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 Oriented around Large Obstacle in MOC Image E1002766: ESP_014132_1425 ESP_020791_1425 (Interval in Earth days: 519)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-37.2	178.	-8.6	14.15	38.0	54.6
Contact between Parallel Bedded and Contorted Layers in South Melas Region: ESP_012862_1685 ESP_013930_1685 (Interval in Earth days: 83)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-11.1	286.	1.87	24.04	48.0	34.2
Channels and Noachian Crater Fill: ESP_012709_1445 ESP_013197_1445 (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
-35.2	146.	1.58	-27.4	46.6	42.6
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
Sublimation Scallops: ESP_013873_1225 ESP_014005_1225 (Interval in Earth days: 10)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-57.0	51.1	6.96	-20.3	45.9	48.6
Exposure of Layered Sequence in Terby Crater: ESP_013160_1530 ESP_074031_1530 (Interval in Earth days: 4743)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-26.9	74.0	-8.4	2.702	41.5	52.0
Faulting in South Polar Layered Deposits: ESP_012762_1070 ESP_013171_1070 (Interval in Earth days: 32)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-72.9	146.	10.3	-12.8	58.0	56.3
Rayed Crater: ESP_013955_1020 ESP_013968_1020 (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
-77.8	345.	-6.7	7.228	62.3	61.6
Hill and Adjacent Depression in Polar Layered Deposits: ESP_012815_1080 ESP_013013_1080 (Interval in Earth days: 15)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-71.7	141.	1.59	-20.3	57.3	57.1
Cratered Cones in Galaxias Colles: ESP_012946_2165 ESP_013236_2165 (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
36.17	147.	4.76	26.24	74.0	71.2
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