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

Dissected Wrinkle Ridge Surrounded by Viscous Flows in Elysium Planitia: ESP_025776_1875 ESP_026132_1875 (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
7.509	157.	-3.0	6.875	45.6	46.7
Hebrus Valles: ESP_025777_1990 ESP_027254_1990 (Interval in Earth days: 115)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
18.14	127.	9.74	-19.1	40.7	47.4
A Youthful Crater in the Cydonia Colles Region: ESP_025716_2200 ESP_027417_2200 (Interval in Earth days: 132)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
39.64	350.	4.65	24.57	39.9	42.0
An Impact Crater on Upper Rim Valles Marineris: ESP_025705_1675 ESP_025560_1675 (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
-12.3	298.	-0.6	-20.3	55.9	55.8
Fresh Crater on Northern Plains: ESP_025116_2320 ESP_025195_2320 (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
51.71	172.	-20.	0.151	48.6	46.4
Peridier Crater Dune Changes: ESP_025383_2055 ESP_025528_2055 (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
25.09	83.5	2.17	17.79	38.8	37.8
Kipuka in Amazonis Planitia: ESP_025181_1950 ESP_025669_1950 (Interval in Earth days: 38)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
14.70	200.	-3.0	-27.5	39.6	44.4
Strange Features in Hellas Basin: ESP_025160_1445 ESP_042395_1445 (Interval in Earth days: 1343)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-35.2	58.5	10.2	-13.7	65.2	61.7
Light-Toned Layering along Plains South of Melas Region: ESP_025310_1690 ESP_025455_1690 (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
-10.8	281.	-9.0	9.973	51.7	52.0
Small Mounds in Chryse Planitia: ESP_025071_1995 ESP_025137_1995 (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
19.39	322.	-4.0	-23.5	38.6	40.7
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