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

Wrinkle Ridge and Channel Intersection Along Huygens Crater Rim: ESP_064034_1610 ESP_063744_1610 (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
-18.6	56.7	22.8	-4.84	58.9	62.2
Erebus Montes: ESP_064174_2195 ESP_064464_2195 (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
39.21	189.	-5.3	17.58	63.2	65.6
Jezero Crater: ESP_064165_1985 ESP_072422_1985 (Interval in Earth days: 643)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
18.87	77.3	0.68	-25.2	57.5	55.9
Candidate ExoMars Landing Site in Oxia Planum: ESP_063839_1980 ESP_064261_1980 (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
17.84	336.	21.8	7.745	52.6	57.7
Intra-Flow Margins and Flow Edge Margins in Deuteronilus Mensae: ESP_064022_2275 ESP_064246_2275 (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
47.17	18.0	-4.5	26.36	63.6	64.6
Terrain Sample: ESP_064073_1570 ESP_063928_1570 (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
-22.7	73.7	8.23	-6.39	61.1	63.0
Dichotomy Boundary East of Gale Crater: ESP_064176_1745 ESP_064532_1745 (Interval in Earth days: 27)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-5.27	139.	7.06	17.69	56.8	55.9
Crater in Arabia Terra: ESP_063838_2245 ESP_063416_2245 (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
44.33	2.43	-6.6	7.772	59.9	52.6
Deposits in Ganges Chasma: ESP_064051_1715 ESP_064473_1715 (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
-8.61	312.	7.21	-6.31	57.4	58
Crater Cut by Wrinkle Ridge: ESP_064059_1680 ESP_063914_1680 (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
-11.6	94.6	7.89	-7.36	58.0	59.4
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