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

Inverted Channel in Noachis Terra: ESP_085083_1605 ESP_085149_1605 (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
-19.2	22.4	9.36	-12.4	34.7	36.8
Small Delta or Fan: ESP_085070_2120 ESP_085136_2120 (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
31.78	11.8	-1.3	-18.2	54.2	54.4
Glacial Ridges in Arsia Mons Fan-Shaped Deposit: ESP_085207_1745 ESP_085352_1745 (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
-5.44	236.	2.19	25.29	35.1	33.5
Landforms in Utopia Planitia: ESP_085146_2110 ESP_085423_2110 (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
30.77	96.2	7.62	-4.77	52.0	49.5
Exhumed Fracture Network: ESP_085266_2080 ESP_085899_2080 (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
27.54	62.5	-9.7	6.656	49.4	42.9
Streamlined Form and Hill in Marte Vallis: ESP_085156_1980 ESP_085433_1980 (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
17.73	185.	7.29	-6.33	43.5	42.2
Lighter-Toned Deposits in Young Crater: ESP_085271_1870 ESP_085337_1870 (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
7.156	287.	-1.6	-20.0	38.2	39.4
Crater: ESP_085139_2030 ESP_085073_2030 (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
22.64	289.	-7.8	11.69	47.6	47.1
Channels near Huygens Crater: ESP_085240_1615 ESP_085306_1615 (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
-18.1	57.5	-4.1	-22.8	36.5	38.5
Mesa Stratigraphy at Terby Crater: ESP_085068_1525 ESP_085213_1525 (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
-27.1	74.1	-4.4	13.86	37.8	37.8
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