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

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
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
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
Fresh 7-Kilometer Diameter Crater Within Herschel Crater: ESP_019751_1665 ESP_020028_1665 (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
-13.5	128.	10.6	-14.9	57.4	58.2
Possible Future Mars Landing Site near Mawrth Vallis: ESP_019730_2055 ESP_027167_2055 (Interval in Earth days: 580)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
25.21	339.	-15.	5.539	54.8	43.4
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
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
Central Uplift in Crater: ESP_019876_2185 ESP_028355_2185 (Interval in Earth days: 660)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
38.20	309.	8.09	-11.0	57.5	54.1
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
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