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

Contact between Fluvial Units in Aeolis Dorsa : ESP_044132_1750 ESP_053138_1750 (Interval in Earth days: 702)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-4.80	151.	-1.0	19.38	54.3	53.2
Collapsed Channel Margin : ESP_044073_1655 ESP_044218_1655 (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
-14.4	322.	4.97	24.30	60.2	59.2
Channels on Alba Patera : ESP_043983_2275 ESP_044273_2275 (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
47.03	251.	1.43	25.12	40.6	38.5
Landslide in Southern Mid-Latitude Crater : ESP_043963_1550 ESP_044741_1550 (Interval in Earth days: 60)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-24.4	87.4	-2.0	20.53	67.4	66.1
Dark Ridges over Light-Toned Substrate in Eridania Region : ESP_043920_1505 ESP_043854_1505 (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
-29.1	181.	1.96	21.17	70.4	69.1
Pitted Cones in Melas Chasma : ESP_043995_1685 ESP_044971_1685 (Interval in Earth days: 76)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-11.4	290.	18.7	-13.7	57.1	58.7
Well-Preserved 5-Kilometer Impact Crater North of Gale Crater : ESP_044106_1800 ESP_053679_1800 (Interval in Earth days: 746)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
0.147	139.	5.54	20.38	50.9	50.5
Candidate Landing Site for 2020 Mission in Gusev Crater : ESP_043907_1650 ESP_043841_1650 (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
-14.6	175.	-8.9	12.57	60.7	59.2
Candidate ExoMars Landing Site in Oxia Palus Region : ESP_044178_1985 ESP_061136_1985 (Interval in Earth days: 1322)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
18.46	335.	-25.	-3.40	44.9	41.7
Possible Layered Ejecta Deposits from Bakhuysen Crater : ESP_043913_1590 ESP_044190_1590 (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
-20.8	11.6	1.25	-20.0	64.4	66.3
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