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

Debris Apron in Promethei Terra Region: ESP_011919_1400 ESP_011985_1400 (Interval in Earth days: 5)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-39.7	115.	2.55	-16.4	59.0	59.5
Possible MSL Rover Mawrth 2 Landing Site: ESP_012517_2045 ESP_012227_2045 (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
24.02	341.	4.34	-22.2	66.8	68.2
Oudemans Crater Central Uplift: ESP_011676_1700 ESP_028449_1700 (Interval in Earth days: 1307)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-9.84	267.	-22.	7.568	59.1	56.2
Central Structures of Crater North of Hellas Basin: ESP_012461_1515 ESP_012883_1515 (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
-28.2	76.8	4.41	-11.7	49.8	45.3
Layered Sinuous Ridge in the Argyre Planitia: ESP_012281_1240 ESP_012360_1240 (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
-55.7	316.	-6.2	17.71	58.6	55.5
Well-Preserved 6-Kilometer Diameter Impact Crater with Gullies: ESP_012300_1440 ESP_020871_1440 (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
-35.7	154.	-7.5	9.261	53.3	53.5
East Wall of Ritchey Crater: ESP_011780_1515 ESP_011846_1515 (Interval in Earth days: 5)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-28.4	309.	-4.3	-23.6	58.8	59.7
Survey Layering and Faulting in Melas Chasma Layered Deposits: ESP_012361_1685 ESP_012572_1685 (Interval in Earth days: 17)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-11.2	285.	-1.6	-11.8	53.2	52.0
Gullies: ESP_012446_1435 ESP_066089_1435 (Interval in Earth days: 4180)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-36.2	127.	2.45	-12.6	50.5	43.6
Well-Preserved 15-Kilometer Crater with Gullies and Pitted Ponded Material: ESP_011773_1460 ESP_011839_1460 (Interval in Earth days: 5)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-33.5	140.	5.89	-13.7	59.1	59.8
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