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

Bedrock Exposures in Uzboi Vallis and a Crater Rim: ESP_013586_1490 ESP_021722_1490 (Interval in Earth days: 634)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-30.8	323.	-0.0	-28.7	36.4	44.3
Western Half of Very Well-Preserved Gullied Crater: ESP_012807_1505 ESP_012952_1505 (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
-29.4	351.	-5.9	9.919	45.8	42.6
Layering in Argyre Planitia Sinuous Ridge: ESP_012927_1245 ESP_013626_1245 (Interval in Earth days: 55)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-55.1	318.	1.77	-23.3	48.2	46.0
Ares Vallis Wall and Floor Exposures: ESP_013216_1870 ESP_022143_1870 (Interval in Earth days: 695)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
6.694	340.	-2.5	20.39	53.0	48.5
Ejecta Falling Into Earlier Large Crater: ESP_013346_1940 ESP_013768_1940 (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
13.86	29.4	6.71	-7.95	55.5	51.3
Marte Vallis Streamlined Landforms: ESP_014092_1955 ESP_014158_1955 (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
15.46	183.	-6.8	-25.9	48.1	48.6
Differential Erosion of Light-Toned Stratigraphy in Melas Chasma: ESP_013640_1710 ESP_012928_1710 (Interval in Earth days: 56)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-8.93	285.	8.51	-10.3	39.1	48.9
Landslides at the Edge of the South Polar Layered Deposits: ESP_013026_1080 ESP_013224_1080 (Interval in Earth days: 15)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-71.9	143.	-8.2	-28.8	56.2	56.7
Contact between Parallel Bedded and Contorted Layers in South Melas Region: ESP_012862_1685 ESP_013930_1685 (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
-11.1	286.	1.87	24.04	48.0	34.2
Comparative Gully Morphology: ESP_013934_1335 ESP_014000_1335 (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
-46.0	183.	6.35	-11.3	40.0	41.5
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