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

Planned ExoMars Landing Site in Oxia Planum: ESP_088157_1975 ESP_088447_1975 (Interval in Earth days: 23)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
17.33	336.	-8.6	8.83	47.5	46.8
Jezero Crater: ESP_088061_1985 ESP_088272_1985 (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
18.47	77.3	-10.	-24.7	46.9	48.7
Sedimentary Deposits in Chryse Planitia: ESP_088092_2050 ESP_088527_2050 (Interval in Earth days: 34)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
24.88	309.	-6.8	17.17	44.9	43.9
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
Dune Monitoring in Northern Mid-Latitude Crater: ESP_088230_2400 ESP_088454_2400 (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
59.81	135.	-4.2	14.96	47.5	46.2
Athabasca Valles: ESP_088177_1855 ESP_088467_1855 (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
5.328	151.	-4.9	13.93	52.5	51.8
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
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
Terrain in Crater in Tempe Terra: ESP_088260_2150 ESP_088827_2150 (Interval in Earth days: 44)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
34.74	40.1	2.83	-11.4	42.9	45.9
Grooves and Undercutting in Columbia Valles: ESP_088171_1705 ESP_088316_1705 (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
-9.60	316.	-5.9	3.691	61.1	60.9
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