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

Small Crater Filled By Deltaic Deposits: PSP_006954_1885 ESP_016250_1885 (Interval in Earth days: 724)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
8.520	312	-0.3	-27.7	38.5	44.0
Intersecting Ridges in the Dorsa Argentea: PSP_006255_1020 ESP_023911_1020 (Interval in Earth days: 1376)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-77.8	336.	0	-11.9	79.0	79.9
Streamlined Features in Argyre Planitia: PSP_006163_1345 ESP_011714_1345 (Interval in Earth days: 433)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-45.3	316.	0	-23.3	52.2	65.7
Columnar Jointing Exposed in An Impact Crater in Marte Vallis: PSP_006774_2020 PSP_007341_2020 (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
21.57	184.	7.5	-9.82	38.5	40.5
Central Peak of Well-Preserved Unnamed Crater: PSP_006782_1630 PSP_006927_1630 (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
-16.7	331.	-6.1	5.697	45.0	46.2
Gorgonum Chaos: PSP_006906_1425 ESP_016004_1425 (Interval in Earth days: 709)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-37.2	188.	1.20	29.59	58.9	61.5
Sinuous Ridge in Argyre Basin: PSP_006730_1235 PSP_007007_1235 (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
-56.1	316.	7.79	-14.4	69.5	75.4
Evolution of Surface Near the Granicus and Tinjar Valles: PSP_005932_2080 ESP_057873_2080 (Interval in Earth days: 4047)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
27.73	135.	-18.	2.277	48.7	58.1
Layering along Oudemans Crater Wall: PSP_005057_1695 PSP_005690_1695 (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
-10.1	267.	2.39	-22.3	35.8	34.8
Unnamed Well-Preserved Central Pit Crater: PSP_005600_1160 PSP_005890_1160 (Interval in Earth days: 23)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-63.5	212.	-5.0	11.46	56.8	60.5
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