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

Northeast Melas Chasma Dune Fields and Wall Rock : ESP_028857_1700 ESP_028923_1700 (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
-10.0	290.	-4.8	-26.4	56.1	57.7
Layering in Graben Wall : ESP_028793_2265 ESP_072482_2265 (Interval in Earth days: 3404)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
45.91	229.	0	24.14	61.8	55.9
Chevrons on Lava Surface in Marte Vallis : ESP_028716_1880 ESP_053704_1875 (Interval in Earth days: 1947)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
7.810	177.	0	12.89	53.4	47.2
Fretted Terrain : ESP_028613_1375 ESP_028758_1375 (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
-42.0	116.	-5.6	5.302	70.5	68.1
Erosional Morphologies in Lower Shalbatana Vallis : ESP_028869_1890 ESP_029291_1890 (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
8.738	319.	6.05	-5.96	53.6	56.4
Fresh Small Rayed Crater : ESP_028629_1660 ESP_029051_1660 (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
-13.9	34.4	8.94	-9.1	56.9	56.5
Layering in Crater in Mawrth Vallis : ESP_028855_2045 ESP_020297_2045 (Interval in Earth days: 666)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
24.23	341.	-13.	-25.2	57.0	61.1
Proposed Future Landing Site in Arda Valles : ESP_028882_1600 ESP_028948_1600 (Interval in Earth days: 6)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-19.6	327.	7.83	-15.0	57.5	58.8
Central Structure of a Large Impact Crater : ESP_028829_1450 ESP_029251_1450 (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
-34.8	336.	4.72	-6.35	63.9	59.9
Flow Boundary in Tharsis Region East of Pavonis Mons : ESP_028621_1775 ESP_034291_1775 (Interval in Earth days: 442)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-2.48	251.	3.73	-19.1	54.2	50.4
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