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

South Polar Layered Deposits Exposed in Ultimum Chasma: ESP_013619_0990 ESP_013672_0990 (Interval in Earth days: 4)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-80.8	151.	18.0	4.365	60.2	61.5
Cratered Cones in Olympus Mons Aureole: ESP_013853_2130 ESP_022002_2130 (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
32.87	224.	6.20	28.86	63.2	67.7
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
Raga Crater: ESP_014011_1315 ESP_014288_1315 (Interval in Earth days: 21)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-48.1	242.	1.60	-18.1	41.9	45.6
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
Interesting Contrasts in Gully Morphology: ESP_014104_1360 ESP_021686_1360 (Interval in Earth days: 591)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-43.8	222.	3.50	25.74	40.1	42.0
Layers in Spallanzani Crater: ESP_013041_1215 ESP_013120_1215 (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
-58.1	86.8	5.04	26.10	48.1	45.8
Layers on Columbus Crater Wall: ESP_014105_1495 ESP_014382_1495 (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
-30.0	193.	-0.6	-23.8	34.9	38.0
Possible Arete in North and South Debris Flows: ESP_013528_1380 ESP_013673_1380 (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
-41.6	108.	-4.1	9.479	39.1	37.6
Alcove in East Candor Chasma Layered Deposits: ESP_012809_1725 ESP_013310_1725 (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
-7.44	293.	-2.1	22.37	50.2	42.7
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