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 Crater Southeast of Hellas Planitia : ESP_057044_1325 ESP_057189_1325 (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
-47.0	90.9	3.72	23.28	42.1	38.9
Cratered Features in Olympus Mons Aureole : ESP_057052_2145 ESP_057131_2145 (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
34.27	225.	-29.	3.024	72.2	70.0
Crater-Related Pitted Materials Adjacent to 6-Kilometer Diameter Crater : ESP_056965_1545 ESP_056899_1545 (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
-25.3	84.2	1.56	18.61	40.5	40.0
Central Pit of Asimov Crater : ESP_057034_1330 ESP_057245_1330 (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
-46.8	4.83	-5.7	3.292	42.8	39.8
Transverse Ridges on Euripus Mons : ESP_057083_1350 ESP_057426_1350 (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
-44.5	104.	15.7	1.51	39.9	37.7
Light-Toned Layered Deposits in Argentea Planum : ESP_056733_1060 ESP_056746_1060 (Interval in Earth days: 1)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-74.0	306.	8.34	25.36	59.0	57.6
Well-Exposed Breccia in Huygens Crater : ESP_056623_1650 ESP_058008_1650 (Interval in Earth days: 108)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-14.9	58.1	3.89	-11.3	46.0	32.2
West Syria Planum : ESP_056550_1680 ESP_058225_1680 (Interval in Earth days: 131)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-11.8	251.	-7.9	6.069	48.2	30.2
Crater Gullies and Fractures in Acidalia Planitia: ESP_054832_2185 ESP_055320_2185 (Interval in Earth days: 38)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
37.96	338.	0	-16.8	52.1	60.1
Spiders with Big Spring Fans : ESP_055947_0970 ESP_055948_0970 (Interval in Earth days: 0)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-82.6	167.	9.03	-28.5	77.0	80.4
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