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

Northern Gale Crater Wall: ESP_022467_1760 ESP_085303_1760 (Interval in Earth days: 4896)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-4.18	137.	2.14	-21.1	39.6	37.2
Channel Head on Pavonis Mons: ESP_022331_1815 ESP_022753_1815 (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
1.616	249.	2.95	-10.7	44.4	40.2
Aonia Terra Dune Field Changes: ESP_022488_1300 ESP_022422_1300 (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
-49.8	293.	-19.	-5.14	41.7	40.7
Possible Rafted Lava Crust in Tartarus Colles: ESP_022320_2050 ESP_023032_2050 (Interval in Earth days: 56)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
24.52	188.	-13.	0.88	61.0	51.0
Eastern Half of Iazu Crater: ESP_022670_1775 ESP_023092_1775 (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
-2.69	354.	8.00	-9.77	37.6	34.9
Layered Material in Crater Seen in CTX Image: ESP_022425_1925 ESP_058609_1925 (Interval in Earth days: 2820)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
12.54	202.	-5.4	8.895	50.6	37.5
Light-Toned Material along Valley near Coprates Catena: ESP_022527_1645 ESP_023028_1645 (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
-15.5	300.	1.62	23.37	34.6	29.7
Stratigraphy of Kasimov Crater Fill: ESP_022473_1550 ESP_023119_1550 (Interval in Earth days: 50)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-24.9	337.	-8.5	27.5	34.5	30.2
Mawrth Vallis Strata with Interesting Geometry Exposed in Small Crater: ESP_022354_2035 ESP_022288_2035 (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
23.41	340.	-8.4	11.78	59.5	59.1
Landslides in Valles Marineris: ESP_022632_1670 ESP_031124_1670 (Interval in Earth days: 661)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-12.6	313.	4.73	24.39	34.2	36.3
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