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

Fresh Shallow Valleys: ESP_031789_1380 ESP_049881_1380 (Interval in Earth days: 1410)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-41.5	162.	5.59	-8.59	38.0	42.9
Rough Terrain and Albedo Boundary on South Polar Layered Deposits: ESP_032059_0925 ESP_032216_0925 (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
-87.4	82.3	1.27	8.289	77.8	78.9
Portion of Mound in Gale Crater: ESP_031803_1750 ESP_031948_1750 (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
-4.99	137.	-13.	6.521	35.5	33.1
Youthful Crater Superimposed on Volcanic Plain: ESP_031974_1855 ESP_039873_1855 (Interval in Earth days: 616)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
5.304	146.	4.53	16.53	37.3	48.5
Karzok Crater West Rim: ESP_031760_1985 ESP_032261_1985 (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
18.37	228.	-8.3	24.63	48.4	40.6
Light-Toned Layered Material Exposed in Coprates Chasma Scarp Wall: ESP_031942_1645 ESP_032575_1645 (Interval in Earth days: 49)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-15.2	303.	-3.3	-25.0	32.1	37.0
Constriction in Kasei Valles: ESP_031837_1990 ESP_032193_1990 (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
18.69	286.	-8.5	10.33	47.7	42.4
South Polar Layered Deposit Spiral Troughs during Katabatic Wind Season: ESP_031918_0945 ESP_031957_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	289.	-8.2	4.508	73.5	72.9
Exposure of South Polar Layered Deposits: ESP_031788_0960 ESP_031959_0960 (Interval in Earth days: 13)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-84.1	225.	-7.9	6.554	70.1	71.5
Pits in South Polar Layered Deposits: ESP_032000_0925 ESP_040280_0925 (Interval in Earth days: 646)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-87.2	236.	0.37	14.64	76.2	67.4
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