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

Light-Toned Layering on Plains Next to Ganges Chasma: PSP_005161_1720 ESP_016237_1720 (Interval in Earth days: 863)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-8.14	307.	6.27	-10.6	35.3	48.9
Sinuous Ridge in Dark Lava Flow in Western Elysium Planitia: PSP_006723_1865 PSP_007013_1865 (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
6.196	140.	-7.6	15.48	37.8	37.9
Ridges in Nili Fossae Phyllosilicates: PSP_005855_2020 PSP_006712_2020 (Interval in Earth days: 67)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
21.80	77.1	-2.4	7.233	44.7	38.7
Basal Exposure of South Polar Layered Deposits: PSP_005089_1040 PSP_005313_1040 (Interval in Earth days: 18)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-75.8	131.	-6.9	7.077	60.1	61.9
Alcove in West Hellas Region: PSP_006753_1425 PSP_010814_1425 (Interval in Earth days: 317)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-37.0	45.9	0	-22.6	56.4	72.8
Avalanche Features of Dune Slip Face Seen in MOC Image R06-00380: PSP_006899_1330 PSP_006965_1330 (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
-46.7	20.1	8.63	-9.75	65.3	67.4
Light-Toned Layering along Plains Adjacent to Melas Chasma: PSP_005030_1685 ESP_012427_1685 (Interval in Earth days: 576)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-11.2	284.	3.48	-15.1	35.7	53.6
Small Valley Delta in Crater Near Maja Valles: PSP_005926_1850 ESP_011279_1850 (Interval in Earth days: 417)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
4.925	301.	-8.3	17.11	36.4	55.6
On the Floor of the Labyrinth of the Night: PSP_006969_1725 ESP_028093_1725 (Interval in Earth days: 1646)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-7.38	263.	5.15	28.42	42.3	54.3
Alluvial Fan in Crater East of Maja Valles: PSP_006941_1825 PSP_007732_1825 (Interval in Earth days: 61)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
2.684	308.	-8.3	7.693	39.9	45.8
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