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

Kasei Valles Flood Grooves: ESP_089015_2055 ESP_089305_2055 (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
25.40	307.	-6.3	17.83	47.4	46.6
Possible New Impact near InSight Lander: ESP_088995_1845 ESP_088929_1845 (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
4.578	135.	0.70	23.70	53.8	52.0
Lava Flows in Elysium Region: ESP_088994_1975 ESP_089139_1975 (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
17.31	162.	-7.9	5.137	49.5	48.8
Antoniadi Crater Fluvial Features: ESP_088945_2015 ESP_089222_2015 (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
21.18	58.3	7.36	-21.9	47.0	50.4
Depression in Nepenthes Mensae: ESP_088956_1935 ESP_089167_1935 (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
13.27	119.	1.73	-7.93	50.0	51.2
Shearing Structures between Viscous Flow Features: ESP_089078_2200 ESP_089355_2200 (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
39.55	24.6	5.18	-17.0	45.8	49.7
Terrain Sample in Young Lava Flows of Elysium Mons: ESP_088941_2005 ESP_089231_2005 (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
20.42	168.	-4.5	19.76	48.1	47.0
Streamlined Feature in Elaver Vallis: ESP_089015_1710 ESP_089160_1710 (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
-9.05	311.	5.33	19.12	60.8	59.7
Elysium Fossae Infills: ESP_088876_2080 ESP_088942_2080 (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
27.49	142.	-0.6	-20.5	46.0	48.0
Gypsum Dunes and Basal Unit Contact: ESP_089030_2605 ESP_088911_2605 (Interval in Earth days: 9)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
80.49	242.	-7.7	7.217	60.3	58.6
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