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

Complex Banded Flow Terrain on Hellas Basin Floor: PSP_007702_1405 PSP_008559_1405 (Interval in Earth days: 67)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-39.2	53.5	1.51	-17.5	71.9	80.6
Wrinkle Ridge in Hesperia Planum: PSP_007726_1560 PSP_008082_1560 (Interval in Earth days: 28)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-23.9	115.	8.10	-3.05	61.0	65.3
Chasma Borealis: PSP_007020_2580 PSP_007178_2580 (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
77.78	292.	0	12.81	69.8	67.1
Mangala Valles: PSP_008118_1645 PSP_008408_1645 (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
-15.5	210.	4.85	15.67	59.6	61.0
8-Kilometer Diameter Rayed Crater: PSP_007757_1605 ESP_016196_1605 (Interval in Earth days: 658)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-19.2	348.	3.29	-18.5	58.6	55.2
Central Peak of Unnamed Crater within the Medusae Fossae Formation: PSP_007870_1830 PSP_009228_1830 (Interval in Earth days: 106)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
3.031	140.	4.36	-20.5	47.0	55.2
Unmantled Central Uplift Feature in Unnamed Crater: PSP_007526_1435 PSP_010875_1435 (Interval in Earth days: 261)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-36.4	178.	4.32	-6.88	67.4	70.7
Debris Flows on Mars: PSP_007033_1445 ESP_016197_1445 (Interval in Earth days: 714)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-34.9	321.	-6.8	8.328	59.9	64.1
3-Kilometer Diameter Crater with Good Bedrock Exposures in Upper Walls: PSP_007892_1865 ESP_079800_1865 (Interval in Earth days: 5603)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
6.625	259.	4.25	-7.35	45.6	54.0
Distal End of Lethe Vallis: PSP_007263_1845 PSP_007553_1845 (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
4.500	156.	-7.8	5.828	42.2	43.6
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