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

Recent Crater on Northern Plains: ESP_069968_2390 ESP_069889_2390 (Interval in Earth days: 6)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
58.81	110.	9.20	-6.73	50.1	51.9
Undeveloped Collapse Pit: ESP_069849_1975 ESP_070060_1975 (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
17.41	127.	7.78	-7.90	50.1	51.5
Fluvial Feature South of Candidate ExoMars Landing Site in Oxia Planum: ESP_069815_1975 ESP_072017_1975 (Interval in Earth days: 171)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
17.56	335.	10.7	-21.7	49.9	53.3
Mounds in Southern Jezero Crater: ESP_069864_1985 ESP_069930_1985 (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
18.13	77.5	12.6	-11.4	49.5	51.5
Layer Exposure in Candidate Alluvial Fan Deposits: ESP_069936_2020 ESP_070938_2020 (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
21.63	272.	-6	6.892	50.1	48.6
Fractured Crater: ESP_069858_2480 ESP_063368_2480 (Interval in Earth days: 505)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
67.95	233.	0.33	-20.6	54.8	63.2
Layered Crater Rim near Mawrth Vallis: ESP_069749_2060 ESP_070039_2060 (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
25.81	337.	4.25	18.89	48.6	47.0
Valley Networks in Arabia Terra: ESP_069945_1880 ESP_069378_1880 (Interval in Earth days: 44)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
7.782	26.2	22.9	-6.58	52.6	51.8
Mounds in Western Oxia Colles: ESP_069802_2005 ESP_069657_2005 (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
20.16	330.	8.76	-7.69	49.3	50.3
Mesa in Chryse Planitia: ESP_069644_1990 ESP_069433_1990 (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
18.86	323.	11.6	-6.14	49.0	49.3
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