1705 ESP_028132_1705 (Interval in Earth days: 650)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-9.21	281.	-8.1	5.223	57.3	56.8
The Beautiful Arc of a Dune: ESP_019992_1340 ESP_020269_1340 (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
-45.5	33.9	8.50	-14.2	69.5	67.2
Contact between Wallrock and Light-Toned Layering in West Candor Chasma: ESP_019719_1750 ESP_020075_1750 (Interval in Earth days: 27)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-4.90	282.	-8.7	6.86	56.3	54.8
Eastern Edge of Eberswalde Crater Delta in Possible MSL Rover Landing Site: ESP_019757_1560 ESP_020034_1560 (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
-23.8	326.	7.74	-16.3	61.7	61.4
Possible MSL Rover Landing Site in Holden Crater: ESP_019823_1530 ESP_019889_1530 (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
-26.5	325.	8.09	-12.7	62.3	63.3
Lower Northwest Portion of Mound in Gale Crater: ESP_019698_1750 ESP_019988_1750 (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
-4.88	137.	-22.	13.72	57.5	54.3
Extensive Debris Apron near Reull Vallis: ESP_019897_1370 ESP_020530_1370 (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
-42.7	107.	0	-17.4	69.8	62.5
Central Peak of Crater in Tyrrhena Terra: ESP_019951_1510 ESP_028509_1510 (Interval in Earth days: 666)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-28.6	72.1	-5.4	11.57	63.1	63.5
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