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

Enigmatic Channel Carved into the Floor of Mangala Valles: ESP_033686_1635 ESP_033831_1635 (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
-16.1	210.	-23.	-7.27	51.4	52.2
Possible Smectite Deposits in Northwest Hellas Region: ESP_033652_1580 ESP_041907_1580 (Interval in Earth days: 643)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-21.6	57.2	2.99	20.83	52.5	43.8
Marte Vallis Channel between Crater Ejecta: ESP_033423_1970 ESP_033713_1970 (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
16.63	184.	-1.8	25.48	37.7	36.4
Light-Toned Layered Deposits Exposed along Ladon Valles Floor: ESP_033642_1585 ESP_033787_1585 (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
-21.0	330.	-3.9	12.32	52.4	53.4
Pit South of Arsia Mons: ESP_033342_1660 ESP_050089_1660 (Interval in Earth days: 1305)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-13.8	240.	-0.3	-8.91	43.9	32.6
High-Lava Mark in Kasei Valles: ESP_033617_1990 ESP_034316_1990 (Interval in Earth days: 55)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
18.64	285.	20.6	-9.79	36.5	42.1
Pedestal Crater Modification: ESP_033663_2395 ESP_033953_2395 (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
59.21	104.	6.93	21.26	53.6	49.9
Pedestal Crater and Mantle: ESP_033612_2300 ESP_033744_2300 (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
49.83	59.1	3.92	-21.3	48.5	49.4
Floor of Mclaughlin Crater: ESP_033391_2020 ESP_037149_2020 (Interval in Earth days: 293)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
21.90	337.	1.00	18.02	38.3	51.1
Flow Boundary in Phlegra Dorsa: ESP_033608_2085 ESP_034109_2085 (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
28.33	172.	-2.7	21.29	39.9	37.9
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