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

Furthest Part of Young Channel in Lyot Crater: ESP_025899_2295 ESP_026031_2295 (Interval in Earth days: 10)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
49.20	30.5	20.2	-6.05	40.6	42.7
Cut Crater and Fault Scarp along Candor Chasma: ESP_026114_1745 ESP_025547_1745 (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
-5.51	290.	5.32	-4.4	53.9	50.6
Fan with Light-Toned Deposits: ESP_025990_1995 ESP_026135_1995 (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
19.10	76.1	-27.	-15.8	44.5	43.8
Oudemans Crater Layered Central Uplift: ESP_026194_1700 ESP_026339_1700 (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
-9.86	268.	-8.2	8.812	57.9	57.5
Terrain with Layered Material and Circular Pits: ESP_025976_2290 ESP_026464_2290 (Interval in Earth days: 38)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
48.73	91.1	1.38	-19.8	42.0	43.7
Source Area for Channel Network Near Gigas Sulci: ESP_025905_1980 ESP_026327_1980 (Interval in Earth days: 32)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
17.74	232.	19.4	5.703	40.5	43.1
Channel from Main Athabasca Valles Channel: ESP_025908_1875 ESP_026053_1875 (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
7.418	153.	-1.5	13.07	46.2	45.9
Crater with Viscous Flows and a Channel: ESP_025970_2235 ESP_025904_2235 (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
42.90	257.	-8.9	7.02	41.4	40.1
Light-Toned Material along Coprates Chasma Wallrock and Plateau: ESP_025929_1645 ESP_026430_1645 (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
-15.5	303.	-6.5	17.74	60.0	61.1
Dark Slope Streak Extending to Channel Floor: ESP_026064_2045 ESP_026697_2045 (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
24.17	212.	0	-15.4	41.0	44.0
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