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

Light-Toned Outcrops along Ius Region Wallrock: ESP_012849_1705 ESP_013126_1705 (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
-9.22	281.	-3.9	-28.8	49.2	48.0
Very Fresh Small Crater in Hesperia Planum: ESP_013976_1670 ESP_020279_1670 (Interval in Earth days: 491)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-12.8	113.	-1.1	19.13	35.3	54.4
Exposures of Layered Bedrock Northwest of Hellas Basin: ESP_012620_1540 ESP_013688_1540 (Interval in Earth days: 84)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-25.5	55.4	3.80	26.88	47.8	33.4
Pit Crater: ESP_013167_1785 ESP_013589_1785 (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
-1.32	239.	-7.4	-22.9	49.4	45.4
Phyllosilicate and Possible Chlorite Prehnite Northwest of Hellas Region: ESP_012765_1535 ESP_013477_1535 (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
-26.2	56.4	7.51	22.87	45.6	35.6
Layered Crater Fill Material: ESP_014017_2085 ESP_022021_2085 (Interval in Earth days: 624)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
27.99	68.5	0.69	16.01	57.5	64.7
Well-Preserved 8 Kilometer Diameter Crater: ESP_013650_1230 ESP_013927_1230 (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
-56.4	20.2	1.13	-19.3	45.0	47.6
Martian Volcanic Vent with Elevated Rim: ESP_013008_1825 ESP_020801_1825 (Interval in Earth days: 607)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
2.452	259.	-3.3	21.93	52.7	53.7
Gullies in Crater North of Gorgonum Chaos: ESP_013169_1450 ESP_013314_1450 (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
-34.7	189.	-4.4	7.868	41.0	38.5
Gullies Previously Identified in MOC Image: ESP_013849_1080 ESP_013981_1080 (Interval in Earth days: 10)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-71.9	354.	-7.6	-22.1	56.8	59.0
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