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

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
Kasei Valles Alluvial Fans and Terraced Scarps: ESP_089042_2025 ESP_088765_2025 (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
22.38	291.	-8.7	22.53	48.3	44.7
Chryse Chaos: ESP_089120_1850 ESP_089265_1850 (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
5.033	322.	3.73	17.70	53.5	52.6
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
Eroded Debris Covered Glaciers in Protonilus Mensae: ESP_088866_2220 ESP_089156_2220 (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
41.89	52.0	7.85	24.36	44.5	44.6
Alluvial Fan and Light-Toned Deposits in Coprates Catena Trough: ESP_089187_1655 ESP_089121_1655 (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
-14.1	297.	-21.	2.298	65.3	63.9
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
The Persistence of Dust: ESP_087831_1860 ESP_088042_1860 (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
5.837	237.	10.3	-7.81	49.9	52.0
Stacked!: ESP_089198_1885 ESP_089343_1885 (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
8.276	352.	4.96	19.07	52.2	51.2
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