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

Fractured Ground in Arabia Terra: ESP_032704_2155 ESP_032994_2155 (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
34.95	12.2	7.31	26.45	47.7	43.5
Thermokarst: ESP_032872_1405 ESP_040837_1405 (Interval in Earth days: 621)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-39.2	116.	-3.2	-16.8	52.1	41.5
Layered Exposures in Southern Argyre Planitia: ESP_032614_1250 ESP_041225_1250 (Interval in Earth days: 671)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-54.4	323.	-6.5	12.04	58.9	54.9
Light-Toned Deposits in Crater North of Eberswalde Crater: ESP_032706_1575 ESP_040605_1575 (Interval in Earth days: 616)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-22.0	326.	-10.	4.419	39.8	33.3
Gullies in Bogia Crater: ESP_032504_1355 ESP_033150_1355 (Interval in Earth days: 50)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-44.1	83.0	7.64	28.51	48.7	58.4
Rugged Banded Material in Crater in Northwest Hellas Planitia: ESP_032769_1420 ESP_033191_1420 (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
-37.7	47.8	-0.0	-19.1	49.1	57.3
Columnar Jointing in Crater Wall: ESP_032741_2040 ESP_032886_2040 (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
23.59	84.4	-1.3	12.77	41.2	39.2
Possible Mars 3 Landing Site: ESP_032737_1345 ESP_032447_1345 (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
-45.0	202.	5.6	-16.6	53.3	49.8
Bright Dunes in Syria Planum: ESP_032814_1670 ESP_032880_1670 (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
-12.8	254.	22.5	-0.47	35.1	37.6
Well-Preserved Impact Crater: ESP_032563_1370 ESP_032708_1370 (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
-42.4	271.	12.0	23.43	48.2	50.0
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