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

Ridges in Nilosyrtis Mensae: ESP_088312_2135 ESP_088246_2135 (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
33.36	60.4	2.84	21.93	43.1	41.2
Pits in North Polar Layered Deposits: ESP_088394_2650 ESP_088367_2650 (Interval in Earth days: 3)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
84.81	318.	-7.7	6.46	60.4	59.8
Candidate ExoMars Landing Site in Oxia Planum: ESP_088078_2000 ESP_088012_2000 (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
19.56	334.	-28.	-7.03	48.3	46.2
Patterned Ground in Elysium Planitia: ESP_088335_1845 ESP_088546_1845 (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
4.634	156.	3.81	-11.4	52.6	54.2
Group of Channels along Old Crater Wall: ESP_088288_2130 ESP_088499_2130 (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
32.59	357.	-6.7	-18.5	44.0	45.7
Alluvial Fans in Kasei Valles: ESP_088264_2035 ESP_088475_2035 (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
23.06	294.	-13.	-26.2	46.4	48.0
Channels Going Into Echus Chasma: ESP_087724_1850 ESP_088792_1850 (Interval in Earth days: 84)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
4.863	278.	5.37	-4.74	50.2	53.9
Small Delta or Fan: ESP_087771_2065 ESP_087837_2065 (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
26.42	74.2	-7.4	-23.7	43.8	45.4
Crater in Arabia Terra: ESP_087747_2200 ESP_087681_2200 (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
39.57	7.75	-7.8	6.691	43.3	42.0
4-Kilometer Diameter Rayed Crater: ESP_087802_1915 ESP_088448_1915 (Interval in Earth days: 51)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
11.13	309.	0.34	12.37	48.0	49.1
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