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

Future Mars Landing Site in Acidalia Mensa: ESP_018161_2270 ESP_018227_2270 (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
46.68	331.	-1.6	-15.5	43.8	45.4
Future Mars Landing Site in Antoniadi Crater: ESP_018105_2045 ESP_018250_2045 (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
24.05	63.0	-0.2	13.32	44.2	43.5
Ridges and Flow-Like Forms: ESP_017734_2075 ESP_071880_2075 (Interval in Earth days: 4219)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
27.32	111.	-1.2	16.1	42.7	47.9
Layered Deposits in Crater in Western Arabia Terra: ESP_017936_1890 ESP_060489_1890 (Interval in Earth days: 3315)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
8.810	-0.9	0.22	-9.82	49.5	41.2
Amazonis Planitia: ESP_017836_1970 ESP_017981_1970 (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
16.64	209.	-11.	2.253	46.8	46.0
Very Well-Preserved 10-Kilometer Diameter Impact Crater: ESP_017901_2375 ESP_017980_2375 (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
57.35	225.	8.89	25.25	44.9	43.6
Nozzle for Scarp-Fed Sands: ESP_017871_2745 ESP_026613_2745 (Interval in Earth days: 681)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
85.24	183.	2.61	-7.04	65.2	66.3
Valley-Crater Intersection with Exposed Layers: ESP_018055_2120 ESP_018899_2120 (Interval in Earth days: 66)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
31.60	346.	3.16	-20.2	42.5	48.6
Central Uplift of Impact Crater in Tyrrhena Terra: ESP_017748_1665 ESP_026108_1665 (Interval in Earth days: 651)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-13.3	93.8	8.34	24.74	61.6	57.7
Well-Preserved Oblique Impact Crater in Acidalia Planitia: ESP_017792_2285 ESP_018425_2285 (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
47.90	323.	9.53	-4.67	42.0	45.6
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