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

Layered Sediments in Valles Marineris: ESP_072546_1725 ESP_072836_1725 (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
-7.53	292.	-2.7	22.00	59.0	56.6
Possible Inverted Channels on Fan Feature: ESP_073059_1600 ESP_073204_1600 (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
-20.0	327.	7.39	22.17	59.8	57.6
Possible Mars Science Helicopter Traverse Route: ESP_072994_1645 ESP_073139_1645 (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
-15.2	301.	2.27	17.70	59.4	57.5
Ridged Landforms in Southern Hellas Region: ESP_072950_1290 ESP_073016_1290 (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
-50.6	68.7	-3.2	-18.4	73.6	73.7
Mound with Layering and Cross-Cutting Bands: ESP_072874_2055 ESP_072808_2055 (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
25.15	336.	-28.	-10.6	60.7	58.3
Layering in Western Arabia Terra: ESP_073071_1910 ESP_073493_1910 (Interval in Earth days: 32)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
11.09	356.	3.51	-5.99	57.5	60.3
Mounds in Utopia Planitia: ESP_072869_2050 ESP_073159_2050 (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
24.71	109.	-1.4	23.09	58.1	58.9
Layering in Western Arabia Terra: ESP_073005_1910 ESP_073150_1910 (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
10.76	358.	-1.3	13.56	57.5	57.0
Hills in Phlegra Montes: ESP_073091_2170 ESP_081478_2170 (Interval in Earth days: 654)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
36.82	163.	27.7	15.69	61.3	57.4
Crater in Arabia Terra: ESP_072965_2175 ESP_073031_2175 (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
37.31	5.86	8.59	-8.55	61.6	63.9
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