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

Fresh Impact Crater: ESP_019784_1900 ESP_020140_1900 (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
9.847	305.	0	14.10	53.3	53.9
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
Viscous Flow Feature: ESP_019635_2205 ESP_019780_2205 (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
40.38	49.0	3.74	15.81	55.2	56.2
Central Peak of Northern Plains Crater: ESP_019658_2345 ESP_020159_2345 (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
54.34	139.	-2.4	13.47	61.1	68.0
Well-Preserved Impact Crater with Central Uplift and Glacial Flow Features: ESP_019657_2125 ESP_020290_2125 (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
32.24	169.	8.74	-4.23	53.1	61.9
Candidate MSL Landing Site in Holden Crater: ESP_019612_1535 ESP_019678_1535 (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
-26.4	325.	8.73	-12.3	63.9	64.9
Possible Future Mars Landing Site in South Meridiani Planum: ESP_019690_1765 ESP_019624_1765 (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
-3.42	354.	-9.7	12.95	56.1	54.3
Crater and Landslides in CTX Image: ESP_019647_1625 ESP_020003_1625 (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
-17.3	89.9	-6.6	7.971	60.6	57.7
Densest Pit and Fracture Concentrations in Mojave Crater Fill: ESP_019625_1875 ESP_028183_1875 (Interval in Earth days: 667)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
7.492	327.	-3.2	6.008	53.2	51.0
Fracture Cutting Lava Flow East of Olympus Mons: ESP_019681_1975 ESP_019747_1975 (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
17.41	235.	11.4	-9.56	51.6	53.8
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