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

Ridges and Mounds Near Hecates Tholus: PSP_007672_2155 PSP_007883_2155 (Interval in Earth days: 16)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
34.92	142.	6.64	-7.98	40.8	42.0
Wall Layers of Tooting Crater: PSP_007907_2035 ESP_019115_2035 (Interval in Earth days: 873)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
23.18	208.	-2.3	5.434	41.6	48.0
Lobate Debris Aprons with Ridge-Like Structures: PSP_007693_2300 PSP_008550_2300 (Interval in Earth days: 67)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
49.57	286.	6.42	-7.47	45.2	44.0
Reull Vallis: PSP_007819_1390 PSP_009612_1390 (Interval in Earth days: 140)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-40.6	99.6	-6.4	7.67	74.7	81.0
Possible Submarine Fan in Eastern Portion of Small Melas Chasma Basin: PSP_007377_1700 PSP_008379_1700 (Interval in Earth days: 78)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-9.82	283.	5.56	-6.99	48.4	58.5
Hematite in West Candor Chasma: PSP_007601_1745 PSP_010449_1745 (Interval in Earth days: 222)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-5.55	286.	7.08	-20.0	48.5	59.7
Layering in East Coprates Chasma Wall: PSP_007864_1655 PSP_007508_1655 (Interval in Earth days: 28)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-14.1	307.	-8.1	4.599	57.2	52.4
Light-Toned Rock Exposures: PSP_007101_1730 ESP_019311_1730 (Interval in Earth days: 952)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-6.99	260.	-7.9	3.361	44.7	56.7
Well-Peserved Large Crater with Central Peak and Pit: PSP_007366_1360 ESP_024732_1360 (Interval in Earth days: 1353)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-43.4	229.	2.46	-27.4	70.5	67.3
Finely-Layered Deposits in Henry Crater: PSP_008072_1905 PSP_009153_1905 (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
10.17	24.0	0.27	15.57	45.7	48.8
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