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

Mawrth Region Crater with Possible Sedimentary Features: ESP_025123_2045 ESP_026811_2045 (Interval in Earth days: 131)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
24.24	340.	12.4	-19.9	37.4	44.7
Channels in Northern Arabia Region: ESP_025122_2215 ESP_026177_2215 (Interval in Earth days: 82)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
41.18	6.08	6.88	-8.44	41.6	41.2
Reticulate Bedform and Recent Impact Crater: ESP_025152_1945 ESP_025007_1945 (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
14.48	268.	28.3	15.12	36.7	37.2
Dunes: ESP_025330_1730 ESP_025475_1730 (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
-6.93	93.9	8.60	25.68	48.5	48.7
Banded Terrain in Hellas Region: ESP_025147_1410 ESP_025437_1410 (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
-38.5	55.3	-4.0	23.78	68.2	70.2
Light-Toned Layering along Plains South of Melas Region: ESP_025310_1690 ESP_025455_1690 (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
-10.8	281.	-9.0	9.973	51.7	52.0
Varied Crater Morphologies: ESP_025391_2325 ESP_025470_2325 (Interval in Earth days: 6)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
52.17	220.	4.72	24.81	45.1	43.0
Well-Preserved 8-Kilometer Impact Crater with Central Peak: ESP_025295_2090 ESP_025994_2090 (Interval in Earth days: 54)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
28.72	325.	6.64	-19.1	38.4	41.8
Small Mounds in Chryse Planitia: ESP_025071_1995 ESP_025137_1995 (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
19.39	322.	-4.0	-23.5	38.6	40.7
Fan Below Alcove Cut in Lower Southwest Gale Mound: ESP_025012_1745 ESP_033082_1745 (Interval in Earth days: 629)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-5.47	137.	-15.	4.534	46.0	37.1
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