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

Double Terraces around Streamlined Hills in South End of Eastern Dao Vallis: ESP_011722_1460 ESP_011577_1460 (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
-33.8	94.0	-5.9	-20.3	60.8	63.6
Gully in Crater Wall: ESP_011877_1410 ESP_012510_1410 (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
-38.8	182.	3.05	-13.9	59.3	51.1
Survey Layering and Faulting in Melas Chasma Layered Deposits: ESP_012361_1685 ESP_012572_1685 (Interval in Earth days: 17)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-11.2	285.	-1.6	-11.8	53.2	52.0
Well-Preserved 15-Kilometer Crater with Gullies and Pitted Ponded Material: ESP_011773_1460 ESP_011839_1460 (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
-33.5	140.	5.89	-13.7	59.1	59.8
Gullies in Southern Hemisphere Crater: ESP_011661_1410 ESP_011938_1410 (Interval in Earth days: 21)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-38.5	319.	-5.4	-27.1	62.8	60.8
Emission of Dark Material in Cerberus Fossae: ESP_011785_1875 ESP_011930_1875 (Interval in Earth days: 12)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
7.411	168.	-8.3	7.691	59.6	58.6
Dual-Outlined Polygon Pattern in Uzboi Vallis in MOC Image R14-02434: ESP_011608_1525 ESP_020878_1525 (Interval in Earth days: 722)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-27.1	324.	-0.8	-20.2	59.9	54.3
Possible Pingos on Floor of Small Craters: ESP_011675_1470 ESP_015987_1470 (Interval in Earth days: 336)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-32.5	296.	-6.2	-21.4	61.0	61.2
Very Well-Preserved 9-Kilometer Crater: ESP_011818_1505 ESP_012029_1505 (Interval in Earth days: 16)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-29.3	351.	6.39	-0.94	57.7	55.8
Debris Apron in Promethei Terra Region: ESP_011919_1400 ESP_011985_1400 (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
-39.7	115.	2.55	-16.4	59.0	59.5
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