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

West Rim of 11-Kilometer Crater in Tyrrhena Terra: ESP_029880_1710 ESP_030658_1710 (Interval in Earth days: 61)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-9.13	79.2	8.92	-6.32	51.0	45.4
Well-Preserved 2-3 Km Impact Crater: ESP_029962_1800 ESP_030463_1800 (Interval in Earth days: 39)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-0.08	1.00	-8.8	3.197	54.4	50.6
Compositional Diversity in Northern Hellas Region: ESP_030092_1530 ESP_029815_1530 (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
-26.7	55.2	-12.	17.29	48.7	49.8
Central Uplift in Impact Crater: ESP_029985_1710 ESP_030196_1710 (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
-9.07	92.9	6.87	-9.52	50.5	50.1
Portion of Gale Crater Mound: ESP_030102_1750 ESP_030880_1750 (Interval in Earth days: 60)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-5.03	137.	9.9	-8.53	50.6	44.8
Gullied Niquero Crater: ESP_030021_1410 ESP_030443_1410 (Interval in Earth days: 33)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-38.7	193.	4.97	-16.9	49.4	45.0
Light-Toned Gully Deposits in Hale Crater: ESP_030003_1440 ESP_030214_1440 (Interval in Earth days: 16)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-35.4	324.	5.96	-8.14	49.1	47.1
Valleys with Layered Sediments along Uplands at Ladon Valles Basin: ESP_029871_1615 ESP_031084_1615 (Interval in Earth days: 94)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-18.5	326.	5.61	27.24	50.1	34.7
Candidate Future Landing Site in Sabrina Vallis Delta: ESP_029845_1920 ESP_029990_1920 (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
11.97	313.	-7.3	11.05	59.1	57.8
Fresh Small Rayed Crater: ESP_029908_1660 ESP_029974_1660 (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
-13.7	34.2	22.6	1.785	48.9	50.0
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