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

Kasei Valles Lava: ESP_088884_1965 ESP_089174_1965 (Interval in Earth days: 22)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
16.49	285.	-4.6	20.18	49.2	47.9
Kasei Valles Remnant Fan: ESP_089055_2040 ESP_089200_2040 (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
23.60	294.	5.44	17.55	46.9	46.4
Crater Deposits: ESP_088867_2175 ESP_079927_2175 (Interval in Earth days: 696)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
37.05	28.6	-18.	-8.45	46.7	46.2
Depression in Nepenthes Mensae: ESP_088956_1935 ESP_089167_1935 (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
13.27	119.	1.73	-7.93	50.0	51.2
Features around Crater in Arabia Terra: ESP_089012_2200 ESP_088933_2200 (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
39.85	26.4	5.94	-19.7	45.3	47.2
Ismenius Cavus Channel and Fan-Looking Feature: ESP_089052_2140 ESP_089197_2140 (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
33.89	16.6	-6.6	4.435	46.6	46.5
Fine Layer Deformation in Lobate Debris Apron: ESP_088932_2270 ESP_089275_2270 (Interval in Earth days: 27)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
46.44	49.8	2.69	-29.9	45.8	51.3
Dune Interaction with Residual Polar Ice: ESP_088917_2590 ESP_088970_2590 (Interval in Earth days: 4)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
78.89	82.0	8.16	-5.86	57.7	58.9
Kasei Valles Remnant Fan: ESP_088910_2040 ESP_089411_2040 (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
23.51	294.	-5.2	12.24	47.3	47.9
The Persistence of Dust: ESP_087831_1860 ESP_088042_1860 (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
5.837	237.	10.3	-7.81	49.9	52.0
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