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

Crossing Ridges in Dorsa Argentea: ESP_012729_1020 ESP_013032_1020 (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
-77.8	337.	-6.9	14.65	62.3	58.2
Channels and Noachian Crater Fill: ESP_012709_1445 ESP_013197_1445 (Interval in Earth days: 38)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-35.2	146.	1.58	-27.4	46.6	42.6
Faulting in South Polar Layered Deposits: ESP_012762_1070 ESP_013171_1070 (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
-72.9	146.	10.3	-12.8	58.0	56.3
Rayed Crater: ESP_013955_1020 ESP_013968_1020 (Interval in Earth days: 1)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-77.8	345.	-6.7	7.228	62.3	61.6
Steep Lobate Scarps in Kasei Valles: ESP_012717_1910 ESP_013139_1910 (Interval in Earth days: 33)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
10.88	282.	2.07	-8.93	59.1	56.6
Light-Toned Material in a Crater in Terra Cimmeria: ESP_013750_1440 ESP_021543_1440 (Interval in Earth days: 608)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-35.8	166.	-2.2	19.05	36.5	43.0
Well-Preserved Crater with Central Peak in Chryse Planitia: ESP_013810_2085 ESP_022869_2085 (Interval in Earth days: 706)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
28.43	319.	5.59	-12.7	60.4	56.9
Her Desher Vallis: ESP_013771_1550 ESP_020562_1550 (Interval in Earth days: 529)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-24.7	311.	-2.6	-22.5	35.2	57.6
Western Slope of Asimov Crater: ESP_013110_1325 ESP_013611_1325 (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
-47.0	4.17	-23.	-7.91	45.4	41.0
Hill and Adjacent Depression in Polar Layered Deposits: ESP_012815_1080 ESP_013013_1080 (Interval in Earth days: 15)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-71.7	141.	1.59	-20.3	57.3	57.1
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