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

Channels in North Argyre Planitia : ESP_048095_1405 ESP_049018_1405 (Interval in Earth days: 71)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-39.2	322.	1.87	-16.5	41.6	35.6
Light-Toned Fragments in Linear Depressions : ESP_047965_1720 ESP_048967_1720 (Interval in Earth days: 79)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-7.92	267.	0	13.75	46.4	34.9
Pitted Material in Northern Rim of Lowell Crater: ESP_047477_1295 ESP_048123_1295 (Interval in Earth days: 51)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-50.3	278.	2.20	13.91	54.1	43.6
Well-Preserved 10-Kilometer Impact Crater: ESP_047444_2095 ESP_065193_2095 (Interval in Earth days: 1383)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
29.40	89.0	-5.8	28.88	65.3	67.9
Candidate Landing Site for 2020 Mission in Mclaughlin Crater: ESP_047448_2020 ESP_047158_2020 (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
21.74	337.	24.5	1.923	59.0	58.7
Two-Kilometer Diameter Rayed Crater: ESP_047484_1855 ESP_048987_1855 (Interval in Earth days: 117)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
5.491	79.6	-0.8	16.80	53.6	41.9
Candidate ExoMars Landing Site in Oxia Palus Region: ESP_047435_1985 ESP_064195_1985 (Interval in Earth days: 1306)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
18.05	335.	-0.4	28.08	59.0	55.2
Candidate ExoMars Landing Site in Mawrth Vallis: ESP_047738_2020 ESP_048806_2020 (Interval in Earth days: 83)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
21.94	341.	1.3	-13.0	61.9	57.4
Light-Toned Inverted Terrain in Gorgonum Chaos Basin: ESP_047546_1410 ESP_048469_1410 (Interval in Earth days: 72)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-38.5	190.	20.9	-5.01	47.7	37.5
Dunes on Floor of Infilled Crater: ESP_047471_2015 ESP_056886_2015 (Interval in Earth days: 734)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
21.11	72.4	0	25.01	60.6	60.1
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