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

Valleys and East Rim of Huygens Crater : ESP_043120_1670 ESP_044254_1670 (Interval in Earth days: 88)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-12.8	59.4	6.87	28.07	53.9	57.9
Terraced and Rounded Crater Rim in West Utopia Planitia: ESP_043119_2185 ESP_043409_2185 (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
38.38	81.7	-9.4	14.08	41.3	38.7
Distal Rampart of Toconao Crater: ESP_043125_1590 ESP_043837_1590 (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
-20.9	284.	-5.6	19.06	60.0	63.2
Landslides in Trough South of Ius Chasma : ESP_043376_1710 ESP_043943_1710 (Interval in Earth days: 44)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-8.90	270.	-2.0	9.783	53.9	55.9
Holden Crater Dune Topography : ESP_043229_1540 ESP_043374_1540 (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
-25.7	326.	-7.9	7.843	64.3	64.6
Infilled Crater with Overlying Secondary Craters in Arcadia Planitia : ESP_043260_2265 ESP_043972_2265 (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
46.21	189.	0.67	17.69	42.2	39.1
InSight Mission Candidate Landing Site : ESP_043183_1845 ESP_043671_1845 (Interval in Earth days: 38)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
4.459	135.	21.3	-10.5	43.7	48.4
Crater with Intersecting Faults in Tempe Terra : ESP_043283_2220 ESP_043560_2220 (Interval in Earth days: 21)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
41.94	282.	-0.8	-19.2	40.9	41.9
Clusters of Small Mesas in Northern Arabia Terra : ESP_043201_2160 ESP_043834_2160 (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
35.65	1.82	5.82	-4.54	39.4	39.8
Hills in Coprates Chasma : ESP_043177_1655 ESP_042887_1655 (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
-14.1	301.	23.0	-6.26	54.1	53.4
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