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

Tongue-Shaped Features within Alcoves on South Mid-Latitude Crater Wall: ESP_014058_1450 ESP_014335_1450 (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
-34.5	37.1	1.29	-21.3	36.0	39.2
Bright Gully Deposits in Western Hale Crater: ESP_013230_1445 ESP_014074_1445 (Interval in Earth days: 66)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-35.0	322.	8.51	-20.1	39.3	37.8
Wrinkle Ridge in Lunae Palus: ESP_014022_1950 ESP_014167_1950 (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
14.94	294.	-7.9	7.828	48.7	45.9
Distal Ramparts for Fresh Crater Santa Fe in Chryse Planitia: ESP_012795_1995 ESP_013639_1995 (Interval in Earth days: 66)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
19.03	312.	-0.8	-24.0	63.6	57.4
Pasteur Crater Mound with Exposed Layers: ESP_013544_1995 ESP_013610_1995 (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
19.19	24.0	-4.4	-23.3	57.5	57.9
Light-Toned Outcrops Near Crater Rim in Arabia Terra: ESP_014165_1985 ESP_022314_1985 (Interval in Earth days: 635)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
18.07	349.	2.28	28.31	48.4	53.8
Hydrated Minerals and Gully on Central Uplift of Li Fan Crater: ESP_013564_1330 ESP_013709_1330 (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
-46.8	207.	-5.9	5.732	40.8	39.9
A Fan in a Southern Highlands Crater: ESP_014159_1670 ESP_020106_1670 (Interval in Earth days: 464)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-12.7	157.	-7.0	7.119	34.6	56.0
Knobby Terrain in Sinus Meridiani Seen in MOC Image M03-01935: ESP_013756_1850 ESP_021905_1850 (Interval in Earth days: 635)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
4.817	357.	0.67	27.44	45.2	49.2
Gullies on Southwest Slope of Asimov Crater: ESP_012767_1320 ESP_012912_1320 (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
-47.5	4.40	10.5	21.65	47.2	44.3
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