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

Planned ExoMars Landing Site in Oxia Planum: ESP_089014_1995 ESP_089080_1995 (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
19.15	335.	2.69	-18.5	48.1	50.1
Terrain Features around Crater in Arabia Terra: ESP_088875_2215 ESP_088585_2215 (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
41.06	167.	2.85	-12.9	44.9	45.1
Possible Vent on Volcanic Terrain near Lineated Valley Floor Material: ESP_089020_2110 ESP_089086_2110 (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
30.47	170.	-7.4	-24.8	46.8	48.8
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
Dune Survey: ESP_088879_2170 ESP_089301_2170 (Interval in Earth days: 33)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
36.67	58.2	5.83	-8.82	44.5	48.3
Kasei Valles Remnant Fan: ESP_088910_2040 ESP_089411_2040 (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
23.51	294.	-5.2	12.24	47.3	47.9
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
Channels near Osuga Valles: ESP_089041_1635 ESP_089463_1635 (Interval in Earth days: 33)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-16.2	319.	29.7	15.43	63.4	63.3
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
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
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