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

Pitted and Fractured Surfaces in Southern Mojave Region: ESP_014034_1870 ESP_014311_1870 (Interval in Earth days: 21)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
7.105	327.	0.98	-24.4	43.1	41.9
Active Geyser Locale: ESP_014083_0945 ESP_014122_0945 (Interval in Earth days: 3)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-85.4	103.	8.28	22.35	69.3	68.8
Floor of Mawrth Vallis: ESP_014007_2030 ESP_022578_2030 (Interval in Earth days: 668)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
22.98	341.	9.10	25.33	53.5	54.6
Lobate Features in the Charitum Montes: ESP_013165_1275 ESP_013244_1275 (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
-51.9	301.	-4.0	20.40	45.0	42.6
Possible Cyclic Bedding in Arabia Terra: ESP_013611_1910 ESP_014033_1910 (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
10.87	355.	0.61	-17.2	50.8	46.6
Light-Toned Outcrops along Ius Region Wallrock: ESP_012849_1705 ESP_013126_1705 (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
-9.22	281.	-3.9	-28.8	49.2	48.0
Martian Volcanic Vent with Elevated Rim: ESP_013008_1825 ESP_020801_1825 (Interval in Earth days: 607)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
2.452	259.	-3.3	21.93	52.7	53.7
Central Pit Gullies in Asimov Crater: ESP_013123_1330 ESP_013268_1330 (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
-46.8	4.93	13.8	22.63	42.3	40.3
Olympus Mons Aureole: ESP_013273_2015 ESP_014262_2015 (Interval in Earth days: 77)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
21.19	220.	12.1	-1.21	60.9	49.4
Rocky Deposit on Crater Floor with Thermal Signature: ESP_012788_1365 ESP_013856_1365 (Interval in Earth days: 84)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-43.2	151.	2.54	20.66	46.5	37.4
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