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

Curving Channel Near Rahway Valles: PSP_008607_1900 PSP_009042_1900 (Interval in Earth days: 34)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
10.11	175.	-8.0	8.124	48.9	49.1
Western Mawrth Vallis Phyllosilicates: PSP_008245_2045 ESP_016394_2045 (Interval in Earth days: 635)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
24.41	338.	-5.9	-26.1	42.8	42.5
Dune Interaction with Topography in Ganges Chasma: PSP_008536_1725 PSP_009604_1725 (Interval in Earth days: 83)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-7.40	314.	8.72	-5.05	56.9	60.1
Characterize Surface Hazards and Science of Possible MSL Rover Landing Site: PSP_008680_2050 PSP_009260_2050 (Interval in Earth days: 46)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
24.63	340.	-11.	19.88	44.5	43.4
Tyrrhena Terra Crater with Phyllosilicate-Rich Ejecta: PSP_008505_1675 PSP_009085_1675 (Interval in Earth days: 45)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-12.5	83.5	-9.5	14.57	61.2	61.7
Pit in Southeastern Syria Planum: PSP_008749_1660 PSP_009039_1660 (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
-13.9	260.	-4.7	8.94	62.8	62.9
Athabasca Valles: PSP_009280_1905 PSP_009557_1905 (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
10.29	156.	11.7	-18.0	49.3	52.2
Pristine Pancake Crater in Northern Plains: PSP_008649_2130 PSP_009216_2130 (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
32.46	104.	0.54	-19.8	42.1	45.4
Tube-Fed Lava Flow Field: PSP_008433_1755 PSP_009501_1755 (Interval in Earth days: 83)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-4.58	247.	7.65	-15.8	54.7	59.2
Central Peak of Large Well-Preserved Crater: PSP_008860_2165 ESP_053799_2160 (Interval in Earth days: 3502)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
35.93	101.	5.76	-5.62	41.8	42.8
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