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

Shallow Channels Entering Collapse Terrain near Orson Welles Crater: ESP_066979_1780 ESP_073877_1780 (Interval in Earth days: 537)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-1.90	313.	-5.2	10.09	42.0	55.8
Charitum Montes: ESP_067138_1275 ESP_066030_1275 (Interval in Earth days: 86)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-52.0	302.	-1.7	-24.1	48.8	48.4
Large New Impact Crater: ESP_066951_2150 ESP_084385_2150 (Interval in Earth days: 1358)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
34.67	352.	-1.0	24.80	64.3	64.4
Gully Monitoring and Topography: ESP_067155_1415 ESP_074132_1415 (Interval in Earth days: 543)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-38.3	195.	5.52	26.12	41.5	49.6
Flow Surface with Cones in Tartarus Colles: ESP_067050_2070 ESP_067591_2070 (Interval in Earth days: 42)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
26.78	172.	-4.5	-16.3	57.5	52.4
Crater Uplift and Ejecta in Tyrrhena Terra: ESP_067054_1760 ESP_067595_1760 (Interval in Earth days: 42)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-3.93	67.0	3.09	-11.7	40.2	40.2
Vent and Channel East of Olympus Mons: ESP_067061_1990 ESP_067404_1990 (Interval in Earth days: 27)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
18.89	232.	5.92	17.21	51.5	47.2
Exposure of South Polar Layered Deposits: ESP_067292_0880 ESP_058563_0880 (Interval in Earth days: 680)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-88.0	192.	18.6	27.12	77.8	79.2
Gullies Emanating from Lobate Flow: ESP_067296_1315 ESP_058856_1315 (Interval in Earth days: 658)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-48.0	309.	9.71	-12.4	47.6	50.0
Gullies in Crater in Terra Cimmeria: ESP_067275_1335 ESP_074041_1335 (Interval in Earth days: 527)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-46.1	163.	-4.3	6.951	47.2	54.2
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