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 Lava: ESP_088884_1965 ESP_089174_1965 (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
16.49	285.	-4.6	20.18	49.2	47.9
Eruptive Center in Arcadia Planitia: ESP_089164_2265 ESP_089230_2265 (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
46.26	195.	8.34	-6.10	46.8	48.6
Deposits in Ganges Chasma: ESP_088883_1725 ESP_089094_1725 (Interval in Earth days: 16)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-7.29	314.	5.58	-5.54	59.8	60.4
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
Ismenius Cavus Channel and Fan-Looking Feature: ESP_089052_2140 ESP_089197_2140 (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
33.89	16.6	-6.6	4.435	46.6	46.5
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 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
Flow Entering Fretted Terrain Valley: ESP_089025_2170 ESP_089091_2170 (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
36.42	31.9	6.73	-11.0	45.2	47.2
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
Valleys in Terra Cimmeria: ESP_088890_1800 ESP_089391_1800 (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
0.027	123.	-6.7	12.85	56.6	55.2
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