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

Gullies in a Crater Wall: PSP_007977_2385 PSP_008043_2385 (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
58.24	89.7	4.13	-8.34	47.7	48.4
Mesas in Huo Hsing Vallis: PSP_007688_2075 PSP_008690_2075 (Interval in Earth days: 78)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
27.10	66.7	5.61	-11.4	40.1	43.9
Chasma Borealis: PSP_007020_2580 PSP_007178_2580 (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
77.78	292.	0	12.81	69.8	67.1
Possible Sulfates in Ius Chasma: PSP_007509_1720 ESP_050839_1720 (Interval in Earth days: 3376)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-7.70	279.	-2.3	13.43	49.3	36.5
Layering in Eastern Central Peak of Oudemans Crater: PSP_007193_1700 PSP_008195_1700 (Interval in Earth days: 79)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-9.89	268.	4.49	-6.29	46.3	57.2
Dark Dune-Like Forms in Southern Melas Chasma: PSP_007522_1685 ESP_025666_1685 (Interval in Earth days: 1414)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-11.1	284.	0.94	-27.7	51.1	56.6
Central Peak of Unnamed Crater within the Medusae Fossae Formation: PSP_007870_1830 PSP_009228_1830 (Interval in Earth days: 106)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
3.031	140.	4.36	-20.5	47.0	55.2
Light-Toned Outcrops Exhumed From Dark Material in Arabia Terra: PSP_008139_1905 PSP_009576_1905 (Interval in Earth days: 112)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
10.54	355.	-7.9	17.40	46.6	49.4
Geologic Contacts in Mangala Valles: PSP_007617_1750 PSP_007973_1750 (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
-4.85	209.	5.90	-6.28	48.4	52.6
Debris Flows on Mars: PSP_007033_1445 ESP_016197_1445 (Interval in Earth days: 714)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-34.9	321.	-6.8	8.328	59.9	64.1
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