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

Light-Toned Rocks inside a Crater: ESP_017292_1680 ESP_025375_1680 (Interval in Earth days: 630)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-11.8	304.	-4.3	26.62	59.6	50.6
Layered Mesa in Candor Chasma: ESP_017266_1715 ESP_017411_1715 (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
-8.17	294.	-9.6	5.488	57.5	57.2
Layered Terrain in Zephyria Planum: ESP_017126_1755 ESP_018115_1755 (Interval in Earth days: 78)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-4.51	155.	4.60	-17.2	53.5	58.1
Diverse Lava Morphologies in Elysium Planitia: ESP_017271_1870 ESP_017416_1870 (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
6.820	155.	-6.6	7.712	48.9	48.5
Crater and Ejecta and Context for MOC Image SP2-47903: ESP_017046_2080 ESP_017824_2080 (Interval in Earth days: 61)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
27.58	175.	4.05	-7.84	40.8	43.4
Possible Phyllosilicate-Rich Terrain: ESP_016918_2030 ESP_017986_2030 (Interval in Earth days: 83)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
22.68	71.0	-0.6	12.29	41.6	43.2
East Rim of Well-Preserved Crater on Rim of Larger Crater: ESP_016971_1610 ESP_017683_1610 (Interval in Earth days: 56)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-18.5	69.1	-0.5	8.387	61.8	65.0
Possible Chlorites and Prehnite in Northern Plains Crater: ESP_016933_2310 ESP_017210_2310 (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
50.48	16.5	4.76	-14.3	43.8	44.8
Thermally Distinct Crater in Arcadia Dorsa: ESP_017097_2340 ESP_017532_2340 (Interval in Earth days: 34)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
53.62	218.	3.64	24.24	44.5	42.0
Eastern Ejecta of Zumba Crater: ESP_017229_1510 ESP_017374_1510 (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
-28.6	227.	-7.4	6.288	71.1	71.1
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