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

Chaos and Outflow Channel Floor Transition in Osuga Valles: ESP_027392_1650 ESP_027880_1650 (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
-15.0	322.	8.60	-5.08	61.6	61.1
Central Peak of Fournier Crater in Tyrrhena Terra: ESP_027322_1755 ESP_027810_1755 (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
-4.38	72.6	-1.4	-16.4	56.0	56.7
Linear Ridges: ESP_027229_1825 ESP_028350_1825 (Interval in Earth days: 87)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
2.474	89.8	7.62	-4.36	51.7	53.4
Depression in CTX P13_006195_1728_XN_07S202W and THEMIS V14574001: ESP_027398_1740 ESP_027886_1740 (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
-5.87	157.	6.23	-7.42	56.3	56.6
Phyllosilicate Deposits of Possible Hydrothermal Origins in Exhumed Terrain: ESP_027270_1530 ESP_027758_1530 (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
-26.4	55.0	-1.9	-16.6	70.1	69.1
High-Latitude Exposure of North Polar Layered Deposits: ESP_027246_2680 ESP_027034_2680 (Interval in Earth days: 16)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
87.96	353.	-29.	-21.3	65.9	64.0
Crater with Layered Material in THEMIS Image V18397010: ESP_027100_1990 ESP_028643_1990 (Interval in Earth days: 120)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
18.61	10.2	-2.1	-14.8	45.5	54.4
Dune Migration: ESP_027341_2580 ESP_027578_2580 (Interval in Earth days: 19)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
77.65	256.	-4.2	17.63	58.2	58.9
Layered Deposits in West Candor Chasma: ESP_027288_1750 ESP_027644_1750 (Interval in Earth days: 28)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-4.93	282.	-24.	-1.62	58.0	56.1
Narrow Ejecta Flow Lobe of Lonar Crater: ESP_027138_2525 ESP_026914_2525 (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
72.00	38.9	6.93	-9.02	52.9	53.0
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