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

Arsia Mons Reticulate Bedform Change Detection : ESP_029215_1740 ESP_029360_1740 (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
-6.16	235.	5.36	19.71	54.1	52.6
Fault-Bounded Depression in Lucus Planum : ESP_029217_1795 ESP_029362_1795 (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
-0.45	180.	-8.9	5.466	55.3	54.2
Multiple Geologic and Geomorphic Units in Contact : ESP_029151_1695 ESP_029296_1695 (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
-10.4	182.	4.21	20.99	54.6	52.7
Collapse Structures South of Orson Welles Crater : ESP_028988_1775 ESP_028355_1775 (Interval in Earth days: 50)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-2.69	313.	-10.	6.729	55.4	54.0
Mounds and Small Ridges along Wrinkle Ridge on Huygens Crater Floor : ESP_029103_1675 ESP_029037_1675 (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
-12.5	54.0	-1.6	21.19	55.5	53.9
Cerberus Fossae : ESP_028954_1900 ESP_029376_1900 (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
9.810	158.	6.13	-8.14	54.0	57.1
Kasei Valles Lava Surface : ESP_029147_2015 ESP_055335_2015 (Interval in Earth days: 2041)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
21.36	287.	5.39	17.42	57.5	52.4
Light-Toned Fractures in Uzboi Vallis: ESP_029014_1525 ESP_038495_1525 (Interval in Earth days: 739)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-27.3	324.	8.88	0.117	58.8	54.9
Western Portion of Central Structure in Mazamba Crater : ESP_029134_1520 ESP_029846_1520 (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
-27.5	290.	-11.	0.335	59.2	50.7
20-Kilometer Crater in Meridiani Planum Exposing Layers : ESP_029092_1770 ESP_029804_1770 (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
-2.96	353.	-8.5	3.934	55.2	53.2
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