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

Depositional Fan in Hargraves Crater: ESP_042816_2010 ESP_042961_2010 (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
20.88	75.4	1.38	14.45	39.2	38.4
Possible Sulfate-Rich Terrain in Northeast Syrtis Major Region: ESP_042750_1970 ESP_043172_1970 (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
16.63	77.4	7.00	-9.18	39.0	41.7
Possible Multi-Terraced Crater in Arcadia Planitia: ESP_042996_2210 ESP_043273_2210 (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
40.56	197.	8.28	-12.5	40.8	41.7
Tectonics in Hebes Chasma: ESP_042914_1795 ESP_042413_1795 (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
-0.78	282.	4.83	-11.6	45.6	42.7
Mars 2020 Candidate Landing Site in Mclaughlin Crater: ESP_042991_2020 ESP_043136_2020 (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
21.64	337.	-0.2	13.11	39.7	38.8
Double-Terrace Crater in Arcadia Planitia: ESP_043036_2275 ESP_043102_2275 (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
47.23	183.	16.5	2.794	42.2	43.0
Light-Toned Layered Material along Ius Chasma Plateau: ESP_042822_1715 ESP_043534_1715 (Interval in Earth days: 55)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-8.21	275.	-0.0	18.35	48.9	53.2
Coprates Region Falling Dunes and Landslide Scarps: ESP_043098_1650 ESP_043599_1650 (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
-15.0	303.	-25.	1.007	57.2	59.1
Central Mound of Crater in Tyrrhena Terra: ESP_042934_1690 ESP_043356_1690 (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
-10.6	98.2	-5.6	-19.9	51.7	56.1
Steep Slopes in Melas Chasma: ESP_043072_1685 ESP_043573_1685 (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
-11.3	290.	-7.9	19.28	53.5	55.3
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