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

Apron of Material in Columbus Crater: PSP_010492_1510 ESP_045278_1510 (Interval in Earth days: 2710)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-28.8	194.	-5.8	-28.5	69.7	69.7
Fresh Impact Crater on Northern Plains: PSP_010441_2385 PSP_010810_2385 (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
58.19	135.	-7.9	20.93	58.0	61.1
Possible Active Geyser Locale: ESP_011406_0945 ESP_011407_0945 (Interval in Earth days: 0)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-85.4	103.	14.4	-9.73	87.5	89.6
Distributary Channel South of Ascraeus Mons: PSP_010872_1865 ESP_011373_1865 (Interval in Earth days: 39)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
6.197	254.	-2.2	20.12	55.7	55.8
Fresh Unnamed Crater in Northern Hesperia Planum: ESP_011339_1665 ESP_011972_1665 (Interval in Earth days: 49)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-13.1	106.	5.47	-13.2	58.4	56.8
Central Structure of Kirsanov Crater: PSP_010500_1575 ESP_028328_1575 (Interval in Earth days: 1389)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-22.1	334.	-4.6	-20.1	66.0	63.9
Light-Toned Layering along Wallrock in Southwest Melas Chasma: ESP_011504_1700 ESP_016106_1700 (Interval in Earth days: 359)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-9.99	284.	-28.	-15.4	60.3	48.7
Noachis Region Clays: ESP_011592_1595 ESP_011658_1595 (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
-20.3	40.3	4.94	-17.2	58.3	59.6
Ithaca Region Plumes: ESP_011350_0945 ESP_011351_0945 (Interval in Earth days: 0)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-85.2	181.	22.8	-3.81	87.6	89.8
Crater with Extensive Ejecta Deposits: PSP_010611_2210 ESP_027173_2210 (Interval in Earth days: 1290)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
40.51	175.	0.50	-12.9	54.2	44.1
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