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

Gullies in Southern Hemisphere Crater: ESP_013894_1410 ESP_022676_1410 (Interval in Earth days: 684)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-38.8	195.	-5.6	5.235	37.6	35.2
Wrinkle Ridge in Lunae Palus: ESP_014022_1950 ESP_014167_1950 (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
14.94	294.	-7.9	7.828	48.7	45.9
Small Rayed Crater in Syrtis Major Planum: ESP_012791_1910 ESP_012857_1910 (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
10.67	62.2	4.22	-17.8	58.5	59.5
Light-Toned Outcrops Near Crater Rim in Arabia Terra: ESP_014165_1985 ESP_022314_1985 (Interval in Earth days: 635)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
18.07	349.	2.28	28.31	48.4	53.8
Pit Crater Chain Southwest of Arsia Mons: ESP_014077_1660 ESP_058186_1660 (Interval in Earth days: 3437)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-13.9	236.	-3.3	8.798	34.6	29.8
Layered Material Exposed on Crater Floor: ESP_013017_2150 ESP_013518_2150 (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
34.69	8.85	6.51	22.48	72.6	67.8
Recent 10 Kilometer Diameter Crater in Ares Vallis: ESP_013335_1975 ESP_020772_1975 (Interval in Earth days: 580)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
17.40	329.	1.40	17.37	58.3	58.8
Contact between Wallrock and Light-Toned Deposits in Hebes Chasma: ESP_013772_1795 ESP_022910_1795 (Interval in Earth days: 712)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-0.51	283.	-21.	-5.7	43.5	37.1
Crater Wall with Gullies at Multiple Elevations in MOC Image E1101445: ESP_013236_1410 ESP_013948_1410 (Interval in Earth days: 56)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-38.7	159.	5.50	16.26	39.9	36.0
Gullies in Southern Hemisphere Crater: ESP_013749_1410 ESP_013894_1410 (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
-38.8	195.	-16.	-5.65	38.5	37.6
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